search for the cosmic neutrino background and the nuclear beta decay (katrin). amand faessler...
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Search for the Cosmic Neutrino Background and the Nuclear Beta Decay (KATRIN).
Amand FaesslerUniversity of Tuebingen
Germany
Publication: Amand Faessler, Rastislav Hodak, Sergey Kovalenko, Fedor Simkovic:
arXiv: 1304.5632 [nucl-th] 20. April 2013.
Cosmic Microwave Background Radiation
(Photons in the Maximum 2 mm)
Decoupling of the photons from matter about 300 000 years after the Big Bang, when the electrons are captured by the protons and He4 nuclei and the
universe gets neutral. Photons move freely.
Penzias and Wilson;BellTelephon
Nobel Price 1978
Microwave Background Radiation
Planck Satellite Temperature FluctuationsComic Microwave Background (March 21. 2013)
6
Curvature of the Univers
flat
xx x
1 1 1
WMAP 2002 :
1.00 0.02
We know the size of the hot spots.
Black body radiation.
Temperature adjusted
(pdg 2012):T=2.7255(6) K
Experiment
Microwave Background Radiation
T = 2.7255(6) Kelvin
Planck‘s Black Body Radiation
Neutrino Decoupling and Cosmic Neutrino Background
For massless-massive Neutrinos:
Estimate of Neutrino Decoupling
Universe Expansion rate: H=(da/dt)/a ~ n Interaction rate: = G ne-e+<svrelative>
H = \sqrt{8 p G rtotal /3} = \sqrt{8 p r/(3 MPlanck2)}[1/time]
G ~ T3 <GF2 p2 c=1> = T3 GF
2 T2 = GF2 T5 [Energy = 1/time]
hbar = h/(2p) = c = 1
Neutrino Decoupling
G/H = ( kB T/ 1MeV)3 ~ 1 T(Neutrinos)decoupl ~ 1MeV ~ 1010 Kelvin; today: 1.95 K
Time after Big Bang: 1 Second
T(Photons)decoupling = 3000 Kelvin; today: 2.7255 K Time(Photons)decoupling = 300 000 years
Below T = 1 MeV:
(Energy=Mass)-Density of the Universe
log r
a(t)~1/T
Radiation dominated: r ~ 1/a4 ~ =Stefan-Boltzmann
Matter dominated: r ~ 1/a3 ~ T3
Dark Energy
1/Temp1 MeV1sec n
dec.
1 eV3x104y today
3000 K300 000 y
g dec.
8x109 y g 2.7255 Kn 1.95 K
Hamburg, March 3. 2008.
Tranformation from Mass to Flavor Eigenstates
Mass of the Electron Neutrino?Tritium decay (Mainz + Troisk)
With:
Hamburg, March 3. 2008.
Measurement of the upper Limit of the Neutrino Mass in Mainz: mn < 2.2 eV 95% C.L.
Kurie-Plot
Q = 18.562 keV
mn 2>0 mn2 <0 Electron Energy
Eur. Phys. J. C40 (2005) 447
Search for Cosmic Neutrino Background CnB by Beta decay: Tritium
Kurie-Plot of Beta and induced Beta Decay: n(CB) + 3H(1/2+) 3He (1/2+) + e-
Electron Energy
2xNeutrino Masses
Emitted electron
Q = 18.562 keV
Infinite good resolution
Resolution Mainz: 4 eV mn < 2.3 eV
Resolution KATRIN: 0.93 eV mn < 0.2 eV 90% C. L.
Fit parameters: mn
2 and Q value meVAdditional fit: only
intensity of CnB
Tritium Beta Decay: 3H 3He+e-+nce
Neutrino Capture: n(relic) + 3H 3He + e-
20 mg(eff) of Tritium 2x1018 T2-Molecules: Nncapture(KATRIN) = 1.7x10-6 nn/<nn> [year-1]
Every 590 000 years a count!! for <nn> = 56 cm-3
Kurie-Plot
Electron Energy
2xNeutrino Masses
Emitted electron
Resolution KATRIN: 0.93 eV mn < 0.2 eV 90% C.L.
Fit parameters: mn
2 and Q value meVAdditional fit: only
intensity of CnB
Two Problems1. Number of Events with average Neutrino Density
of nne = 56 [ Electron-Neutrinos/cm-3] Katrin: 1 Count in 590 000 Years Gravitational Clustering of Neutrinos!!!???2. Energy Resolution (KATRIN) DE ~ 0.93 eV
Gravitational Clustering of NeutrinosR.Lazauskas,P. Vogel and C.Volpe, J. Phys.g. 35 (2008) 025001;
Light neutrinos: Gravitate only on Mpc (Galaxy Cluster) scale: nn/<nn> ~ nb/<nb> ~ 103 – 104; <nb>= 0.22 10-6 cm-3
A. Ringwald and Y. Wong: Vlasov trajectory simulations
Clustering on Galactic Scale possible nn/<nn> = nb/<nb> ~ 106 ; (R = 30 kpc)Nncapture(KATRIN) = 1.7x10-6 nn/<nn> (year-1)
= 1.7 [counts per year]
Effective Tritium Source: 20 microgram 2 milligramNncapture(KATRIN*) = 1.7x10-4 nn/<nn> (year-1)
= 170 [counts per year]
Summary 1• The Cosmic Microwave Background allows to
study the Universe 300 000 year after the BB.
• The Cosmic Neutrino Background 1 sec after the Big Bang (BB): Tn(today) = 1.95 Kelvin.
• Extremly difficult to detect: Small Cross Section and low Density 56 n‘s/cm3 and low Energies (1.95 Kelvin = 2x10-4 eV).
2xNeutrino Masses
Emitted electron
Resolution KATRIN: 0.93 eV mn < 0.2 eV 90% C.L.
Fit parameters: mn
2 and Q value meVAdditional fit: only
intensity of CnB
Kurie-Plot
Electron Energy
Summary 21. Average Density: nne = 56 [ Electron-Neutrinos/cm-3] Katrin: 1 Count in 590 000 Years Gravitational Clustering of Neutrinos nn/<nn> < 106
1.7 counts per year (2 milligram 3H 170 per year)2. Measure only an upper limit of nn
ENDE