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• W2039930002 abstract "Primordial black holes (PBHs) can form in the early Universe via the collapse of large density perturbations. There are tight constraints on the abundance of PBHs formed due to their gravitational effects and the consequences of their evaporation. These abundance constraints can be used to constrain the primordial power spectrum, and hence models of inflation, on scales far smaller than those probed by cosmological observations. We compile, and where relevant update, the constraints on the abundance of PBHs before calculating the constraints on the curvature perturbation, taking into account the growth of density perturbations prior to horizon entry. We consider two simple parametrizations of the curvature perturbation spectrum on the scale of interest: constant and power-law. The constraints from PBHs on the amplitude of the power spectrum are typically in the range ${10}^{ensuremath{-}2}--{10}^{ensuremath{-}1}$ with some scale dependence." @default.
• W2039930002 created "2016-06-24" @default.
• W2039930002 creator A5014963573 @default.
• W2039930002 creator A5026066309 @default.
• W2039930002 creator A5089031708 @default.
• W2039930002 date "2009-05-20" @default.
• W2039930002 modified "2023-09-23" @default.
• W2039930002 title "Generalized constraints on the curvature perturbation from primordial black holes" @default.
• W2039930002 cites W1509168094 @default.
• W2039930002 cites W1823193264 @default.
• W2039930002 cites W1965202898 @default.
• W2039930002 cites W1965864871 @default.
• W2039930002 cites W1973368884 @default.
• W2039930002 cites W1974098534 @default.
• W2039930002 cites W1982657801 @default.
• W2039930002 cites W1985318134 @default.
• W2039930002 cites W1986054395 @default.
• W2039930002 cites W1987323465 @default.
• W2039930002 cites W1988144585 @default.
• W2039930002 cites W1988993357 @default.
• W2039930002 cites W1993692677 @default.
• W2039930002 cites W1996645546 @default.
• W2039930002 cites W1998388948 @default.
• W2039930002 cites W1998431825 @default.
• W2039930002 cites W2003384852 @default.
• W2039930002 cites W2005024908 @default.
• W2039930002 cites W2008059488 @default.
• W2039930002 cites W2008075884 @default.
• W2039930002 cites W2012357430 @default.
• W2039930002 cites W2012869431 @default.
• W2039930002 cites W2013529620 @default.
• W2039930002 cites W2015543356 @default.
• W2039930002 cites W2016770316 @default.
• W2039930002 cites W2020014379 @default.
• W2039930002 cites W2020790161 @default.
• W2039930002 cites W2024447830 @default.
• W2039930002 cites W2026926262 @default.
• W2039930002 cites W2031013908 @default.
• W2039930002 cites W2031350292 @default.
• W2039930002 cites W2031430331 @default.
• W2039930002 cites W2032375827 @default.
• W2039930002 cites W2035649997 @default.
• W2039930002 cites W2036422095 @default.
• W2039930002 cites W2037049681 @default.
• W2039930002 cites W2038455887 @default.
• W2039930002 cites W2042043669 @default.
• W2039930002 cites W2043885810 @default.
• W2039930002 cites W2044260983 @default.
• W2039930002 cites W2057201186 @default.
• W2039930002 cites W2057980978 @default.
• W2039930002 cites W2062182342 @default.
• W2039930002 cites W2062339379 @default.
• W2039930002 cites W2065805883 @default.
• W2039930002 cites W2065823041 @default.
• W2039930002 cites W2066838282 @default.
• W2039930002 cites W2072549870 @default.
• W2039930002 cites W2072606360 @default.
• W2039930002 cites W2072820732 @default.
• W2039930002 cites W2077000898 @default.
• W2039930002 cites W2078768185 @default.
• W2039930002 cites W2079685375 @default.
• W2039930002 cites W2080426263 @default.
• W2039930002 cites W2082627752 @default.
• W2039930002 cites W2084112171 @default.
• W2039930002 cites W2086624850 @default.
• W2039930002 cites W2088669741 @default.
• W2039930002 cites W2089005876 @default.
• W2039930002 cites W2090386790 @default.
• W2039930002 cites W2096676597 @default.
• W2039930002 cites W2107875899 @default.
• W2039930002 cites W2108255833 @default.
• W2039930002 cites W2127185383 @default.
• W2039930002 cites W2128443531 @default.
• W2039930002 cites W2136696603 @default.
• W2039930002 cites W2143513913 @default.
• W2039930002 cites W2150904269 @default.
• W2039930002 cites W2922507461 @default.
• W2039930002 cites W2986218762 @default.
• W2039930002 cites W3101239365 @default.
• W2039930002 cites W3101478357 @default.
• W2039930002 cites W3101968594 @default.
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• W2039930002 cites W3103122522 @default.
• W2039930002 cites W3104696400 @default.
• W2039930002 cites W3104906012 @default.
• W2039930002 cites W3106157645 @default.
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• W2039930002 doi "https://doi.org/10.1103/physrevd.79.103520" @default.
• W2039930002 hasPublicationYear "2009" @default.
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