dc.contributor.author |
Poddar, Tanmay Kumar |
|
dc.contributor.author |
Pachhar, Debashis |
|
dc.coverage.spatial |
United States of America |
|
dc.date.accessioned |
2023-02-22T06:52:40Z |
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dc.date.available |
2023-02-22T06:52:40Z |
|
dc.date.issued |
2023-02 |
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dc.identifier.citation |
Poddar, Tanmay Kumar and Pachhar, Debashis, "Constraints on monopole-dipole potential from the tests of gravity: first bounds from single astrophysical observations", arXiv, Cornell University Library, DOI: arXiv:2302.03882, Feb. 2023. |
en_US |
dc.identifier.uri |
http://arxiv.org/abs/2302.03882 |
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dc.identifier.uri |
https://repository.iitgn.ac.in/handle/123456789/8580 |
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dc.description.abstract |
Ultralight Axion Like Particle (ALP) can mediate a long range monopole-dipole macroscopic force between Earth and Sun if Earth is treated as a polarized source. There are about 1042 number of polarized electrons in Earth due to the presence of the geomagnetic field. The monopole-dipole interactions between electrons in Earth and nucleons in Sun can influence the perihelion precession of Earth, gravitational light bending and Shapiro time delay. The contribution of monopole-dipole potential is limited to be no larger than the measurement uncertainty. We obtain the first bound on monopole-dipole strength from single astrophysical observations. The perihelion precession of Earth puts the stronger bound on monopole-dipole coupling strength as gSgP≲3.62×10−11 for the ALP of mass ma≲1.35×10-18 eV |
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dc.description.statementofresponsibility |
by Tanmay Kumar Poddar and Debashis Pachhar |
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dc.language.iso |
en_US |
en_US |
dc.publisher |
Cornell University Library |
en_US |
dc.subject |
ALP |
en_US |
dc.subject |
Monopole-dipole macroscopic force |
en_US |
dc.subject |
Shapiro time delay |
en_US |
dc.subject |
Polarized source |
en_US |
dc.subject |
Perihelion precession |
en_US |
dc.title |
Constraints on monopole-dipole potential from the tests of gravity: first bounds from single astrophysical observations |
en_US |
dc.type |
Pre-Print Archive |
en_US |
dc.relation.journal |
arXiv |
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