Why measure Geoneutrinos: the Earth's Heat Budget Bill McDonough, *Scott Wipperfurth Geology, U...
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Transcript of Why measure Geoneutrinos: the Earth's Heat Budget Bill McDonough, *Scott Wipperfurth Geology, U...
![Page 1: Why measure Geoneutrinos: the Earth's Heat Budget Bill McDonough, *Scott Wipperfurth Geology, U Maryland Fabio Mantovani, *Virginia Strati Physics, U Ferrara,](https://reader035.fdocuments.in/reader035/viewer/2022062221/56649f525503460f94c75a5c/html5/thumbnails/1.jpg)
Why measure Geoneutrinos: the Earth's Heat Budget
Bill McDonough, *Scott Wipperfurth Geology, U Maryland
Fabio Mantovani, *Virginia StratiPhysics, U Ferrara, Italy
Hiroko Watanabe, Physics, Tohoku U
Steve Dye, Natural Science,Hawaii Pacific U and Physics, U Hawaii
*graduate student
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Plate Tectonics, Convection,Geodynamo
Radioactive decay driving the Earth’s engine! K, Th & U!
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U in the Earth: ~13 ng/g U in the Earth
Metallic sphere (core) <<<1 ng/g U
Silicate sphere 20* ng/g U
*O’Neill & Palme (2008) 10 ng/g
*Turcotte & Schubert (2002) 31 ng/g
Continental Crust 1300 ng/g U
Mantle ~12 ng/g U
“Differentiation”
Chromatographic separationMantle melting & crust formation
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after Jaupart et al 2008 Treatise of Geophysics
Mantle cooling(18 TW)
Crust R*(7 ± 1 TW)(Rudnick and Gao ’03
Huang et al ‘13)
Mantle R*(13 ± 4 TW)
Core(~9 TW)
-
(4-15 TW)
Earth’s surface heat flow 46 ± 3 TW
(0.4 TW) Tidal dissipationChemical differentiation
*R radiogenic heat (after McDonough & Sun ’95)
total R*20 ± 4
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the future is… Geoneutrino studies
Nature & amount of Earth’s thermal power radiogenic heating vs secular cooling
estimates of BSE from 9TW to 36TW
constrains chondritic Earth models
estimates of mantle 1.3TW to 28TW
layers, LLSVP, superplume piles
- abundance of heat producing elements (K, Th, U) in the Earth
- clues to planet formation processes
- amount of radiogenic power to drive mantle convection & plate tectonics
- is the mantle compositionally layered? or has large structures?
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Summary of geoneutrino results
SILICATE EARTH MODELSCosmochemical: uses meteorites – 10 TWGeochemical: uses terrestrial rocks –20 TWGeodynamical: parameterized convection – 30 TW
TW scales relative to U 10, 20, 30 TW ≈ 10, 20, 30 ppb
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KamLAND, Japan (1kt) Borexino, Italy (0.3kt)
116+28-27
from Mar ‘02 to Nov ‘12
14.3±4.4
from Dec ‘07 to Aug ‘12
SNO+, Canada (1kt)
under construction (online 2015/16?)
Present Liquid Scintillator Detectors
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HanohanoInternational ocean-based (10kt)
LENA,EU
(50kt)
JUNOChina(20kt)
Futuredetectors?
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Geoneutrino Flux on Earth Surface
Earth structure (r and L) and chemical composition (a)
Activity and number of produced geoneutrinos
Volume of source unit
Survival probability function
Distance between source unit and detector
Abundance and density of the source unit
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Constructing a 3-D reference model Earth
assigning chemical and physical states to Earth voxels
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Predicted Global geoneutrino flux based on our new Reference Model
Huang et al (2013) G-cubed arXiv:1301.0365
Geoneutrino detection rate--TNU: Terrestrial Neutrino Unit-- 1 TNU = one geoneutrino event per 1032 free protons per year
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SUMMARY Earth’s radiogenic (Th & U) power
22 ± 12 TW - Borexino 11.2 TW - KamLAND
Prediction: models range from 8 to 28 TW (for Th & U)
On-line and next generation experiments: - SNO+ online 2015 - JUNO: 2020, good experiment, big bkgd, geonu …- Hanohano: this is FUNDAMENTAL for geosciences Geology must participate & contribute to the cost
Future:
-Neutrinographic Imaging of Earth’s deep interior
+ 7.9- 5.1