Neutrino tomography of the earth: the earth total mass, moment of inertia and hydrostatic equilibrium constraints

Abstract We investigate the implications of the constraints following from the precise knowledge of the total Earth mass, $$M_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> , and moment of inertia, $$I_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>I</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> , and from the requirement that Earth be in hydrostatic equilibrium (EHE), in the neutrino tomography studies of the Earth density structure. In order to estimate the sensitivity of a given neutrino detector to possible deviations of the inner core (IC), outer core (OC), core (IC + OC) and mantle Earth densities from those obtained using geophysical and seismological data and described by the preliminary reference Earth model (PREM), in the statistical analyses performed within the neutrino tomography studies one typically varies the density of each of these structures. These variations, however, must respect the $$M_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> , $$I_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>I</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> and EHE constraints. Working with PREM average densities we derive the $$M_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> , $$I_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>I</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> and EHE constraints on the possible density variations when one approximates the Earth density structure with (i) three layers – mantle, outer core and inner core, and (ii) four layers – upper mantle, lower mantle, outer core and inner core. We get drastically different results in the two cases.

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Publication Details

Journal
The European Physical Journal C
Published
2024-09-30
DOI
https://doi.org/10.1140/epjc/s10052-024-13348-7
Citations
2
Primary Topic
Neutrino Physics Research
Type
article
Field-Weighted Citation Impact
1.32

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article

Neutrino tomography of the earth: the earth total mass, moment of inertia and hydrostatic equilibrium constraints

S.T. Petcov
2 citations
The European Physical Journal C
Neutrino Physics Research
1.32
article

Neutrino tomography of the earth: the earth total mass, moment of inertia and hydrostatic equilibrium constraints

S.T. Petcov
article en
2 citations

Abstract

Abstract We investigate the implications of the constraints following from the precise knowledge of the total Earth mass, $$M_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> , and moment of inertia, $$I_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>I</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> , and from the requirement that Earth be in hydrostatic equilibrium (EHE), in the neutrino tomography studies of the Earth density structure. In order to estimate the sensitivity of a given neutrino detector to possible deviations of the inner core (IC), outer core (OC), core (IC + OC) and mantle Earth densities from those obtained using geophysical and seismological data and described by the preliminary reference Earth model (PREM), in the statistical analyses performed within the neutrino tomography studies one typically varies the density of each of these structures. These variations, however, must respect the $$M_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> , $$I_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>I</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> and EHE constraints. Working with PREM average densities we derive the $$M_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> , $$I_\oplus $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>I</mml:mi> <mml:mo>⊕</mml:mo> </mml:msub> </mml:math> and EHE constraints on the possible density variations when one approximates the Earth density structure with (i) three layers – mantle, outer core and inner core, and (ii) four layers – upper mantle, lower mantle, outer core and inner core. We get drastically different results in the two cases.

The European Physical Journal CVol. 84(9)
Scuola Internazionale Superiore di Studi Avanzati (IT), Kavli Institute for the Physics and Mathematics of the Universe (JP), Bulgarian Academy of Sciences (BG), Institute for Nuclear Research and Nuclear Energy (BG), The University of Tokyo (JP)
European Commission, Ministry of Education, Culture, Sports, Science and Technology
Openalex Percentile: Top 11%
Neutrino Physics Research
1.32
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