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• W1801239452 abstract "If inflation was preceded by a radiation era, then at the time of inflation there will exist a decoupled thermal distribution of gravitons. Gravitational waves generated during inflation will be amplified by the process of stimulated emission into the existing thermal distribution of gravitons. Consequently, the usual zero temperature scale invariant tensor spectrum is modified by a temperature dependent factor. This thermal correction factor amplifies the B-mode polarization of the cosmic microwave background radiation by an order of magnitude at large angles, which may now be in the range of observability of the Wilkinson Microwave Anisotropy Probe." @default.
• W1801239452 created "2016-06-24" @default.
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• W1801239452 date "2006-12-18" @default.
• W1801239452 modified "2023-09-26" @default.
• W1801239452 title "Enhanced Polarization of the Cosmic Microwave Background Radiation from Thermal Gravitational Waves" @default.
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• W1801239452 doi "https://doi.org/10.1103/physrevlett.97.251301" @default.
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