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.
arXiv comment12 pages, 3 figures, 1 table. Accepted for publication in Phys. Rev. D
References in corpus (71)
- 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
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- Advanced LIGO
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- GW190425: Observation of a Compact Binary Coalescence with Total Mass
- 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
- Transient Events from Neutron Star Mergers
- A gravitational-wave standard siren measurement of the Hubble constant
- Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
- Interferometer design of the KAGRA gravitational wave detector
- 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
- Gravitational-wave constraints on the neutron-star-matter Equation of State
- Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger
- Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities
- 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
- KAGRA: 2.5 Generation Interferometric Gravitational Wave Detector
- What is the Most Promising Electromagnetic Counterpart of a Neutron Star Binary Merger?
- Detection methods for stochastic gravitational-wave backgrounds: a unified treatment
- The Sensitivity of the Advanced LIGO Detectors at the Beginning of Gravitational Wave Astronomy
- Upper Limits on the Isotropic Gravitational-Wave Background from Advanced LIGO's and Advanced Virgo's Third Observing Run
- A template bank for gravitational waveforms from coalescing binary black holes: non-spinning binaries
- Accretion during the merger of supermassive black holes
- 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
- Fermi GBM Observations of LIGO Gravitational Wave event GW150914
- Search for the isotropic stochastic background using data from Advanced LIGO's second observing run
- The Sensitivity of Ligo to a Stochastic Background, and its Dependance on the Detector Orientations
- The First Fermi LAT Gamma-Ray Burst Catalog
- IndIGO and LIGO-India: Scope and Plans for Gravitational Wave Research and Precision Metrology in India
- Dual Jets from Binary Black Holes
- Gravitational wave background from binary systems
- Mergers of Charged Black Holes: Gravitational Wave Events, Short Gamma-Ray Bursts, and Fast Radio Bursts
- Neutrino heating near hyper-accreting black holes
- Stochastic Gravitational Wave Background from Coalescing Binary Black Holes
- A year in the life of GW170817: the rise and fall of a structured jet from a binary neutron star merger
- Ram-pressure stripping of a kicked Hill sphere: Prompt electromagnetic emission from the merger of stellar mass black holes in an AGN accretion disk
- The afterglow and kilonova of the short GRB 160821B
- GROWTH on S190425z: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR
- Localization of Gamma-Ray Bursts using the Fermi Gamma-Ray Burst Monitor
- Characteristic Signatures in the Thermal Emission from Accreting Binary Black Holes
- Probing the anisotropies of a stochastic gravitational-wave background using a network of ground-based laser interferometers
- Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs
- Accessibility of the Gravitational-Wave Background due to Binary Coalescences to Second and Third Generation Gravitational-Wave Detectors
- 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
- Shouts and Murmurs: Combining Individual Gravitational-Wave Sources with the Stochastic Background to Measure the History of Binary Black Hole Mergers
- Gravitational wave radiometry: Mapping a stochastic gravitational wave background
- THESEUS: a key space mission concept for Multi-Messenger Astrophysics
- Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs
- Light-curve models of black hole - neutron star mergers: steps towards a multi-messenger parameter estimation
- Time-dependence of the astrophysical stochastic gravitational wave background
- Merging Rates of Compact Binaries in Galaxies: Perspectives for Gravitational Wave Detections
- Science Impacts of the SPHEREx All-Sky Optical to Near-Infrared Spectral Survey II: Report of a Community Workshop on the Scientific Synergies Between the SPHEREx Survey and Other Astronomy Observatories
- IceCube Search for Neutrinos Coincident with Compact Binary Mergers from LIGO-Virgo's First Gravitational-Wave Transient Catalog
- Inferring the lensing rate of LIGO-Virgo sources from the stochastic gravitational wave background
- WFIRST Science Investigation Team "Cosmology with the High Latitude Survey" Annual Report 2017
- Constraining the lensing of binary black holes from their stochastic background
- Stochastic background from extra-galactic double neutron stars
- Prospects for joint observations of gravitational waves and gamma rays from merging neutron star binaries
- The Gravitational-wave Optical Transient Observer (GOTO)
- Multibaseline gravitational wave radiometry
- Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
- The Probability Distribution of Astrophysical Gravitational-Wave Background Fluctuations
- Fermi GBM follow-up of LIGO-Virgo binary black hole mergers -- detection prospects
Cited by in corpus (11)
- Probing Anisotropies of the Stochastic Gravitational Wave Background with LISA
- Detection of Early-Universe Gravitational Wave Signatures and Fundamental Physics
- Can we distinguish astrophysical from primordial black holes via the stochastic gravitational wave background?
- 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