high energy density physics with intense ion beams

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8/20/2019 High Energy Density Physics With Intense Ion Beams http://slidepdf.com/reader/full/high-energy-density-physics-with-intense-ion-beams 1/20 High energy density physics with intense ion beams Boris Yu. Sharkov  a ,e , Dieter H.H. Hoffmann  b ,e,f, *, Alexander A. Golubev  c,e , Yongtao Zhao  d,a FAIR GmbH: Facility for Antiproton and Ion Research in Europe GmbH, Planckstra  ß e 1, 64291 Darmstadt, Germany b  Institut fu¨ r Kernphysik, Technische Universit at Darmstadt, Schlossgartenstrasse 9, 64289 Darmstadt, Germany c State Scientific Center Russian Federation  e Institute for Theoretical and Experimental Physics of National Research Center  Kurchatov Institute (SSC RF  ITEP of NRC  Kurchatov Institute), FSBI SSC RF ITEP, Bolshaya Cheremushkinskaya, 25, 117218 Moscow, Russia d School of Science, Xian Jiaotong University and Institute of Modern Physics, CAS, Xianning West Road 28#, Xi an 710049, PR China e  National Research Nuclear Univer sity MEPhI, Moscow, Russia N ational Research Nuclear Univers ity «  MEPhI »  , Kas hirskoe shosse, 31, 1 15409 Moscow, Russ ia  Institute of Modern Physics, CAS, Lanzhou 730000, PR China Received 18 November 2015; revised 30 November 2015; accepted 30 November 2015 Available online  ▪ ▪ ▪ Abstract We review the development of High Energy Density Physics (HEDP) with intense heavy ion beams as a tool to induce extreme states of matter. The development of this field connects intimately to the advances in accelerator physics and technology. We will cover the generation of intense heavy ion beams starting from the ion source and follow the acceleration process and transport to the target. Intensity limitations and potential solutions to overcome these limitations are discussed. This is exemplified by citing examples from existing machines at the Gesell- schaft fu ¨r Schwerionenforschung (GSI-Darmstadt), the Institute of Theoretical and Experimental Physics in Moscow (ITEP-Moscow), and the Institute of Modern Physics (IMP-Lanzhou). Facilities under construction like the FAIR facility in Darmstadt and the High Intensity Accelerator Facility (HIAF), proposed for China will be included. Developments elsewhere are covered where it seems appropriate along with a report of recent results and achievements. Copyright  ©  2016 Science and Technology Information Center, China Academy of Engineering Physics. Production and hosting by Elsevier B.V. This is an open access article under the CC BY-NC-ND license ( http://creativecommons.org/licenses/by-nc-nd/4.0/ ). PACS codes:  52.25.Os; 52,38.Mf; 52,38.Ph; 52.40.Db; 52.50.Gj; 52.58.Hm; 52.59.-f Keywords: High energy density physics; Ion driven fusion; Warm dense matter 1. Introduction This millennium experienced a fast-paced development of High Energy Density Physics (HEDP). This evolved parallel to the advancements in driver technology. Most prominent is the development of high power and high-energy lasers, where the National Ignition Facility (NIF) is an outstanding example [1e3]. Also pulsed power devices like the Z-Machine at Sandia National Laboratory, Albuquerqe, and Angara-5-1 in Troitsk reported towering progress [4e8]. Along with laser and pulsed power devices, high explosives [9,10] and intense particle beams [11e13] are suitable and commonly used drivers to induce high energy density states. The expressions High Energy Density-matter, Hot Dense Matter or Warm Dense Matter (WDM) are often used interchangeably and are not defined unambiguously; however, we are talking about matter of temperature at least in the eV/k B -regime and above (where k B  is the Boltzmann constant, which we will omit in future when we talk about a temperature stated in eV). The density is about solid-state density and higher, and finally owing to these parameters, depending on the equation of state of the material, the pressure is above the GPa range. Thus * Corresponding author. Institut fu ¨r Kernphysik, Technische Universit at Darmstadt, Schlossgartenstrasse 9, 64289 Darmstadt, Germany. E-mail address:  [email protected] (D.H.H. Hoffmann). Peer review under responsibility of Science and Technology Information Center, China Academy of Engineering Physics. Please cite this article in press as: B.Y. Sharkov, et al., High energy density physics with intense ion beams, Matter and Radiation at Extremes (2016), http:// dx.doi.org/10.1016/j.mre.2016.01.002  Available online at www.sciencedirect.com ScienceDirect Matter and Radiation at Extremes xx (2016) 1e20 MATTER AND RADIATION AT EXTREMES www.journals.elsevier.com/matter-and-radiation-at-extremes +  MODEL http://dx.doi.org/10.1016/j.mre.2016.01.002 2468-080X/Copyright  © 2016 Science and Technology Information Center, China Academy of Engineering Physics. Production and hosting by Elsevier B.V. This is an open access article under the CC BY-NC-ND license ( http://creativecommons.org/licenses/by-nc-nd/4.0/).

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Page 1: High Energy Density Physics With Intense Ion Beams

8/20/2019 High Energy Density Physics With Intense Ion Beams

http://slidepdf.com/reader/full/high-energy-density-physics-with-intense-ion-beams 1/20

High energy density physics with intense ion beams

Boris Yu. Sharkov  a,e, Dieter H.H. Hoffmann  b,e,f ,*, Alexander A. Golubev  c,e, Yongtao Zhao  d,f 

a FAIR GmbH: Facility for Antiproton and Ion Research in Europe GmbH, Planckstra ß e 1, 64291 Darmstadt, Germanyb  Institut fu r Kernphysik, Technische Universit €at Darmstadt, Schlossgartenstrasse 9, 64289 Darmstadt, Germany

c State Scientific Center Russian Federation  e  Institute for Theoretical and Experimental Physics of National Research Center   “Kurchatov Institute”   (SSC RF 

 ITEP of NRC   “Kurchatov Institute”), FSBI SSC RF ITEP, Bolshaya Cheremushkinskaya, 25, 117218 Moscow, Russiad School of Science, Xi' an Jiaotong University and Institute of Modern Physics, CAS, Xianning West Road 28#, Xi ' an 710049, PR China

e  National Research Nuclear Univer sity MEPhI, Moscow, Russia N ational Research Nuclear Univers ity « MEPhI » , Kas hirskoe shosse, 31, 1 15409 Moscow, Russ iaf  Institute of Modern Physics, CAS, Lanzhou 730000, PR China

Received 18 November 2015; revised 30 November 2015; accepted 30 November 2015

Available online   ▪ ▪ ▪

Abstract

We review the development of High Energy Density Physics (HEDP) with intense heavy ion beams as a tool to induce extreme states of 

matter. The development of this field connects intimately to the advances in accelerator physics and technology. We will cover the generation of 

intense heavy ion beams starting from the ion source and follow the acceleration process and transport to the target. Intensity limitations and

potential solutions to overcome these limitations are discussed. This is exemplified by citing examples from existing machines at the Gesell-

schaft fur Schwerionenforschung (GSI-Darmstadt), the Institute of Theoretical and Experimental Physics in Moscow (ITEP-Moscow), and the

Institute of Modern Physics (IMP-Lanzhou). Facilities under construction like the FAIR facility in Darmstadt and the High Intensity Accelerator

Facility (HIAF), proposed for China will be included. Developments elsewhere are covered where it seems appropriate along with a report of 

recent results and achievements.

Copyright ©

 2016 Science and Technology Information Center, China Academy of Engineering Physics. Production and hosting by ElsevierB.V. This is an open access article under the CC BY-NC-ND license ( http://creativecommons.org/licenses/by-nc-nd/4.0/ ).

PACS codes:   52.25.Os; 52,38.Mf; 52,38.Ph; 52.40.Db; 52.50.Gj; 52.58.Hm; 52.59.-f 

Keywords: High energy density physics; Ion driven fusion; Warm dense matter

1. Introduction

This millennium experienced a fast-paced development of 

High Energy Density Physics (HEDP). This evolved parallelto the advancements in driver technology. Most prominent is

the development of high power and high-energy lasers, where

the National Ignition Facility (NIF) is an outstanding example

[1e3]. Also pulsed power devices like the Z-Machine at

Sandia National Laboratory, Albuquerqe, and Angara-5-1 in

Troitsk reported towering progress   [4e8]. Along with laser

and pulsed power devices, high explosives  [9,10]  and intense

particle beams   [11e13]   are suitable and commonly useddrivers to induce high energy density states. The expressions

High Energy Density-matter, Hot Dense Matter or Warm

Dense Matter (WDM) are often used interchangeably and are

not defined unambiguously; however, we are talking about

matter of temperature at least in the eV/k B-regime and above

(where k B   is the Boltzmann constant, which we will omit in

future when we talk about a temperature stated in eV). The

density is about solid-state density and higher, and finally

owing to these parameters, depending on the equation of state

of the material, the pressure is above the GPa range. Thus

*   Corresponding author. Institut fur Kernphysik, Technische Universit€at

Darmstadt, Schlossgartenstrasse 9, 64289 Darmstadt, Germany.

E-mail address:  [email protected] (D.H.H. Hoffmann).

Peer review under responsibility of Science and Technology Information

Center, China Academy of Engineering Physics.

Please cite this article in press as: B.Y. Sharkov, et al., High energy density physics with intense ion beams, Matter and Radiation at Extremes (2016), http:// 

dx.doi.org/10.1016/j.mre.2016.01.002

 Available online at  www.sciencedirect.com

ScienceDirect 

Matter and Radiation at Extremes xx (2016) 1e20

MATTER AND RADIATION

AT EXTREMES

www.journals.elsevier.com/matter-and-radiation-at-extremes

+   MODEL

http://dx.doi.org/10.1016/j.mre.2016.01.002

2468-080X/Copyright  ©  2016 Science and Technology Information Center, China Academy of Engineering Physics. Production and hosting by Elsevier B.V. Thisis an open access article under the CC BY-NC-ND license ( http://creativecommons.org/licenses/by-nc-nd/4.0/ ).

Page 2: High Energy Density Physics With Intense Ion Beams

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matter with such properties takes up a large area of the

respective phase diagram, and is of interest in diverse domains

of physics, such as astrophysics, planetary physics, power

engineering, controlled thermonuclear fusion, material science

and more.

The National Ignition Campaign [14] was supposed to show

ignition of a fusion target in the laboratory by the end of 2012.However, even though the laser worked perfectly up to the

design parameters and even outperformed them with respect to

the total energy delivered to the target, ignition of the fusion

target did not occur. Of course one may debate that the fusion

energy output measured in terms of neutron yield [15], which

is on the order of some 10 kJ, is equivalent to the energy that

finally reaches the compressed fuel, and therefore in some

respect one may speak of scientific breakeven. The reason why

ignition did not occur is still under debate within the scientific

community and most probably a number of sources play a role,

among them turbulent mix of the fuel during the compression

phase. During the compression phase the fuel heats up and

passes through the Warm Dense Matter regime. Here the

properties of matter as expressed by an Equation of State

(EOS) are widely unknown. In the high compression regime

we have to deal with degenerate matter. Energy loss of charged

particles in degenerate matter is practically unexplored, which

was pointed out by RD Petrasso in his Teller-award lecture

during IFSA 2013 at Nara, Japan (International Conference on

Inertial Fusion Science and Applications).

Since the perspectives of fusion energy are very important

and very promising, we think it is time to review alternative

inertial fusion driver concepts. Such an alternative to intense

laser beams is constituted by intense high energy heavy ion

beams. They can be produced efficiently, where the conversionof electric power to kinetic energy of heavy ions is on the

order of 25% and accelerators by design work at high repe-

tition rate. Thus swift, heavy ions are very efficient carriers of 

energy. Moreover their specific interaction properties also

make them ideal candidates to generate high energy densities

in matter.

2. Accelerator issues of high energy density physics

2.1. High current ion sources

As well as even the longest journey starts with the first step

(Chinese wisdom), an efficient accelerator depends on the ion

source and here we start our discussion.

Inertial Fusion Energy (IFE) and similarly the generation

of high energy density matter generated by ion beams require

considerably more ions per pulse, than classical ion sources

are able to deliver   [16]. One way to overcome this problem

was the suggestion that was already made in the early system

studies for heavy ion driven fusion like HIBALL (Heavy Ion

Beams and Lithium Lead) and HIDIF (Heavy Ion Driven

Ignition Facility)  [17e19]. It was proposed to have multiple

ion sources, and to increase the intensity by beam funneling

as shown in Fig. 1. This of course causes the beam emittance

to grow, which we will discuss later. Alternative solutions to

decrease the number of funneling stages, as well as the ne-

cessity to overcome the Child Langmuir space charge limi-

tations, had to be investigated. In a conventional electron- or

ion source (see  Fig. 2) the current density  J   is limited to

 J fU 3=2

d 2  ð1Þ

where   U   is the extraction voltage and d is the gap distance

between the ion source electrodes. For a given gap distance the

voltage U  is limited by the electric breakdown, which leads to

a general limit for a given geometry. Laser-produced plasmas

may partially overcome this limit. Today high power laserinteraction with plasma does generate intense high energy

particle beams [20e22]. However, these kinds of beams have

not yet been effectively coupled to accelerator structures.

Several institutes are currently working on this problem,

among them CERN and GSI-Darmstadt. On the other hand

laser generated plasmas have been used very efficiently as ion

sources. One of the first examples is the laser plasma ion

source at CERN   [23]. This ion source was later moved to

Fig. 1. Multiple ion sources and beam funneling to achieve high intensity as

proposed by the HIDIF study  [18,19].

Fig. 2. Schematic set-up of a plasma ion source. The ions are emitted from the

concave plasma sheath, which forms an equipotential surface.

2   B.Yu. Sharkov et al. / Matter and Radiation at Extremes xx (2016) 1e20

+   MODEL

Please cite this article in press as: B.Y. Sharkov, et al., High energy density physics with intense ion beams, Matter and Radiation at Extremes (2016), http:// 

dx.doi.org/10.1016/j.mre.2016.01.002

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ITEP-Moscow, where it served for many years as ion source

for highly charged ions [24]. The original CO2  laser was later

tried to be replaced by an Nd-laser to produce helium like ions

up to medium and high Z-targets, however, there was no sig-

nificant advantage with respect to technology and repetition

rate, thus for the whole project the CO2   laser was used. The

expanding laser plasma (see Fig. 3) is funneled by an aperturesystem into the extraction system operated at 120 kV and an

adjacent low energy beam transport system with gridded

electrostatic lenses. A final double aperture simulates the

acceptance of the RFQ-accelerator section (Radio-Frequency-

Quadrupole). The expanding plasma is still quasi-neutral.

However, after the extraction system there exists a beam

with space charge. In order to match this beam to the accel-

erator structure, space charge compensation by injecting

electrons from a thermionic tungsten cathode was applied. By

this technique a current density increase of up to a factor of 25

was achieved   [25]. H. Riege and co-workers (1998) used

electron beams emitted from ferroelectric materials for space

charge neutralization with pulsed electron beams   [65]. Even

though the offline experiments showed very good results, this

technique never entered the testing phase in an actual accel-

erator [65]. A typical charge state spectrum obtained for Pb is

shown in Fig. 4, with the most intense charge state Pb27þ and

Pb28þ. A similar charge state spectrum is obtained from

stripping lead ions at an energy of 1.4 MeV/u after a gas

stripper. This is the situation which is common at the GSI

accelerator where a stripping section exists at 1.4 MeV/u after

a total acceleration length of about 50 m, which is necessary

for a powerful low energy accelerator system to handle ions of 

low charge state. The advantage of a laser-plasma ion source is

thus obvious. In the example shown in Fig. 4, a CO2-laser of 92.5 J and a power density of  P ¼  3   1013 (W cm2), with

the parameters indicated there was used. For non-resonant

photoionization the laser intensity   I   necessary to obtain the

charge state distribution with a maximum charge state q of an

element with atomic number Z and ionization energy  E ion( Z )

is approximately given by:

 I 

 W

cm2

z4 109E ionð Z Þ4

q2  :   ð2Þ

The charge state spectrum, under the assumption of local

thermal equilibrium in the expanding laser plasma, represents

the relative abundance of ionization states given by the Saha

equation, where   n zþ1

n zis the ratio of the particle numbers in

different ionization states   z   and   zþ1. This ratio is then

multiplied by the electron density  ne:

n zþ1ne

n z

¼ g zþ1

g z

$eW izkT $

2m3

e

1=2

p2Z3  $

Z ∞0  ffiffiffiffi

E p   $e

E kT dE 

¼ g zþ1

g z

$2ð2pmekT Þ3=2

h3  e

W izkT  ð3Þ

Fig. 3. Laser Plasma ion source at CERN and ITEP.

Fig. 4. Charge state distribution of Laser-plasma ion source, generated from

irradiation of a Pb target with CO2 laser. The laser parameters are indicated in

the figure.

3 B.Yu. Sharko v et al. / Matter and Radiation at Extremes xx (2016) 1e20

+   MODEL

Please cite this article in press as: B.Y. Sharkov, et al., High energy density physics with intense ion beams, Matter and Radiation at Extremes (2016), http:// 

dx.doi.org/10.1016/j.mre.2016.01.002

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In this equation g are the statistical weights of the quantum

states,  W iz  is the ionization energy,  me   is the electron mass at

rest,  k  is the Boltzmann constant,   Z ¼   h2p

  is Planck 's constant

divided by 2p, and   T   the temperature. In the expanded laser

plasma this equation approximately presents the situation.

Observed deviations from the charge state ratio point to a

situation which is not fully in equilibrium. Moreover the ioncharge state distribution does not remain   “frozen”   during

plasma expansion as long as the density is high enough to

allow for three-body recombination. This process, however

scales with   n2e . Therefore at the later stage of expansion, the

equilibrium is determined by collisional ionization and radi-

ative recombination, a situation which is called corona

equilibrium.

At the GSI radio frequency quadrupole accelerator RFQ-

Maxilac matching of a laser ion source to this accelerator was

demonstrated [26]. A 1 0 J /  ms CO2 laser has been used to produce

a hot plasma plume, from which highly charged tantalum ions

were emitted. For the charge state Ta10þ a current of 1.8-mAwas

measured after acceleration to 45 keV/u.

Laser-plasma ion sources are today used in many places,

Refs.   [27,28]   give just two examples of currently ongoing

research in this field.

2.2. Low energy beam transport 

Space charge limitations are especially serious at low en-

ergy. Therefore special attention is necessary to match the low

energy beam, which was produced from the ion source, to the

low energy accelerator section. In 1979 Alfred Maschke at

Brookhaven National Laboratories developed a set of equa-

tions to determine the transport limit for a generalized linear

accelerator [29]. The current density J is thus determined by:

 J 

mA

cm2

f

 A

 Z ðbgÞ3

:   ð4Þ

This equation shows that at low energy the beam is severely

subjected to space charge, and strong focusing forces are

necessary to overcome this effect. Therefore the invention of 

radiofrequency quadrupole focusing and acceleration (RFQ)

by Kapchinsky and Teplakov in 1970 [30], represented a major

progress to increase the beam intensity of particle accelerators.

Later under the guidance of Kapchinsky and Koshkarev at

ITEP in Moscow   [59,60], and even a bit later at GSI Darm-stadt under the leadership of R. Muller [31] RFQ accelerators

for heavy ions were built and used for early high energy

density physics experiments. The machine at GSI was

designed to accelerate heavy ions up to an energy of 45 keV/u.

The accelerator was called MAXILAC and was used to

generate the first heavy-ion beam induced plasma with a

temperature of 0.75 eV.

Phase space limitations are not only a concern during low

energy transport. Intensity limitations are less restrictive at

high energy due to the scaling proportional to (bg)3, as indi-

cated in Eq. (4). At the end of the linear acceleration the beam

is injected into the synchrotron. At GSI-Darmstadt this is a

synchrotron for beams with a maximum rigidity of 18 Tm. If 

the beam may be described by a distribution function  f ( x,v,t ),

which fulfills the conditions of kinetic plasma theory, that is,

we deal with non-interacting particles and local thermal

equilibrium then we obtain the Vlasov equation with

d f ð x;

v;

t Þdt  ¼ 0   ð5Þ

The physical interpretation of this result is, that a particle in

a considered volume does not experience any change of the

distribution function in its local frame of reference as long as it

is subjected to conservative (non-dissipative) forces only. This

amounts to the fact that the local distribution function is

conserved, and it is an invariant. This holds equally true for the

phase space and this result is also known as the Liouville

theorem (Conservation of phase space), which has direct

consequences for the beam properties.

2.3. Multi-turn injection and Liouville limitations

For most experiments and applications that request high

intensities, especially for high energy density plasma physics,

the beam is first accumulated in the synchrotron by filling it

over many turns before it is accelerated (see   Fig. 5). This

technique is known as multi-turn injection. Due to the above

mentioned Liouville theorem it is not possible to inject into an

already occupied phase space volume for a second time

without losing the particles. This means that the phase space

ellipsoid of the injected beam must be well adapted to the

partial ellipsoids that are already present inside the machine.

The phase space matching is done using the beam transport

system before injection (Fig. 5(b)). The equilibrium trajectory(shown in red) is disturbed by means of a number of bumper

magnets (in Fig. 5 two are shown). They cause a local bump

and deviation from the ideal trajectory. The SIS-18 injection

system uses a total of four bumper magnets located close to

the septum magnet. The magnitude of deflection is maximum

at the start of the injection process and is gradually tuned to

zero. As indicated in   Fig. 5(c), the acceptance of the syn-

chrotron (150 mm mrad) shown as red ellipse is filled from the

inside to the outer rim. This method requires, that the emit-

tance of the injected beam is smaller than the acceptance of 

the synchrotron (transverse stacking method).

The intensity and beam quality obtained by multiturn in-

 jection is not sufficient for a cost effective inertial fusion

driver based on rf-linac and synchrotron. A more effective

stacking method therefore was tested at the Terawatt Accu-

mulator of ITEP-Moscow (TWAC) [32]. This method is based

on   Non-Liouvillian Stacking  by Charge exchange injection.

To overcome the limitations set by the Liouville theorem

the circulating particles and the injected particles are of 

different species, thus they are allowed to occupy the same

phase space volume. This is possible by changing the charge

state of the injected species when the injected beam is com-

bined with the circulating beam. The original idea of G.I

Budker in1963 was put forward on an accelerator conference

and was later published in a journal [33]. The process was first

4   B.Yu. Sharkov et al. / Matter and Radiation at Extremes xx (2016) 1e20

+   MODEL

Please cite this article in press as: B.Y. Sharkov, et al., High energy density physics with intense ion beams, Matter and Radiation at Extremes (2016), http:// 

dx.doi.org/10.1016/j.mre.2016.01.002

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tested with H1þ circulating in a storage ring with weak 

focusing. The injected beam was neutral hydrogen H0þ. After

H0þ and H1þ were combined both species had to pass a gas jet

serving as stripper target. The stripping process yields a

combined pulse of   H 1þ. The same scheme may in principle

also applied for heavy ions. However, the stripping process at

the stripper target usually results in the production of a charge

state spectrum and hence results in a loss of beam intensity. A

different situation arises when the energy of the circulating

and injected beam is high enough that stripping produces

predominantly fully ionized ions. This situation is depicted in

Fig. 6. The incoming beam  Z qþ consists of the ion species Zwith charge state qþ. The nuclear charge of these ions is also

 Z   and we have the condition   q ( Z, which means that   q   is

smaller, but in the vicinity of  Z . Therefore a high charge state q

is already necessary, which may be obtained by a laser-plasma

ion source or by an ECR-source (Electron Cyclotron Reso-

nance) [66]. In  Fig. 6 the dashed red circle represents the ideal

trajectory of the fully stripped circulating beam. At the in-

 jection the beam is in a lower charge state, ideally helium like.

In the overlap region the fully stripped and the helium like

beam occupy the same phase space. In a thin stripper foil the

helium like beam is transformed to the fully ionized state. The

stripper foil must be sufficiently thin, in order to minimizebeam degradation during the stacking process. This case was

successfully realized at the ITEP-TWAC accelerator system

[32,34]. The scheme is shown in  Fig. 7. The accelerator sys-

tem at ITEP consists of two rings. In the UK booster ring the

respective ions are accelerated to a maximum energy of 

0.7 GeV/u and then transferred to the U-10 accumulator ring.

In this ring already bare nuclei are circulating. After the

transfer from the booster ring where ions are not yet fully

stripped to the accumulator ring, ions are injected into the

same phase space volume as the already circulating, fully

stripped ions. Then both bunches pass the stripper target and

after the stripper target all ions with minimal loss of intensity

and energy are fully stripped. The inset of   Fig. 7   shows the

example of Carbon at 213 MeV/u and the accumulation of intensity after each injection step. The final intensity is

approximately N ions z (4   5)   1010.

The laser-plasma ion source described above was used to

produce helium like charge states C4þ, S16þ, Ca18þ, and

Co25þ.The maximum stripping energy was 0.7 GeV/u. In the

ideal case one would use lower charge states due to space

charge considerations. In fusion scenarios even  Pb1þ or  Bi1þ

are discussed. In this case one needs a very powerful laser to

resonantly ionize to charge state 2þ. Such lasers are currently

not available to produce intense beams, but there is certainly a

development path. Finally the limit for the maximum intensity

is set by the appearance of beam instabilities, like:

2.4. Incoherent tune shift limit 

Ion driven inertial fusion, as well as experiments of High

Energy Density physics require highest beam intensities.

Therefore a synchrotron has to be operated up to the space

charge limit. As shown in  Fig. 8, this limit was reached for

moderately heavy ions up to   58Ni14þ   and   86Kr34þ   already in

1999. This amounts to approximately (3 4) 1010 particles

of this ion species per ion pulse. For Uranium ions of charge

state 73þ   this limit has not yet been reached. Before we

discuss the reasons let us take a quick look at the physics

Fig. 5. Basic principle of multi-turn injection (a): Synchrotron SIS-18 at GSI-Darmstadt; (b) orbit bump at beam injection with 2 kicker magnets; (c): blow up of 

phase space due to multi-turn injection.

Fig. 6. Schematic set-up of non-Liouville charge-changing injection.

5 B.Yu. Sharko v et al. / Matter and Radiation at Extremes xx (2016) 1e20

+   MODEL

Please cite this article in press as: B.Y. Sharkov, et al., High energy density physics with intense ion beams, Matter and Radiation at Extremes (2016), http:// 

dx.doi.org/10.1016/j.mre.2016.01.002

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underlying this space charge limit. The Coulomb repulsion,

due to the positive charge of the ions constituting the beampulse, is offset by focusing forces of the electromagnetic

quadrupoles. Close to the ideal trajectory of the beam the

focusing force increases linearly with the distance from the

beam center. The individual beam particles, however, do not

follow the ideal trajectory, but they do perform oscillations as

shown in the schematic drawing of   Fig. 9. If the number of 

betatron oscillations per circulation (Q) is an integer or close

to it, the particle will come to the same position after an

integer number m of circulations. The resonance condition is

m$Q  ¼   integer.Thus any positioning error of the beam

transport system will amplify and the beam is lost within a

few circulations. Therefore the number   Q   of betatron oscil-

lations must be chosen carefully to stay off any of these

resonances. An increase in beam intensity tends to reduce the

number of betatron oscillations and hence a shift  DQ  occurs.

If this shift causes a resonance condition, the beam experi-

ences a resonance condition and is lost. In heavy ion syn-

chrotrons the beam is stored only for a relatively short time

during multi-turn injection, therefore a tune shift of up to

DQ   z   0.5 is possible   [36]. The reason why until now thespace charge limits for heavy ions at low charge state has not

yet been reached is due to the problem of the dynamic

vacuum.

2.5. Dynamic vacuum

Up to very recently (2014) all experiments at the High

Energy Density Physics area at GSI were performed with a

maximum of 4    109 beam ions. The bunch length may

presently be varied between 80 ns (minimum, lower intensity)

and 120 ns (maximum intensity). A higher intensity for U73þ

was achieved in 2014 by measures that we will discuss here.

Eventually, even still higher intensities may be expected for a

lower charge state e.g. U28þ. However the problems encoun-

tered with the higher charge state will turn out to be even more

severe in the low charge state case. To prove the feasibility,

experiments at the SIS-18 were conducted to test high in-

tensity uranium operation with low charge states [37]. During

these injection experiments, a varying number of U28þ-parti-

cles up to 7.4109 were injected and stored at the injection

energy of 11.4 MeV/u. The results (see   Fig. 9) showed

extremely fast and intensity-dependent particle losses.

Fig. 7. Non-Liouville injection at ITEP with Carbon ions at 213 MeV/u. The stripping process takes C 4þto fully ionized C6þ.

Fig. 8. Incoherent space charge limit of SIS-18 at GSI-Darmstadt. This limit

has been reached up to medium heavy ions, but not yet for the most heavy ion

species like Uranium (charge state 73þ)  [35].

Fig. 9. Beam transport of a synchrotron (FODO). Beam ions are undergoing a

number of Q betatron oscillations. An increasing number of particles decreases

the number of oscillations and the beam is lost due to arising instability.

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Moreover the more intensity was injected, the faster the beam

was lost as can clearly be seen from   Fig. 10. With this in-

 jection experiment the pressure at various locations of the

synchrotron was measured. This required the possibility of fast

pressure measurements. Simultaneously with the loss of beam

a dynamic increase in the residual gas pressure was observed.

Therefore we concluded that the beam was not lost due tospace charge instabilities since the intensity was still well

below this limit. The effect was, however, a result of desorp-

tion effects. The inset of  Fig. 10 shows schematically a section

of the synchrotron with a bending magnet. Even at ultra-high

vacuum conditions there are still 106 107 particles per cubic

centimeter. Charge changing collisions have a high cross

section and therefore the probability of a collision that results

in a change of charge state of the beam ion is quite high. If 

such a collision occurs, the ion is removed from the ideal

trajectory and will hit the beam pipe at some later position.

Kinetic energy of the beam ion is deposited into the surface of 

the beam pipe where a multitude of molecules are adsorbed.

The sudden input of energy causes desorption and per original

beam ion up to 10,000 desorbed ions may be released into the

vacuum of the synchrotron. Thus more beam-ions undergo a

charge changing collision, which sets off an avalanche with

the consequence of total beam loss. Ultrahigh vacuum is

therefore mandatory for high intensity heavy-ion synchrotrons

and it is the main reason for superconducting magnets, since

the cold surface also serves as a cryo-pump to keep the vac-

uum low. Currently sticking coefficients are measured to gain

more knowledge about adsorption and absorption effects. The

results will help to design optimum parameters for the FAIR

facility, which is under construction. Therefore, a quantitative

description of the observed effects, which affect the lifetime of intermediate charged ion beams need to include calculation of 

the interaction of the beam particles with rest gas molecules/ 

atoms and particle trajectories with aperture limits in the ring

structure.

A design concept for the SIS-100 synchrotron of the FAIR

facility must have residual gas pressure stabilization. The idea

was to develop a dedicated ion catcher system and strong

pumping of cold surfaces where effects of desorption are ex-

pected to occur. Thus a careful analysis of the beam transport

system and proper alignment of all magnets is paramount to

the success. Then it is possible to place a properly designed

system of catchers at places with high desorption probability.

This was done by Lars Bozyk in his thesis work:   “Design

and test of a prototype cryo-collimator to control the dynamicvacuum problem” [38]. This collimator must be placed at the

appropriate position, indicated in Fig. 11. Moreover the angle

of incidence should be as close to 90  as possible, in order to

minimize desorption effects.

The result of the design study is shown in  Fig. 12.

Currently this model has been tested and designed and a

number of these collimators have been ordered to be built into

the SIS-100 at FAIR.

Once the intense beam is in the synchrotron it has to be

extracted and transported to the experiment. In order to do this

without beam loss a very efficient beam diagnostic is neces-

sary, which we will discuss in the following section.

2.6. Non-interceptive beam diagnostic

The most applied method to do beam diagnostic of intense

beam is associated with beam induced fluorescence (BIF). A

BIF-monitor exploits fluorescence light emitted by residual

gas molecules after atomic collisions with beam ions.

Fluorescence-images are recorded with an image-intensified

camera system, and beam profiles are obtained by projecting

these images. Such monitors are already in operation at GSI's

LINAC since some years ago   [39]. However, this method

needs further investigation and development, to employ it also

for high intensity accelerators as the new machines under

construction at the moment.

We will here present a different non-invasive diagnostic

method for the experimental determination of the transverse

profile of an intense ion beam which is called electron beam

imaging (EBI). This technique has been developed and was

investigated theoretically as well as experimentally for

employment at the FAIR facility. The method is based on the

deflection of electrons passing the potential generated by an

ion beam (Fig. 13). To achieve this, an electron beam is

generated with a specifically prepared transversal profile.

This distinguishes this method from similar ones which

use thin electron beams for scanning the electromagnetic

field   [40]. First of all the influence of the electromagneticfield of the ion beam on the electrons has been analyzed

theoretically. It was found that the magnetic field causes a

shift of the electrons along the ion beam axis, while the

electric field causes a shift in a plane transverse to the ion

beam. Moreover, in the nonerelativistic case the magnetic

force is significantly smaller than the Coulomb one and the

electrons experience a shift due to the magnetic field and

continue to move parallel to their initial trajectory. Under the

influence of the electric field   E  x, y, the electrons are pushed

off from the ion beam axis, their resulting trajectory shows a

specific angle   q   compared to the original direction. This

deflection angle practically depends just on the electric field

Fig. 10. Injection into the SIS-18 with varying intensities. At the highest in-

 jection intensity the beam's lifetime in the synchrotron is the lowest.

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of the ion beam. Thus the magnetic field has been neglected

when analyzing the experimental data. The deflection angle

follows from:

dv x; y

dt   ¼  e

me

E  x; y/q¼ v y

v x

/q¼   e

mev x Z   E  y

v x

d x;   ð6aÞ

and

v x ¼ ffiffiffiffiffiffiffiffi

2E o

me

r   ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi1þE p

E o

s   /

with E o[E p

/q

¼   e

2E o

Z   E  yd x   ð6bÞ

In these equations v  is the non-relativistic electron velocity,

E  x, y   the electric field components,   E o   is the non-relativistic

kinetic energy of the electron and finally   E p   is the potential

energy of the electron in the field of the ion beam [41].

The theoretical model provides a relationship between the

deflection angle of the electrons and the charge distribution in

the cross section of the ion beam. The model however, can

only be applied for small deflection angles. This implies a

relationship between the lineecharge density of the ion beam

and the initial kinetic energy of the electrons (Method is

shown in Figs. 13 and 14).

Numerical investigations have been carried out to clarify

the application range of the EBI diagnostic method and to

benchmark the theoretical model. Different charge distribu-

tions were considered and the simulation results have been

compared with the theoretical model. Numerical investigations

have shown a very good agreement with the theoretical model

for deflection angles up to 20 mrad. This value defines the

limit for the applicability of the theoretical model. Moreover,

the magnetic field of the ion beam has also been taken into

account in the simulations. The results show that at high ion

beam currents   d   starting at about 1 A   d   the electrons

experience a non-negligible displacement along the ion beam

axis, which has to be taken into consideration in experiments

with intense heavy ion beams. The electrons suffer practically

Fig. 11. Calculated (Strahlsim) trajectories of ions that undergo charge-change collisions (red). Here U 28þ / U 29þ [37,38]. The beam envelope is in yellow.

Fig. 12. Design of a cryo-collimator to minimize the effect of desorbed gas in the SIS-100.

Fig. 13. The electron beam passes a magnetic field (half quadrupole) to achieve a transversal line profile.

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the same displacement under the influence of the magnetic

field, regardless of their offset. At an offset of 10 mm the

deviation from the shift at the ion beam axis is less than 3%.For the experimental investigations of the EBI diagnostic

method an offline experiment had been set up at the HHT

experimental area at GSI in Darmstadt. The Coulomb field of 

the ion beam had been simulated by electrostatically charged

wires. In case of a single wire, the experimental results are in

good agreement with the theoretical model for deflection an-

gles up to 20 mrad. This confirms the results of the numerical

studies. To simulate the field within an ion beam, several wires

have been clamped parallel to each other within a plane

perpendicular to the electron beam. The electrons thus could

pass through the spaces between the wires. The results of these

experiments have quantitatively confirmed the prediction of 

the theoretical model that the derivative of the deflection angle

with respect to the offset is proportional to the charge distri-

bution in the cross section of the ion beam. Quantitatively,

however, deviations from the theoretical model have been

observed, which can be explained by the imprecise modeling

of the charge distribution of an ion beam by the charged wires.

The EBI diagnostic method has been applied for the first

time in collaboration with the group of Professor Ulrich Rat-

zinger at the FRANZ accelerator at the Goethe University

Frankfurt am Main for loweenergy, DC ion beams  d  H 4eþ

at 13.5 keV and a current of approximately 1 mA.

The transverse charge distribution of these beams has been

successfully determined by this diagnostic method. The resultsare displayed in Fig. 15. It is a difficult procedure, but we are

sure that this method will be very useful to diagnose intense

ion-beams at future high intensity accelerators.

Once the intense ion beam is available from the accelerator

and can be diagnosed along the beam-transport system to the

target without loss, it must be focused in order to achieve high

energy density. Due to the high magnetic rigidity focusing of 

ion beams is a larger challenge than the focusing of high en-

ergy electrons. Superconducting magnets are envisioned as a

final focus system at FAIR. However previous experiments

showed that plasma technology may show another solution to

the focusing problem.

3. Beam plasma interaction

3.1. Plasma lens focusing

High energy density physics requires beam bunches of 

high intensity. This is usually achieved through bunch

compression in the synchrotron. This technique, however,

leads to an increase in longitudinal emittance. Along with the

transverse emittance this poses a problem for the final

focusing system. The focusing effect of conventional quad-

rupole doublets is a second order effect. Each quadrupole

focusses in one plane and defocusses in the transverse plane.

Thus the performance of quadrupole lens focusing is limited

by field strength considerations and limitations are severe in

cases where extremely small focal spots are necessary for the

experiment. Here a high focusing gradient and a large aper-

ture for the quadrupole system is necessary. Moreover space

charge considerations may play a role in cases of extreme

intensity like ion beam focusing for inertial fusion. Before we

started our experiments at GSI, part of our team has suc-

cessfully tested a plasma lens to capture antiprotons from the

production target at CERN   [42]. In that case a divergent

beam, originating from a production point had to be adapted

to a beam transport system. We had to deal with the reverse

Fig. 14. Electrons are generated forming a line focus subtending an angle with respect to the ion-beam axis, and pass perpendicularly through the beam. As a

function of the distance to the beam axis they do experience a deflection and form a curved line on a scintillator.

Fig. 15. EBI-Diagnostic of an intense He-ion beam at the FRANZ accelerator

in Frankfurt.

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problem, to focus a beam to a small spot size to induce high

energy density. The starting point was a cylindrical discharge

that produced a homogeneous wall stabilized plasma, which

was also used for beam plasma interaction experiments, which

we discuss later.

Fig. 17 shows the result of a focusing experiment where the

beam was focused down to a 300 mm spot size from originally10 mm. The focus period was 300 ns. This is sufficient since

typical beam bunch lengths are on the order of 100 ns or less.

In this discharge we used a 10 kV discharge with a maximum

current of 22 kA and a total energy of 200 J was stored in the

capacitor bank. Due to the success of this experiment a much

larger Z-pinch plasma was built where the stored energy went

up to 2.1 kJ, the maximum current to 150 kA at a discharge

voltage of 32.5 kV  [43]. The high current plasma lens based

on the Z-pinch principle is shown in  Fig. 16.

During different times of the discharge the current distri-

bution changes from homogeneous, which results in a linear

B-field to inhomogeneous, which produces a non-linear B-

field and leads to an annular focus. This feature became

interesting for the planned experiments at the future FAIR

facility, which we will discuss in a later chapter.

Now that we have followed the beam from the ion source to

the focusing point we are ready to address:

3.2. Beam-plasma interaction physics

Soon after the discovery of alpha-decay, nuclear physics

addressed the problem of energy loss of ions in matter. The

interest in energy loss of heavy ions started, when energetic

ions became available from fission processes. Investigation of 

particle energy loss problems has since then become a tradi-

tional topic of nuclear physics with application mainly in

detector development, but not only there. Tumor therapy with

swift heavy ions started at Berkeley laboratories and today we

see many places where energetic protons, alpha particles and

Fig. 16. Wall-stabilized plasma to serve as a plasma lens-The focal spot of the ion beam is observed with a fast CCD camera on a scintillator screen (NE 102A).

Fig. 17. High current (150 KA, 32.5 kV, 2100 J) Z-pinch plasma lens with linear and nonlinear B-field configuration.

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heavy ions like carbon and oxygen are used in radiation

therapy treatment. Interaction processes of intense ion beams

are also an ideal tool to probe high energy density plasmas and

to investigate their properties. The kinetic energy of the heavy

ions can exactly be tailored to the experimental conditions.

The ions penetrate deep into the volume of the plasma target.

Energy loss and the final charge state distribution of the ionsare the typical signals which reveal the beam plasma inter-

action processes, and they allow to draw conclusions for the

plasma target properties [44].

All institutes involved in this review (GSI-Darmstadt;

ITEP-Moscow and IMP-Lanzhou) carried out experiments to

measure the energy loss of ions in ionized matter. Examples

are given in Refs.   [45e47]. In all reported cases the energy

loss of ions in plasma is higher than the energy loss in normal

matter that we are used to. In this review we suggest to change

our frame of reference and consider the case of a free electron

gas as the reference case. This case is experimentally realized

in a fully ionized hydrogen plasma, and this state is the most

prevalent in the visible universe. Energy loss of ions in plasma

is predominantly due to collisions with electrons. Only at very

low velocity the nuclear stopping is important. The interaction

is mediated by the long range Coulomb force. Impact pa-

rameters up to the Debye shielding length contribute to the

energy loss. This implies that also collisions at large impact

parameter with low energy and momentum transfer contribute

to the energy loss process. This is different when we deal with

energy loss and stopping processes in ordinary   “cold”  matter.

Here we have bound electrons and in general only those col-

lisions contribute to the energy loss of the ions, where the

ionization energy or at least some excitation energy is trans-

ferred in the collision process. If this is not possible due to alarge impact parameter then quantum mechanics rules out any

energy loss. Therefore a vast part of the collisions is without

effect and hence the total energy loss is lower than in the

equivalent amount of fully ionized matter. In inertial fusion,

the target will end up in a highly degenerate state and fusion

generated alpha particles are supposed to deposit their kinetic

energy in degenerate matter. Since in degenerate matter all

states up to the Fermi-edge are occupied, only those collisions

may contribute to the energy loss where an electron is moved

across the Fermi edge. Here again at large impact parameters

with low energy transfer, much less electrons are available for

effective collisional energy transfer, and hence we expect a

lower energy deposition in the target. This effect may add to

the problems we currently see in fusion physics. It may not be

the main problem, compared to turbulent mix of the fuel,

however it adds to the general problem and is an interesting

question of basic physics.Information on heavy-ion beameplasma interaction ex-

periments, became available, when first experiments at GSI

were started. In order to have clean boundary conditions the

first beameplasma interaction experiments at GSI, were per-

formed with hydrogen. Already at moderate temperature and

density conditions, which are easily obtained in a discharge

plasma, a state of almost fully ionization may be obtained for

the duration on the order of microseconds. Later a dense

Zpinch plasma was used to extend the measurements to higher

density and higher temperature   [48e50]. These experiments

made it possible to compare the stopping power of hydrogen

gas and fully ionized hydrogen plasma in one experimental

set-up. In total, the plasma parameters of these first experi-

ments ranged in density from ne   ¼   1016 cm3 to

ne ¼  1019 cm3, with 2 eV   T e    20 eV. The experimental

results clearly demonstrated the high stopping power of fully

ionized plasmas, due to the interaction of beam ions with free

electrons in plasma as compared to lower stopping power,

where bound electrons are involved.

At high energy (left part of  Fig. 18) the energy loss in cold

gas is a factor of 2e3 lower than in the case of fully ionized

hydrogen. At low energy (right part of  Fig. 18) the experiment

was performed at 45 keV/u where the ion velocity is close to

the average electron velocity in the plasma, and thus the

stopping power is close to the maximum. For heavy ions alsothe charge state plays an important role. An electron capture

process of the beam ion requires momentum and energy

conservation. This is difficult to fulfill for the capture of free

electrons. Therefore a heavy ion traversing a fully ionized

plasma shows a high charge state, since capture processes are

reduced but ionization by target nuclei and plasma electron

continues at the cross section determined by the respective

velocities. In the energy range considered, the well-known

Bethe-formula without polarization correction describes the

energy loss in hydrogen ( Z 2 ¼  1) quite well:

Fig. 18. Energy loss of Pb ions in hydrogen gas and hydrogen plasma (a). Stopping power for Kr-ions at low energy (b). The plasma was generated by a discharge.

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dE 

d z ¼ Z 2eff $1$e$u

v2  $lnL   ð7aÞ

Lbound ¼ 2mev2

 I Lfree ¼ 0:76

  4v

bminu

ð7bÞIn Eq.   7(a), (b),   z   denotes the direction of ion beam

movement inside the target, Z eff  is the effective nuclear chargeof the projectile, e is the electron charge,  me  the electron rest

mass,   u   the plasma frequency, which is a function of the

density, and finally   v   is the ion velocity. We distinguish the

Coulomb logarithm L for the case of free and bound electrons

respectively. Therefore in the case of bound electrons, which

refers to non-ionized matter, this term contains the average

ionization energy I , and for the case of free electrons, which

refers to fully ionized matter, the denominator contains the

minimum impact parameter. This may be in some cases, due to

Debye shielding, the respective Debye length, which is indi-

cated by the index   u.

In total, the beam energy in these first experiments wasvaried between 1 and 6 MeV/u for different ion species from

carbon to uranium and the stopping power of fully ionized

matter exceeded that of cold matter always by roughly a factor

of three. This enhancement, as seen in   Fig. 17   was mainly

attributed to the efficient energy transfer to free electrons in

small angle collisions. For lower kinetic energies, where the

projectile velocity is comparable to the thermal velocity of the

plasma electrons, the energy loss behavior is even more dra-

matic. An enhancement factor close to 40 was measured [51],

and the main contribution in this case is the higher effective

charge state   Z eff    of the beam ions, due to the reduced

recombination processes in highly ionized plasma. The dy-

namic equilibrium between ionization and capture processes isshifted towards higher charge states. Free electrons are diffi-

cult to capture for the beam ions, since energy and momentum

conservation requirements are difficult to be fulfilled at the

same time with free electrons. With bound electrons, however,

momentum conservation is generally no problem due to the

strong binding energy. The resulting reduction in electron

capture cross section depends strongly on the ionization de-

gree of the plasma. Therefore hydrogen gas was the first

choice as a plasma target, because it is the only material which

can be transformed from a solid to a liquid, a gas, a plasma

and finally a completely ionized plasma with only a negligible

amount of remaining bound electrons. Charge state analysis of 

beam ions penetrating the fully ionized hydrogen plasma

clearly showed the effect of an enhanced average charge state

[52].The experimental challenge was to extend the investigation

towards plasma parameters with higher temperature and den-

sity, in order to have conditions that are more close to a fusion

plasma. Such conditions can be generated by high power, high

energy lasers.

The diameter of a laser focus usually is in the sub-

millimeter range and the limit is determined by diffraction

effects. One characteristic of laser plasma is the existence of 

strong gradients in density and temperature and a short life-

time. The diameter of ion-beam bunches is usually on the

order of 1 mm. The experimental task was to match these

conditions. As shown in   Fig. 19, the ion beam diameter was

narrowed down by a 500  mm aperture and the laser spot size

was increased to 1 mm and thus the effect of strong laser-

plasma gradients was minimized. Nevertheless, due to the

coherent nature of laser light a laser focus always contains

speckles consisting of intensity variations up to a factor of 4.

This effect is usually minimized by random phase plates (see

Fig. 19). Also the problem of time mismatch could be mini-

mized. The longest possible laser pulses of up to 10 ns dura-

tion were used. The beam bunches from the accelerator arrive

at the target with a frequency of 109 MHz. Therefore they

constitute a pulse train with one ion pulse every 9.9 ns. The

duration of each micro bunch of the beam pulse ranges from

less than 1 ns up to 4 ns. With this set of measures laser andion beam were matched to each other to the best of available

experimental technique. However, there remains the funda-

mental problem of laser plasma generation. Light may pene-

trate matter only up to the critical surface. Therefore, soon

after the onset of the laser pulse a plasma is created on the

surface of the target and the critical density moves away from

the target surface, thus creating a diffusion zone. Finally the

target experiences ablative pressure and a shock wave is

generated, heating the bulk matter of the target. When finally

Fig. 19. In order to achieve more uniform irradiation of the target, a two sided irradiation geometry using both lasers systems at GSI was chosen.

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the ion beam passes through these different zones, each zone

contributes differently to the measured total energy loss.

Plasma diagnostic, based on optical spectroscopy as shown in

Fig. 19 can only analyze the plasma up to the critical density

[53]. For the rest we until now have to rely on simulations.

Therefore in future experiments penetrating radiation must be

used to analyze the dense part of the target. This is a task where the teams are currently working on.

The experiments show the expected effect that after the

plasma generation (see Fig. 20) the energy loss rises from the

initial energy loss in the cold target material (z2 MeV), up to

some maximum (z4 MeV) and decreases with the hydrody-

namic expansion of the target material. Latest measurements

[54]   indicate however, that the increase effect is lower than

expected from available simulations. Since at the moment we

have to rely on simulations, we do not speculate here on the

reasons. It may eventually be an effect attributed to the

properties of warm dense matter that is generated in the bulk 

material of the target.

4. Dense plasma and high energy density matter

4.1. Generating high energy density with intense ion

beams

The quest for a deeper understanding of dense plasma

phenomena and properties of matter under extreme conditions

is the driving motivation for High Energy Density Physics at

many laboratories worldwide.

Among all methods to generate high energy density states

of matter, heavy ion beams hold a unique position.

The total kinetic energy of heavy ions is determined by theacceleration process in the accelerator system and can there-

fore be tailored exactly to the experimental conditions and

needs.  Fig. 21   shows the penetration of a 300 MeV/u Ar-ion

beam into a Krypton crystal. The number of Ar ions is

measured with high precision by fast beam transformers, the

initial energy is 300 MeV/u with an uncertainty well below

1%. Therefore we have the situation that the initial conditions

of the spatial and temporal distribution of the energy deposi-

tion is very well known. High energy density states that are

reached during the heating process can then easily be traced

back to the initial conditions. With this kind of precision for

the initial conditions no other method is able to compete.

Moreover the resulting gradients with respect to temperature

and density extend over macroscopic dimensions of some

millimeter up to centimeter Therefore the starting conditions

are quite homogeneous.

In Fig. 22 we see the result of one of the first high energy

density in matter experiments. At   t  ¼   0 the beam bunch is

deposited deep inside the bulk matter of solid Ne at cryogenictemperature. The deposition region is clearly visible on the

first frame. Heating of the crystal changes the bulk properties

of matter. The first sign of it is that the previously clear and

optically transparent crystal is now opaque. Moreover the

onset of hydrodynamic response to the energy deposition is

revealed on the second frame. The contour of the crystal now

follows the energy deposition profile. The onset of motion

starts close to the maximum energy deposition region at the

end of the range of the ion beam. This region is commonly

denoted as Bragg peak region. After 186 ms this feature is even

more distinct (third frame of  Fig. 22). The expansion velocity

is connected to the bulk properties of matter by the respective

equation of state. A measurement of the expansion velocity

therefore yields equation of state data. From this early

experiment it is clear that, for target material like lead or other

metals, it is necessary to have penetrating radiation as a

diagnostic tool. We will discuss this later.

The figure of merit for laser matter interaction experiments

to induce high energy density is the laser intensity I measured

in W/cm2 and the total energy. Due to the nature of ion matter

interaction, where ions penetrate deep into the target volume,

the important parameter is the energy  E s, deposited per gram

of matter (J/g]) and the deposition power Ps measured in W/g.

Hence the physics of beam induced high energy density

matter is governed by three equations (Eqs.  (8)e(10)):

E s ¼

1:6$1019$

dE dx$ N 

p$r 2  ½ J =g;   ð8Þ

where dE  /d x   is the stopping power of the material,   N   is the

number of beam ions delivered by the accelerator  pr 2 is the

focal spot area. In order to achieve high deposition energy the

accelerator has to provide the maximum beam intensity and

the experiment has to care for an effective focusing. The

stopping power is given by nature and we will show later that

it may be a very different situation if the matter is in an ionized

state or not. The time t H to deliver this energy is limited, due tothe hydrodynamic response of the beam heated material, and is

approximately given by:

Fig. 20. Energy loss of Ar-ions in laser generated carbon plasma. Fig. 21. Space resolved energy deposition of a Neon Beam in a Kr crystal.

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t  H f

 L 2

P

1=3

;   ð9Þ

where, L  is the target dimension. For a cylindrical target this is

the target radius and   t H   is essentially given by the time ararefaction wave needs to travel over the distance  L .

Combining these two equations (Eqs. (8) and (9)) yields the

total deposition power  Ps:

Ps ¼ E s

t  H 

:   ð10ÞFrom Eq.   (10)   the necessity arises to have beam bunches

that are shorter in time  tbb  than the limit for the heating time

set by hydro-motion (tbb    t H). The time scale is set by the

sound speed  C S which defines the time for a rarefaction wave

to travel across the distance of the focal spot radius. By the

time the rarefaction of the target material has reached the outeredge of the focal spot the effective heating of the target ma-

terial stops. Thus the heating t H time is given as the upper limit

of the integral (Eq.  (11)):

r o ¼Z t  H 

o

csðT ðPsÞÞdt    ð11Þ

The effective heating time (t H) therefore depends on the

equation of state of the material. In the limit of a mono-atomic

ideal gas with the adiabaticity coefficient  k ¼ 5/3 this can be

written as:

r o ¼Z t  H 

o

 ffiffiffiffiffiffiffiffiffik$E s

p   $dt ¼

Z t  H 

o

 ffiffiffiffiffiffiffiffiffiffiffiffiffik$Ps$t 

p   dt    ð12Þ

Note that   E s   is given in J/g. The focal spot radius   r o, the

specific energy deposition  E s, and the beam bunch length  tbbare therefore interrelated through:

r o ¼ ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffik$Ps$tbb

p   $

2

3t  H 

32:   ð13Þ

For the experiment this result has important consequences:

The beam intensity, the bunch length and the minimum

focal spot cannot be chosen independently from each other. As

an example we calculated a focus radius of 250   mm for

E s ¼  0.1 TW/g  [55].

In Fig. 22 we present the high energy density states that are

available with heavy ion beams of different intensity. The left

inset of  Fig. 23 shows the available temperature as function of 

deposition power. The quantity E s used in the equations above

is given in MJ/g. Since the temperature which is obtained

depends on the equation of state we used the SESAME li-

brary. In the high temperature limit they approach the ideal

Fig. 22. Hydrodynamic motion induced by heating matter with an intense beam of heavy ions.

Fig. 23. Available high energy density states as function of deposited energy (J/g (a) and entropy (J g1 K 1]. SIS-18 is the synchrotron currently in operation at

GSI-Darmstadt. SIS-100 is the first stage of the planned FAIR facility in Darmstadt.

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gas equation of state. Current experiments are carried out in

the region of 1 kJ/g. This corresponds to the lower left end in

Fig. 23 (0.001 MJ/g). The two red horizontal lines mark the

region of Warm Dense Matter. Above a temperature of 10 eV,

we expect strong hydrodynamic motion and the onset of a

radiation regime. Above 100 eV, we surely enter the radiation

dominated regime, where every additional input of energy isvery efficiently converted to radiation. The aim of future fa-

cilities must be to enter this regime, since it is relevant for ion

driven fusion. The right part shows the pressure as function of 

entropy. Shock wave experiments generally produce data

along the Hugoniot line (black). Our experiments are aimed to

achieve sudden heating with a state on the HI-HEX quasi

isochoric heating line and then have the matter expand to

explore the region below. Current experiments center close to

the indicated critical point (CP). The example is taken for

lead.

The most favorable beam ion for high energy density

physics experiment is Uranium due to its high nuclear charge.

Experiments were able to be operated with up to 4.4    109

particles per bunch in approximately 100e125 ns. The in-

tensity limitations have been discussed in the previous section.

It is important to investigate thermophysical properties and

hydrodynamic response of various materials including Pbsamples. The samples under investigation endure a rapid

heating process, in some experimental conditions 2.2   1010

(K/s) were obtained. This takes the sample into the two-phase

liquidevapor region near the critical point.

The diagnostic tools are at the moment limited to optical

diagnostic. As mentioned above the expansion velocity can be

measured. Another method is to measure the impact of the

expanding material onto a sapphire window. The displacement

of the back surface of the sapphire window can be measured

and from this the pressure can be inferred. A very elegant

Fig. 24. Irradiating a cylindrical target volume (cryogenic, solid Ne) inside bulk matter. The irradiation time is 1000 ns with a U beam of 190 MeV/u. Density,

temperature and phase of the target material are indicated from left to right. The density scale is from 0.2 g/cm3, temperature scale from 10 K to 2000 K.

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method was developed with a fast multi-channel radiation

pyrometer. This is now one of the key diagnostic tools   [56].

Brightness temperature profiles were measured for lead sam-

ples. The results show that the state of matter achieved by

heavy ion beam heating is equivalent to samples that were

initially shocked up to 1.51, 1.80 and 2.23 Mbar. In our ex-

periments using ion beams to heat samples, the physicaltemperature was obtained from the pyrometer measurements,

and fitting a gray-body model to the data. The pyrometer had

six different channels for a simultaneous measurement at six

different wavelength. In the beam-driven experiment, the total

duration of the heating pulse was about 1 ms with full width at

half maximum (FWHM) of 125 ns. During the heating phase,

the sample foil is driven to the melting point and started to

evaporate at the free surface. While expanding, the lead vapor

is rapidly cooling down and at the moment when its temper-

ature becomes sufficient for homogeneous nucleation (near the

vapor spinodal line), liquid droplets appear inside the vapor

and a boiling wave is formed. After this moment, the expan-

sion dynamics is governed by surface evaporation processes.

The heating ion beam itself may also be used as a diag-

nostic source. Due to the hydrodynamic response of the ion-

beam heated target matter, the target density changes as time

progresses.

Therefore the penetration depth of the beam or if a pene-

trating beam is used, the change in energy loss of the emerging

beam is a measure of the target density along the interaction

region. By this technique which was developed by D. Var-

entsov as part of his dissertation work  [57]  first experimental

results on measurements of energy loss dynamics of uranium

beams in neon using different initial energy and intensity were

obtained. The energy loss dynamics measurements were thencomplemented by two-dimensional hydrodynamic simula-

tions. A comparison between the experimental data and sim-

ulations resulted in the development of a new wide-range

equation of state for neon [57]. In the low temperature region

none of the measured results were compatible with existing

data on the equation-of state. However in the high energy

regime simulations agreed with the data within error limits.

This points to the fact that, in the low temperature warm dense

matter, part of the phase diagram we still are in an unchartered

area.

The energy deposition characteristics of high-energy heavy

ion beams in dense matter favor a cylindrical geometry. A

simple experimental scenario is therefore a quasi-cylindrical

plasma volume produced from focusing an intense ion beam

into an extended target volume. A simulation of such experi-

ment is shown in Fig. 24. The beam of U-ions at 190 MeV/u is

deposited inside the target volume(cryogenic, solid Ne) over a

time span of 1000 ns. After 300 ns the hydro motion is clearly

visible showing compressed states of matter. The density

along the interaction zone of target material and the ion beam

decreases due to hydro motion. Therefore the beam penetrates

further and finally exits the target at the rear end. Now the

energy of the beam behind the target can be measured. At the

end the beam will fully evaporate the target. This way the time

it takes for the beam to appear at the rear end and the dynamic

energy loss as well as the surface expansion are indications of 

the high energy state that is reached during the interaction

process.

A different experimental scenario, which we use in our

experiments, is called HIHEX-heavy ion beam heating and

expansion. Fig. 25 shows the diagnostic set-up for the exper-

iment. As a matter of fact in these experiments we use aslightly elliptical beam shape and irradiate a complete sample

in order to heat a bulk piece of matter as homogeneously as

possible. This way we may in first or zero order approximation

assume that we have low gradients in temperature and density

as starting conditions, before hydrodynamic motion sets in.

The diagnostic tool is then to observe the radiation from the

surface with the fast pyrometer, the expansion velocity and the

impact onto the sapphire window.

A more complicated scenario with higher compression

yields can be achieved with a special beam focus geometry,

e.g. a hollow cylindrical beam focus at the target position, as

sketched in Fig. 25.

This scenario has at the moment not yet been tested. It is part

of the collaborative effort of the HEDgeHOB collaboration at

FAIR. To achieve an annular focus is a challenging problem.

The example shown in Fig. 26 was obtained with a non-linear

field distribution of the plasma lens. Problems that will arise

are obvious from this figure. The intensity distribution is not

evenly distributed and will eventually not lead to the cylindrical

compression. Therefore in addition to a plasma lens at ITEP

[62,63] we are currently building at ITEP a wobbler system to

achieve a homogeneous annular distribution [64].

The working principle as sketched in  Fig. 27 is like that of 

an old TV tube, using rf cavities for the deflecting electric

field. In order to achieve sufficient homogeneity it is necessaryto have at least 10 circulations during the beam bunch length

of 100 ns. This sets the requirements for the applied rf-fre-

quency. Nevertheless it is a very challenging problem for the

beam transport and focusing system. Applying an additional

Fig. 25. HIHEX scenario, here the whole sample is irradiated by an elliptical

beam and the associated diagnostic equipment.

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magnetic field, the heating of target material, can be enhanced

by more than an order of magnitude. If an external magnetic

field is introduced (see Fig. 25), the effect of magneto-thermal

insulation may allow to reach even keV temperatures in the

compressed inner cylinder consisting of deuterium gas. The

experimental conditions for these experiments require, how-

ever, the maximum beam intensities available from the new

facility together with a high initial magnetic field. Therefore

this is not an experiment to be performed during the start-up

phase of FAIR. This experiment also requires to diagnose

the conditions inside the outer high-Z cylinder during the

compression phase. Therefore penetrating radiation is neces-

sary and we started to develop radiography based on high

energy protons and we call it: the PRIOR-Project.

4.2. Advanced diagnostic methods: the PRIOR-project 

To the best of our knowledge a breakthrough for radiog-

raphy with protons was achieved at Los Alamos National

Laboratories using 800 MeV protons. We follow this concept

and have designed a proton microscope for experiments at GSI

and FAIR  [58]. With a special set-up of four quadrupoles as

shown in Fig. 28. Focusing as a function of scattering angle is

achieved in a Fourier plane. This allows to get rid of high

angle scattering events that lead to excessive blur of the

resulting picture. The final two quadrupoles achieve a point to

point imaging with some magnification. A number of effects

contribute to image blur. These are Coulomb scattering,

chromatic aberration and detector blur. All these effects may

be minimized by using high energy protons. At GSI we

currently use 4 GeV and an energy up to 10 GeV will be

available at FAIR.

In a collaborative effort of ITEP-Moscow, GSI-Darmstadt,

TU-Darmstadt and Los Alamos National Laboratory, a proton

microscope was constructed and successfully tested in July

2014.   Fig. 29   shows the proton microscope with four quad-

rupoles made of permanent magnets and the test picture,

demonstrating the radiographical capabilities of this device.

We strongly believe that with the completion of FAIR at

GSI in a couple of years, high energy density physics withheavy ion beams will enter a new era.

5. Conclusion and outlook to the future

We believe that it is fair to say that in the recent past there

were 4 accelerator laboratories leading the research in high

energy density physics with ion beams: GSI-Darmstadt, ITEP-

Moscow, LBNL-Berkeley and IMP-Lanzhou (see Fig. 30), not

to forget TIT-Tokyo and Universite de Paris Sud.

Here it would lead too far to list the achievements of the

different laboratories. However two of these laboratories have

remarkable plans for the future. At the site of GSI-Darmstadtthey currently are in the middle of constructing the FAIR

facility, and in China there are plans for a new heavy ion

accelerator facility with intense beams (HIAF). The leading

laboratory here is the Institute of Modern Physics, Lanzhou.

While there are still plans awaiting approval and further

detailing, it is obvious that beam matter interaction with

intense beams will have a future that probably will give us

more insight into the prospects of intense beams as drivers

for inertial fusion. Experiments at GSI are currently carried

out at   E s ¼   1 kJ/g, and this number will rise to 120 kJ/g at

FAIR and the first estimations for HIAF range from 300 kJ/g

up to eventually 1 MJ/g. With these numbers it will be

Fig. 26. The principle of magnetized targets for heavy ion beam experiments. The focus of the ion beam is annular. An example of a ring-focus is shown in the left

part of the figure. This result was achieved with the GSI plasma lens. Highest plasma parameters are obtained where the annular beam heats the outer liner material

in the annular focus region only, and the remaining cold portion of the liner is accelerated inward by the beam heated material. An initial magnetic field of 

approximately 30 T is required to reach the self-sustained magnetic implosion regime in hydrogen.

Fig. 27. Wobbler system to achieve an annular beam focus. Currently under

construction at ITEP Moscow.

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Fig. 29. The PRIOR proton microscope and the first test result with a 4 GeV proton beam at GSI.

Fig. 28. Beam transport system of the proton microscope.

Fig. 30. Leading laboratories in HEDP with ion beams: Helmholtzzentrum fur Schwerionenforschung GSI-Darmstadt, Institute for Theoretical and Experimental

Physics (ITEP-Moscow, now part of Kurchatov Institute), Heavy Ion Fusion Science-Virtual National Laboratory (Berkeley, the national laboratories at Princeton,

Livermore and Berkeley constitute this laboratory), Institute of Modern Physics, Lanzhou (Chinese Academy of Science).

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possible to enter the radiation dominated regime. It is still

not enough to ignite a fusion target, but scaled experiments

will be possible not only for target physics but also provide a

better basis to scale the properties of accelerators up to a

fusion driver.

Acknowledgments

The authors first of all want to thank their respective in-

stitutes for supporting this work. DHHH wants to thank 

especially the Chinese Academy of Sciences and IMP at

Lanzhou for their hospitality during frequent visits and

appointment as guest professor. The support of the German

BMBF is acknowledged for many supporting grants for

PRIOR, cryo-target development, beam diagnostics and ma-

terial properties research. Moreover the support of DFG-

RFBR (German Science Foundation  e Russian Foundation of 

Basic Research), and the Russian grant of Scientific school

НШ e 5814.2014.2 is acknowledged. Last but not least we are

grateful for funding from National Natural Science Foundation

of China NSFC grants Nos.: U1532263, 11505248, 11375034,

11205225, 11275241, and 11275238.

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