| dc.contributor.author |
Chattopadhyay, P. |
|
| dc.contributor.author |
Chaudhuri, Arnab |
|
| dc.contributor.author |
Khlopov, M. Yu. |
|
| dc.coverage.spatial |
United States of America |
|
| dc.date.accessioned |
2022-10-07T13:27:06Z |
|
| dc.date.available |
2022-10-07T13:27:06Z |
|
| dc.date.issued |
2022-09 |
|
| dc.identifier.citation |
Chattopadhyay, P.; Chaudhuri, Arnab and Khlopov, M. Yu., "Dark Matter from evaporating PBH dominated in the early universe", arXiv, Cornell University Library, DOI: arXiv:2209.11288, Sep. 2022. |
en_US |
| dc.identifier.uri |
https://arxiv.org/abs/2209.11288 |
|
| dc.identifier.uri |
https://repository.iitgn.ac.in/handle/123456789/8194 |
|
| dc.description.abstract |
Primordial Black Holes (PBH) could dominate in the early Universe and, evaporating before Big bang Nucleosynthesis, can provide new freeze in mechanism of dark matter (DM) production. The proposed scenario is considered for two possible mechanisms of PBH formation and the corresponding continuous PBH mass spectra so that the effect of non-single PBH mass spectrum is taken into account in the results of PBH evaporation, by which PBH dominance in the early Universe ends. We specify the conditions under which the proposed scenario can explain production of dark matter in very early Universe. |
|
| dc.description.statementofresponsibility |
by P. Chattopadhyay, Arnab Chaudhuri and M. Yu. Khlopov |
|
| dc.language.iso |
en_US |
en_US |
| dc.publisher |
Cornell University Library |
en_US |
| dc.subject |
PBH |
en_US |
| dc.subject |
Dark matter |
en_US |
| dc.subject |
Big bang nucleosynthesis |
en_US |
| dc.subject |
Extended mass spectrum |
en_US |
| dc.subject |
ZN |
en_US |
| dc.title |
Dark Matter from evaporating PBH dominated in the early universe |
en_US |
| dc.type |
Pre-Print Archive |
en_US |
| dc.relation.journal |
arXiv |
|