dc.contributor.author |
Sengupta, S |
|
dc.contributor.author |
Pal, B. P |
|
dc.date.accessioned |
2008-08-04T04:23:37Z |
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dc.date.available |
2008-08-04T04:23:37Z |
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dc.date.issued |
1996-01 |
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dc.identifier.citation |
Physics Letters B, Vol. 365, No. 1 - 4, pp.175 - 177 |
en |
dc.identifier.issn |
0370-2693 |
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dc.identifier.uri |
http://hdl.handle.net/2248/2976 |
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dc.description |
Restricted Access |
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dc.description.abstract |
We point out that an overall electric charge asymmetry in the universe will generate an anisotropy in the cosmic microwave background radiation (CMBR) via the Sach-Wolfe effect. From this, an upper limit on the electric charge asymmetry over a cosmological scale is found using the COBE data, which implies ΔT/T ≤ 10−4 for the CMBR. The same argument constrains the charge of degenerate neutrinos. |
en |
dc.format.extent |
3894 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Elsevier B.V |
en |
dc.relation.uri |
http://dx.doi.org/10.1016/0370-2693(95)01261-3 |
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dc.subject |
Cosmic microwave background radiation |
en |
dc.subject |
Neutrinos |
en |
dc.title |
Constraints on cosmic electric charge asymmetry and neutrino charge from the microwave background |
en |
dc.type |
Article |
en |