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• W3099989555 startingPage "017" @default.
• W3099989555 abstract "Measuring the primordial power spectrum on small scales is a powerful tool in inflation model building, yet constraints from Cosmic Microwave Background measurements alone are insufficient to place bounds stringent enough to be appreciably effective. For the very small scale spectrum, those which subtend angles of less than 0.3 degrees on the sky, an upper bound can be extracted from the astrophysical constraints on the possible production of primordial black holes in the early universe. A recently discovered observational by-product of an enhanced power spectrum on small scales, induced gravitational waves, have been shown to be within the range of proposed space based gravitational wave detectors; such as NASA's LISA and BBO detectors, and the Japanese DECIGO detector. In this paper we explore the impact such a detection would have on models of inflation known to lead to an enhanced power spectrum on small scales, namely the Hilltop-type and running mass models. We find that the Hilltop-type model can produce observable induced gravitational waves within the range of BBO and DECIGO for integral and fractional powers of the potential within a reasonable number of e-folds. We also find that the running mass model can produce a spectrum within the range of these detectors, but require that inflation terminates after an unreasonably small number of e-folds. Finally, we argue that if the thermal history of the Universe were to accomodate such a small number of e-folds the Running Mass Model can produce Primordial Black Holes within a mass range compatible with Dark Matter, i.e. within a mass range 10^{20}g< M_{BH}<10^{27}g." @default.
• W3099989555 created "2020-11-23" @default.
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• W3099989555 date "2012-09-13" @default.
• W3099989555 modified "2023-10-13" @default.
• W3099989555 title "Observable spectra of induced gravitational waves from inflation" @default.
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• W3099989555 cites W1970384842 @default.
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• W3099989555 cites W1973330634 @default.
• W3099989555 cites W1973852867 @default.
• W3099989555 cites W1976359759 @default.
• W3099989555 cites W1980512476 @default.
• W3099989555 cites W1980672343 @default.
• W3099989555 cites W1985372504 @default.
• W3099989555 cites W1988840549 @default.
• W3099989555 cites W1990044200 @default.
• W3099989555 cites W1990069578 @default.
• W3099989555 cites W1996957291 @default.
• W3099989555 cites W2005783817 @default.
• W3099989555 cites W2007931415 @default.
• W3099989555 cites W2010567060 @default.
• W3099989555 cites W2017312540 @default.
• W3099989555 cites W2023841217 @default.
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• W3099989555 cites W2050168982 @default.
• W3099989555 cites W2050287430 @default.
• W3099989555 cites W2052177627 @default.
• W3099989555 cites W2055558232 @default.
• W3099989555 cites W2057037672 @default.
• W3099989555 cites W2057691056 @default.
• W3099989555 cites W2058307417 @default.
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• W3099989555 cites W2077324434 @default.
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• W3099989555 cites W2080690817 @default.
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• W3099989555 cites W2167435391 @default.
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• W3099989555 cites W3100974022 @default.
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• W3099989555 doi "https://doi.org/10.1088/1475-7516/2012/09/017" @default.
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