Multimessenger cosmology: Correlating cosmic microwave background and stochastic gravitational wave background measurements
Journal Article
·
· Physical Review. D.
- Univ. of Illinois at Urbana-Champaign, IL (United States); OSTI
- Univ. of Waterloo, ON (Canada)
- Univ. of New South Wales, Sydney, NSW (Australia)
- Univ. of Portsmouth (United Kingdom); Consejo Superior de Investigaciones Cientificas (CSIC), Madrid (Spain); Autonomous Univ. of Madrid (Spain)
- King's College, London (United Kingdom)
- Swansea University (United Kingdom)
Characterizing the physical properties of the stochastic gravitational wave background (SGWB) is a key step towards identifying the nature of its possible origin. We focus our analysis on SGWB anisotropies. The existence of a nontrivial primordial scalar-tensor-tensor (STT) correlation in the squeezed configuration may be inferred from the effect that a long wavelength scalar mode has on the gravitational wave power spectrum: an anisotropic contribution. Crucially, such a contribution is correlated with temperature anisotropies in the cosmic microwave background (CMB). This paper shows that, for inflationary models that generate suitably large STT non-Gaussianities, cross correlating the CMB with the stochastic background of gravitational waves is a very effective probe of early universe physics. The resulting signal can be a smoking gun for primordial SGWB anisotropies.
- Research Organization:
- University of Illinois at Urbana-Champaign, IL (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC)
- Grant/Contract Number:
- SC0015655
- OSTI ID:
- 1852005
- Journal Information:
- Physical Review. D., Journal Name: Physical Review. D. Journal Issue: 2 Vol. 103; ISSN 2470-0010
- Publisher:
- American Physical Society (APS)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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