Published April 1991 | Version v1
Journal article

Bosons - Hot dark matter with small-scale power

Creators

  • 1. Aarhus, University, Denmark (USA)

Description

An alternative hot dark matter scenario which considers low-mass bosons rather than neutrinos is suggested which has much more small-scale power than the neutrino hot dark matter model while keeping the power peak at large scales comparable to the comoving length scale set by neutrino free-streaming. The reason is that, for a given particle mass, the Bose-Einstein distribution has more low-velocity particles than the corresponding Fermi-Dirac distribution. Therefore, an appreciable fraction of particles stay close to their initial positions, so that even though the mean free-streaming length is similar to that for neutrinos, a fair amount of power survives on small scales. 9 refs

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
371
Series
Astrophys. J.
Journal Page Range
L47-L49
ISSN
0004-637X
CODEN
ASJOA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
22079012
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BOSONS; COSMOLOGICAL MODELS; COSMOLOGY; DEGREES OF FREEDOM; GALACTIC EVOLUTION; MASS; NEUTRINOS; NONLUMINOUS MATTER; TEMPERATURE DEPENDENCE
Descriptors DEC
ELEMENTARY PARTICLES; FERMIONS; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; MATTER

Optional Information

Notes
L47-L49.