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Impact of LIGO-Virgo black hole binaries on gravitational wave background searches
by
Lewicki, Marek
, Vaskonen, Ville
in
Analysis
/ Astronomy
/ Astrophysics and Cosmology
/ Black holes
/ Detectors
/ Elementary Particles
/ Experiments
/ Gravitational waves
/ Hadrons
/ Heavy Ions
/ Measurement Science and Instrumentation
/ Nuclear Energy
/ Nuclear Physics
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Regular Article - Theoretical Physics
/ Searching
/ Sensors
/ Signal to noise ratio
/ Star & galaxy formation
/ String Theory
2023
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Impact of LIGO-Virgo black hole binaries on gravitational wave background searches
by
Lewicki, Marek
, Vaskonen, Ville
in
Analysis
/ Astronomy
/ Astrophysics and Cosmology
/ Black holes
/ Detectors
/ Elementary Particles
/ Experiments
/ Gravitational waves
/ Hadrons
/ Heavy Ions
/ Measurement Science and Instrumentation
/ Nuclear Energy
/ Nuclear Physics
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Regular Article - Theoretical Physics
/ Searching
/ Sensors
/ Signal to noise ratio
/ Star & galaxy formation
/ String Theory
2023
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Impact of LIGO-Virgo black hole binaries on gravitational wave background searches
by
Lewicki, Marek
, Vaskonen, Ville
in
Analysis
/ Astronomy
/ Astrophysics and Cosmology
/ Black holes
/ Detectors
/ Elementary Particles
/ Experiments
/ Gravitational waves
/ Hadrons
/ Heavy Ions
/ Measurement Science and Instrumentation
/ Nuclear Energy
/ Nuclear Physics
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Regular Article - Theoretical Physics
/ Searching
/ Sensors
/ Signal to noise ratio
/ Star & galaxy formation
/ String Theory
2023
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Impact of LIGO-Virgo black hole binaries on gravitational wave background searches
Journal Article
Impact of LIGO-Virgo black hole binaries on gravitational wave background searches
2023
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Overview
We study the impact of the black hole binary population currently probed by LIGO-Virgo on future searches for the primordial gravitational wave background. We estimate the foreground generated by the binaries using the observed event rate and a simple modeling of the black hole population. We subtract individually resolvable binaries from the foreground and utilize Fisher analysis to derive sensitivity curves for power-law signals including these astrophysical foregrounds. Even with optimistic assumptions, we find that the reach of future experiments will be severely reduced.
Publisher
Springer Berlin Heidelberg,Springer,Springer Nature B.V,SpringerOpen
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