low q (10 ppb u) med. q (20 ppb u) high q (30 ppb u) 14±8 tnu bellini et al 2013 mantle flux: need...

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Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 ntle flux: need for Hanoha 13 TW 3-8 TW Depleted MORB Mantle 6-10 TW “EL”: hot basal layer Mantle = BSE - Crust

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Page 1: Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 Mantle flux: need for Hanohano 13 TW 3-8 TW Depleted MORB Mantle 6-10

Low Q(10 ppb U)

Med. Q(20 ppb U)

High Q(30 ppb U)

14±8 TNUBellini et al 2013

Mantle flux: need for Hanohano

13 TW

3-8 TWDepleted MORB Mantle

6-10 TW“EL”: hot basal layer

Mantle = BSE - Crust

Page 2: Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 Mantle flux: need for Hanohano 13 TW 3-8 TW Depleted MORB Mantle 6-10

Early Earth differentiation followed by 4 billion years of plate tectonics

Kellog et al (sciences 2000)

Page 3: Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 Mantle flux: need for Hanohano 13 TW 3-8 TW Depleted MORB Mantle 6-10

What’s hidden in the mantle?

Seismically slow “red” regions in the deep mantle

Core – Mantle Boundary

Can we image itwith geonus?

Retsima et al (Science, 1990)

Page 4: Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 Mantle flux: need for Hanohano 13 TW 3-8 TW Depleted MORB Mantle 6-10
Page 5: Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 Mantle flux: need for Hanohano 13 TW 3-8 TW Depleted MORB Mantle 6-10

HanohanoHanohano

A Deep Ocean

e Electron Anti-Neutrino Observatory

Deployment Sketch

Descent/ascent 39 min

- multiple deployments- deep water cosmic shield- control-able L/E detection

An experiment with joint interests in Physics,

Geology, and Security

Size: scalable from 1 to 50 kT10-yr cost est: $250M @ 10 kT

Page 6: Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 Mantle flux: need for Hanohano 13 TW 3-8 TW Depleted MORB Mantle 6-10

Deployment Sketch

Engineering StudiesEngineering StudiesMakai Ocean Engineering

• Studied vessel design up to 100 kilotons, based upon cost, stability, and construction ease.

– Construct in shipyard– Fill/test in port– Tow to site, can traverse Panama Canal– Deploy ~4-5 km depth– Recover, repair or relocate, and redeploy

Descent/ascent 39 min

Barge 112 m long x 23.3 wide

Page 7: Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 Mantle flux: need for Hanohano 13 TW 3-8 TW Depleted MORB Mantle 6-10

Addressing Technology Addressing Technology IssuesIssues

• Scintillating oil studies in lab– P=450 atm, T=0°C– Testing PC, PXE, LAB and

dodecane– No problems so far, LAB

favorite… optimization needed

• Implosion studies – Design with energy absorption– Computer modeling & at sea– No stoppers

• Power and comm, no problems• Optical detector, prototypes OK• Need second round design

-1

-0.8

-0.6

-0.4

-0.2

0

0.2

0.4

0.6

0.8

1

0.0025 0.0035 0.0045 0.0055 0.0065 0.0075 0.0085 0.0095

30% Foam filled (4105m)

Empty (4280m)

20m x 35mfiducial vol.

1 m oil

2m pure water

Page 8: Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 Mantle flux: need for Hanohano 13 TW 3-8 TW Depleted MORB Mantle 6-10

Testing Earth Models

Šrámek et al, 2012, EPSL

Page 9: Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 Mantle flux: need for Hanohano 13 TW 3-8 TW Depleted MORB Mantle 6-10

Predicted geoneutrino flux

Mantle flux at the surface

Šrámek et al (2013) EPSL 10.1016/j.epsl.2012.11.001; arXiv:1207.0853

Yu Huang et al (2013) G-cubed arXiv:1301.0365 

Total flux at surfacedominated by Continental crust

dominated by deep mantle structures

Page 10: Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 Mantle flux: need for Hanohano 13 TW 3-8 TW Depleted MORB Mantle 6-10

Ocean based experiment!

- Neutrino Tomography…

- Pacific Transect

- Avoid continents

- 4 km depth deployments

- Map out the Earth’s interior

- Test the modelsŠrámek et al (2013) EPSL arXiv:1207.0853

Page 11: Low Q (10 ppb U) Med. Q (20 ppb U) High Q (30 ppb U) 14±8 TNU Bellini et al 2013 Mantle flux: need for Hanohano 13 TW 3-8 TW Depleted MORB Mantle 6-10

Future:

-Neutrino Tomography of the Earth’s deep interior

Hanohano- 10 kt-yr Exposure–Mantle flux U geoneutrinos to ~10%–Heat flux ~15%–Measure Th/U ratio to ~20%–Rule out geo-reactor if P>0.3 TW

• There is also plenty of Neutrino Physics..There is also plenty of Neutrino Physics..• And much astrophysics and nucleon decay And much astrophysics and nucleon decay

too….too….