Multi-messenger astronomy in the new physics modality with GPS constellation

Fuente: arXiv
Enregistré dans:
Détails bibliographiques
Auteurs principaux: Sen, Arko P., Pfeffer, Kalia, Ries, Paul, Blewitt, Geoffrey, Derevianko, Andrei
Format: Preprint
Publié: 2023
Sujets:
Accès en ligne:
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1866917996485672960
author Sen, Arko P.
Pfeffer, Kalia
Ries, Paul
Blewitt, Geoffrey
Derevianko, Andrei
author_facet Sen, Arko P.
Pfeffer, Kalia
Ries, Paul
Blewitt, Geoffrey
Derevianko, Andrei
contents We explore a novel, exotic physics, modality in multi-messenger astronomy. We are interested in exotic fields emitted by the mergers and their direct detection with a network of atomic clocks. We specifically focus on the rubidium clocks onboard satellites of the Global Positioning System. Bursts of exotic fields may be produced during the coalescence of black hole singularities, releasing quantum gravity messengers. To be detectable such fields must be ultralight and ultra-relativistic and we refer to them as exotic low-mass fields (ELFs). Since such fields possess non-zero mass, the ELF bursts lag behind the gravitational waves emitted by the very same merger. Then the gravitational wave observatories provide a detection trigger for the atomic clock networks searching for the feeble ELF signals. ELFs would imprint an anti-chirp transient across the sensor network. ELFs can be detectable by atomic clocks if they cause variations in fundamental constants. We report our progress in the development of techniques to search for ELF bursts with clocks onboard GPS satellites. We focus on the binary neutron star merger GW170817 of August 17, 2017. We find an intriguing excess in the clock noise post LIGO gravitational wave trigger. Potentially the excess noise could be explained away by the increased solar electron flux post LIGO trigger.
format Preprint
id arxiv_https___arxiv_org_abs_2312_12752
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Multi-messenger astronomy in the new physics modality with GPS constellation
Sen, Arko P.
Pfeffer, Kalia
Ries, Paul
Blewitt, Geoffrey
Derevianko, Andrei
Instrumentation and Methods for Astrophysics
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
Atomic Physics
Instrumentation and Detectors
We explore a novel, exotic physics, modality in multi-messenger astronomy. We are interested in exotic fields emitted by the mergers and their direct detection with a network of atomic clocks. We specifically focus on the rubidium clocks onboard satellites of the Global Positioning System. Bursts of exotic fields may be produced during the coalescence of black hole singularities, releasing quantum gravity messengers. To be detectable such fields must be ultralight and ultra-relativistic and we refer to them as exotic low-mass fields (ELFs). Since such fields possess non-zero mass, the ELF bursts lag behind the gravitational waves emitted by the very same merger. Then the gravitational wave observatories provide a detection trigger for the atomic clock networks searching for the feeble ELF signals. ELFs would imprint an anti-chirp transient across the sensor network. ELFs can be detectable by atomic clocks if they cause variations in fundamental constants. We report our progress in the development of techniques to search for ELF bursts with clocks onboard GPS satellites. We focus on the binary neutron star merger GW170817 of August 17, 2017. We find an intriguing excess in the clock noise post LIGO gravitational wave trigger. Potentially the excess noise could be explained away by the increased solar electron flux post LIGO trigger.
title Multi-messenger astronomy in the new physics modality with GPS constellation
topic Instrumentation and Methods for Astrophysics
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
Atomic Physics
Instrumentation and Detectors
url https://arxiv.org/abs/2312.12752