期刊
PHYSICS LETTERS B
卷 528, 期 3-4, 页码 193-198出版社
ELSEVIER SCIENCE BV
DOI: 10.1016/S0370-2693(02)01200-5
关键词
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General expressions are given for the generation of Primordial Black Holes (PBH) in a universe with a presently accelerated expansion due to an (effective) cosmological constant. We give expressions both for a powerlaw scalefree primordial spectrum and for spectra which are not of that type. Specializing to the case of a pure cosmological constant A and assuming flatness, we show that a cosmological constant with Omega(Lambda,0) = 0.7 will decrease the mass variance at the PBH formation time by about 15% compared with a critical density universe. (C) 2002 Elsevier Science B.V All rights reserved.
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