dc.contributor.author |
Sivaram, C |
|
dc.contributor.author |
Arun, K |
|
dc.contributor.author |
Prasad, A |
|
dc.date.accessioned |
2020-11-14T07:30:46Z |
|
dc.date.available |
2020-11-14T07:30:46Z |
|
dc.date.issued |
2018-10 |
|
dc.identifier.citation |
Astrophysics and Space Science, Vol. 363, 202 |
en_US |
dc.identifier.issn |
1572-946X |
|
dc.identifier.uri |
http://prints.iiap.res.in/handle/2248/7017 |
|
dc.description |
Restricted Access © Springer The original publication is available at springerlink.com https://doi.org/10.1007/s10509-018-3428-5 |
en_US |
dc.description.abstract |
Formation of black holes may be constrained by intrinsic parameters characterizing them such as electric charge. Here we discuss the effects of a relatively minute excess of charge on extremal black hole formation and the horizon. We extend the implications of this argument to the formation of primordial black holes (PBH) in the early universe which gives a possible reason for the lack of detection of Hawking radiation. These charge limits also apply to dark matter (DM) particles that may form PHBs in the early universe. The constraint thus obtained on the electric charge of DM particles could also account for the required magnitude of the repulsive dark energy (DE) currently causing an accelerated universe which provides a possible unified picture of DM and DE. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Springer |
en_US |
dc.subject |
Extremal black hole |
en_US |
dc.subject |
Primordial black holes |
en_US |
dc.subject |
Dark matter |
en_US |
dc.subject |
Dark energy |
en_US |
dc.title |
Extremal charged black holes, dark matter and dark energy |
en_US |
dc.type |
Article |
en_US |