| dc.contributor.author |
Bhatt J.R. |
|
| dc.contributor.author |
Desai B.R. |
|
| dc.contributor.author |
Ma E. |
|
| dc.contributor.author |
Rajasekaran G. |
|
| dc.contributor.author |
Sarkar U. |
|
| dc.date.accessioned |
2023-10-13T12:37:29Z |
|
| dc.date.available |
2023-10-13T12:37:29Z |
|
| dc.date.issued |
2010 |
|
| dc.identifier |
10.1016/j.physletb.2010.02.079 |
|
| dc.identifier.issn |
3702693 |
|
| dc.identifier.uri |
https://dspace.imsc.res.in/xmlui/handle/123456789/704 |
|
| dc.identifier.uri |
https://doi.org/10.1016/j.physletb.2010.02.079 |
|
| dc.description.abstract |
We propose a new solution to the origin of dark energy. We suggest that it was created dynamically from the condensate of a singlet neutrino at a late epoch of the early Universe through its effective self-interaction. This singlet neutrino is also the Dirac partner of one of the three observed neutrinos, hence dark energy is related to neutrino mass. The onset of this condensate formation in the early Universe is also related to matter density and offers an explanation of the coincidence problem of why dark energy (70%) and total matter (30%) are comparable at the present time. We demonstrate this idea in a model of neutrino mass with (right-handed) singlet neutrinos and a singlet scalar. © 2010. |
|
| dc.language.iso |
en |
|
| dc.relation.ispartof |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Vol. 687, Issue. 1 |
|
| dc.rights |
Copyrighted by the Publisher |
|
| dc.source |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
|
| dc.subject |
Accelerated expansion |
|
| dc.subject |
Dark energy |
|
| dc.subject |
Neutrino condensates |
|
| dc.subject |
Superconductivity |
|
| dc.title |
Neutrino condensate as origin of dark energy |
|
| dc.description.pages |
75 - 78 |
|
| dc.relation.url |
https://doi.org/10.1016/j.physletb.2010.02.079 |
|
| dc.type |
Article |
|