The relevance of Very Light Dark Matter
A concordant model of Dark Matter and Dark Energy is presented. Dark Energy arises out of magnetic condensation of very light fermions of micro-eV mass charged under an unbroken gauge group U(1)X. The Dark Matter candidate is an oppositely charged fermionic species which is then shown to be natural...
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| Format: | Article |
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EDP Sciences
2014-04-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/20147000046 |
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doaj-d052975de22c4b8dadf367a7554d45bc2021-08-02T03:32:03ZengEDP SciencesEPJ Web of Conferences2100-014X2014-04-01700004610.1051/epjconf/20147000046epjconf_icfp2012_00046The relevance of Very Light Dark MatterYajnik Urjit A. A concordant model of Dark Matter and Dark Energy is presented. Dark Energy arises out of magnetic condensation of very light fermions of micro-eV mass charged under an unbroken gauge group U(1)X. The Dark Matter candidate is an oppositely charged fermionic species which is then shown to be naturally in the MeV to keV range. http://dx.doi.org/10.1051/epjconf/20147000046 |
| collection |
DOAJ |
| language |
English |
| format |
Article |
| sources |
DOAJ |
| author |
Yajnik Urjit A. |
| spellingShingle |
Yajnik Urjit A. The relevance of Very Light Dark Matter EPJ Web of Conferences |
| author_facet |
Yajnik Urjit A. |
| author_sort |
Yajnik Urjit A. |
| title |
The relevance of Very Light Dark Matter |
| title_short |
The relevance of Very Light Dark Matter |
| title_full |
The relevance of Very Light Dark Matter |
| title_fullStr |
The relevance of Very Light Dark Matter |
| title_full_unstemmed |
The relevance of Very Light Dark Matter |
| title_sort |
relevance of very light dark matter |
| publisher |
EDP Sciences |
| series |
EPJ Web of Conferences |
| issn |
2100-014X |
| publishDate |
2014-04-01 |
| description |
A concordant model of Dark Matter and Dark Energy is presented. Dark Energy arises out of magnetic condensation of very light fermions of micro-eV mass charged under an unbroken gauge group U(1)X. The Dark Matter candidate is an oppositely charged fermionic species which is then shown to be naturally in the MeV to keV range.
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| url |
http://dx.doi.org/10.1051/epjconf/20147000046 |
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AT yajnikurjita therelevanceofverylightdarkmatter AT yajnikurjita relevanceofverylightdarkmatter |
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