CBR temperature fluctuations induced by gravitational waves in a spatially 
closed inflationary universe

Allen, Bruce; Caldwell, R. R.; Koranda, Scott

doi:10.1103/PhysRevD.51.1553

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CBR temperature fluctuations induced by gravitational waves in a spatially closed inflationary universe

MPG-Autoren

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Allen, Bruce
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Koranda, Scott
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Zitation

Allen, B., Caldwell, R. R., & Koranda, S. (1995). CBR temperature fluctuations induced by gravitational waves in a spatially closed inflationary universe. Physical Review D, 51(4), 1553-1562. doi:10.1103/PhysRevD.51.1553.

Zitierlink: https://hdl.handle.net/11858/00-001M-0000-0013-5BA8-9

Zusammenfassung

Primordial gravitational waves are created during the de Sitter phase of an exponentially, expanding (inflationary) universe, due to quantum zero-point vacuum fluctuations. These waves produce fluctuations in the temperature of the cosmic background radiation (CBR). We calculate the multipole moments of the correlation function for these temperature fluctuations in a spatially closed Friedmann-Robertson-Walker (FRW) cosmological model. The results are compared to the corresponding multipoles in the spatially flat case. The differences are small unless the density parameter today, Ω0, is greater than 2.