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Primordial Density Perturbations in Tepid Inflation

Published online by Cambridge University Press:  03 August 2017

B. Lukacs  and
G. Paal
B. Lukacs
Affiliation:
Central Research Institute for Physics, H-1525 Bp, T14, Pf.49, Budapest, Hungary
G. Paal
Affiliation:
Konkoly Observatory of the Hungarian Acadeiy of Sciences, H-1525 Bp, T14, Pf. 67, Budapest, Hungary

Extract

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Density fluctuations needed for galaxy formation may have thermal origin in a tepid inflation.

Type
Appendix 1: Poster Papers
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 514
Copyright
Copyright © Reidel 1988 

References

[1] Diosi, L. and Lukacs, B.: Phys. Lett. 112A, 13 (1985); Phys. Rev. 31A, 3415 (1985) Google Scholar
[2] Brandenberger, R. H.: Rev. Mod. Phys, 51, 1 (1985)Google Scholar
[3] Kampfer, B., Lukacs, B. and Paal, G.; Phys. Lett, B181, 11 (1987)Google Scholar