non-newtonian gravity in the earth’s gravity...
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Non-Newtonian gravity in the Earth’s gravity field
Joel Bergé (ONERA / Paris Saclay University) with P. Brax, M. Pernot-Borràs, J.P. Uzan
Looking for non-Newtonian gravity: Yukawa potential
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Kapner+ 2007, Wagner+ 2012, Masuda+ 2009
Joel Bergé, Rencontres de Moriond, March 27, 2019
Yukawa deviation V(r) = −GM
r(1 + αe−r/λ)
Tests of non-Newtonian gravity in space
!3 Joel Bergé, Rencontres de Moriond, March 27, 2019
From space: e.g. advance of perigee (LAGEOS) or equivalence principle (MICROSCOPE —P. Fayet’s and M. Pernot-Borras’ talks)
Possible lack of consistency: most tests either - assume Earth = point mass (ignore Earth’s shape) - or use/correct lowest shape information (extended sphere,
oblateness) from Earth models obtained under Newtonian gravity assumption
Yukawa deviation V(r) = −GM
r(1 + αe−r/λ)
Tests of non-Newtonian gravity in space
!3 Joel Bergé, Rencontres de Moriond, March 27, 2019
From space: e.g. advance of perigee (LAGEOS) or equivalence principle (MICROSCOPE —P. Fayet’s and M. Pernot-Borras’ talks)
Possible lack of consistency: most tests either - assume Earth = point mass (ignore Earth’s shape) - or use/correct lowest shape information (extended sphere,
oblateness) from Earth models obtained under Newtonian gravity assumption
Question: how do the shape of the Earth and a Yukawa deviation affect each other?
Yukawa deviation V(r) = −GM
r(1 + αe−r/λ)
Earth’s shape and gravity field
!4 Joel Bergé, Rencontres de Moriond, March 27, 2019
Two-way problem: invert gravity field to estimate Earth’s mass distribution vs predict gravity field from Earth’s mass distribution
GOCE (ESA)Gravity Field and Steady State Ocean Circulation Explorer, 2009-2013
GRACE (NASA-JPL): Gravity Recovery and Climate Experiment, 2002-2015
× [CNnm cos(mξ) + SN
nm sin(mξ)]
Newtonian gravity!
Spherical harmonics decomposition and Yukawa
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Gravity field of extended body
Taylor expansions
Legendre polynomials Spherical harmonics
JB, P. Brax, M. Pernot-Borras, J.P. Uzan, CQG 35 234001 (2018)
Joel Bergé, Rencontres de Moriond, March 27, 2019
Modified Bessel functions
Spherical harmonics decomposition and Yukawa
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Finally… body’s gravity potential
Joel Bergé, Rencontres de Moriond, March 27, 2019
ylm ∝ Clm − iSlmEasy link to usual Cnm/Snm coefficients
r-dependence!
Yukawa potential brings in a r-dependence
Earth’s shape — Yukawa twist
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Example: homogeneous oblate Earth (only y00 and y20 non-zero)
Form factor
Form factor
Joel Bergé, Rencontres de Moriond, March 27, 2019
Estimating y20 with non-zero Yukawa deviation
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Bias and systematic error if incorrectly assuming Newtonian gravity when inverting gravity field
Yukawa contribution at different altitudes
α α
λ[m] λ[m]Joel Bergé, Rencontres de Moriond, March 27, 2019
Constraining Yukawa from y20(r)
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estimator: compare J2 at two altitudesα
Uncertainty from imperfect knowledge of Earth’s shape and measurement error
uncertainty on oblateness
unce
rtain
ty o
n y 2
0
Joel Bergé, Rencontres de Moriond, March 27, 2019
Current uncertainties
Constraining Yukawa from y20(r): naive GOCE-GRACE comparison
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GOCE vs GRACE’s J2 => significant Yukawa deviation! Excluded for many years => underestimated errors in Earth gravity field models? Time-dependent systematics?
Joel Bergé, Rencontres de Moriond, March 27, 2019
Conclusion
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• Source’s shape and non-Newtonian gravity twisted
• Spherical harmonic decomposition: coefficients ylm are not universal in non-Newtonian gravity, depend on distance to the centre of the source
• Non-Newtonian component implies bias and extra systematic errors when inverting the measured gravity field to reconstruct the source’s shape: still a few orders of magnitude below measurement errors in space, but significant(?) on the ground
• Possibility to test Yukawa deviation by comparing ylm at different altitudes. Ideally, compare measurements taken simultaneously.
• Imperfect knowledge of the source affects constraints on Yukawa parameters: still subdominant compared to measurement errors
Joel Bergé, Rencontres de Moriond, March 27, 2019
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