Published April 1991
| Version v1
Journal article
Bosons - Hot dark matter with small-scale power
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.