The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.
The astrophysical gravitational wave stochastic background
Open accessAbstract
A stochastic background of gravitational waves with astrophysical origins may have resulted from the superposition of a large number of unresolved sources since the beginning of stellar activity. Its detection would put very strong constraints on the physical properties of compact objects, the initial mass function and star formation history. On the other hand, it could be a 'noise' that would mask the stochastic background of its cosmological origin. We review the main astrophysical processes which are able to produce a stochastic background and discuss how they may differ from the primordial contribution in terms of statistical properties. Current detection methods are also presented.
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Cites
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., et al. (1999) · The Astrophysical Journal · doi:10.1086/307221 · Cited by 18,062
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High-precision timing of millisecond pulsars. 3: Long-term monitoring of PSRs B1855+09 and B1937+21
Kaspi, V. M., Taylor, J. H., & Ryba, M. F. (1994) · The Astrophysical Journal · doi:10.1086/174280 · Cited by 595 · cited 2×
“Observations of PSR B1805+09 (Kaspi et al. 1994; Lommen et al. 2003), a very stable narrow profile millisecond pulsar, with the Arecibo and Green Bank radiotelescopes for over 17 years, give an upper limit of Ωgw ∼ 1.2×10−9 at the frequency f = 1Tobs = 1.86×10 −9 nHz, and combining the timings of seven pulsars citepje…”
BackgroundInfluential
Cited by
Primordial black holes—perspectives in gravitational wave astronomy
Sasaki, M., Suyama, T., Tanaka, T., & Yokoyama, S. (2018) · Classical and Quantum Gravity · doi:10.1088/1361-6382/aaa7b4 · Cited by 894
Population of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3
Abbott, R., Abbott, T. D., Acernese, F., Ackley, K., Adams, C., Adhikari, N., Adhikari, R. X., Adya, V. B., Affeldt, C., Agarwal, D., et al. (2023) · Physical Review X · doi:10.1103/physrevx.13.011048 · Cited by 889
Self-citationAstrophysics with the Laser Interferometer Space Antenna
Amaro-Seoane, P., Andrews, J., Arca Sedda, M., Askar, A., Baghi, Q., Balasov, R., Bartos, I., Bavera, S. S., Bellovary, J., Berry, C. P. L., et al. (2023) · Living Reviews in Relativity · doi:10.1007/s41114-022-00041-y · Cited by 609
Gravitational Waves Induced by Non-Gaussian Scalar Perturbations
Cai, R.-G., Pi, S., & Sasaki, M. (2019) · Physical Review Letters · doi:10.1103/physrevlett.122.201101 · Cited by 435
Stochastic gravitational wave backgrounds
Christensen, N. (2019) · Reports on Progress in Physics · doi:10.1088/1361-6633/aae6b5 · Cited by 316
Metadata
- Authors
- Regimbau, T.
- Venue
- Research in Astronomy and Astrophysics
- Publisher
- IOP Publishing
- Published
- 2011-03-25
- Volume
- 11
- Issue
- 4
- Pages
- 369-390
- ISSN
- 1674-4527 (ISSN-L)
- OpenAlex
- W2120549298
- Cited by
- 279
- References
- 3
- FWCI
- 5.19
- Type
- journal article
- Language
- en
- Open access
- bronze
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