Primordial black hole formation in supergravity - art. no. 043512.

Citation
M. Kawasaki et T. Yanagida, Primordial black hole formation in supergravity - art. no. 043512., PHYS REV D, 5904(4), 1999, pp. 3512
Citations number
32
Categorie Soggetti
Physics
Journal title
PHYSICAL REVIEW D
ISSN journal
05562821 → ACNP
Volume
5904
Issue
4
Year of publication
1999
Database
ISI
SICI code
0556-2821(19990215)5904:4<3512:PBHFIS>2.0.ZU;2-L
Abstract
We study a double inflation model (a preinflation + a new inflation) in sup ergravity and discuss the formation of primordial black holes which may be identified with massive compact halo objects (MACHOs) observed in the halo of our galaxy. The preinflation drives an inflaton for the new inflation cl ose to the origin through supergravity effects and the new inflation natura lly occurs. If the total e-fold number of the new inflation is smaller than similar to 60, both inflations produce cosmologically relevant density flu ctuations. If the coherent inflaton oscillation after the preinflation cont inues until the beginning of the new inflation, density fluctuations on sma ll cosmological scales can be set suitably large to produce black holes MAC HOs of masses similar to 1M(.) in a wide region of parameter space in the d ouble inflation model. [S0556-2821(99)03402-5].