Fundamental physics using the temporal gravitational wave background
arXiv:2008.01082 · doi:10.1103/PhysRevD.104.063518
Abstract
We propose a novel probe of fundamental physics that involves the exploration of temporal correlations between the multi-frequency electromagnetic (EM) signal and the sub-threshold GW signal or stochastic gravitational wave background (SGWB) originating from coalescing binaries. This method will be useful for the detection of EM counterparts associated with the sub-threshold/SGWB signal. Exploiting the time delay between concomitant emission of the gravitational wave and EM signals enables inference of the redshifts of the contributing sources by studying the time delay dilation due to cosmological expansion, provided that the time-lag between the emission of gravitational wave signal and the EM signal acts like a standard clock. Measurement of the inevitable time-domain correlations between different frequencies of gravitational and EM waves, most notably in gamma-rays, will test several aspects of fundamental physics and gravitation theory, and enable a new pathway for current and future gravitational wave telescopes to study the universal nature of binary compact objects to high redshifts.
12 pages, 3 figures, 1 table. Accepted for publication in Phys. Rev. D
References in corpus (30)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- Advanced LIGO
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
- Laser Interferometer Space Antenna
- GW190521: A Binary Black Hole Merger with a Total Mass of
- A gravitational-wave standard siren measurement of the Hubble constant
- Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models
- Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger
- Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart
- Upper Limits on the Isotropic Gravitational-Wave Background from Advanced LIGO's and Advanced Virgo's Third Observing Run
- Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. V. Rising X-ray Emission from an Off-Axis Jet
- Localization of Gamma-Ray Bursts using the Fermi Gamma-Ray Burst Monitor
- Characteristic Signatures in the Thermal Emission from Accreting Binary Black Holes
- Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs
- Optical follow-up of the neutron star-black hole mergers S200105ae and S200115j
- General Relativistic Simulations of Magnetized Plasmas around Merging Supermassive Black Holes
- Accretion disks around binary black holes of unequal mass: GRMHD simulations of postdecoupling and merger
- Gravitational wave radiometry: Mapping a stochastic gravitational wave background
- Light-curve models of black hole - neutron star mergers: steps towards a multi-messenger parameter estimation
- IceCube Search for Neutrinos Coincident with Compact Binary Mergers from LIGO-Virgo's First Gravitational-Wave Transient Catalog
- Stochastic background from extra-galactic double neutron stars
- The Gravitational-wave Optical Transient Observer (GOTO)
- Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
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- Stochastic gravitational-wave background as a tool to investigate multi-channel astrophysical and primordial black-hole mergers
- Prospects of discovering sub-solar primordial black holes using the stochastic gravitational wave background from third-generation detectors
- Testing the Early Universe with Anisotropies of the Gravitational Wave Background
- Precision cosmology with primordial GW backgrounds in presence of astrophysical foregrounds
- Unraveling Cosmological Anisotropies within Stochastic Gravitational Wave Backgrounds
- A stochastic search for intermittent gravitational-wave backgrounds
- Spectrogram correlated stacking: A novel time-frequency domain analysis of the Stochastic Gravitational Wave Background
- A New Framework to Detect Multi-Messenger Signals from Bright Sporadic Stochastic Gravitational Wave Background