| dc.contributor.author | Sengupta, S | |
| dc.contributor.author | Pal, B. P | |
| dc.date.accessioned | 2008-08-04T04:23:37Z | |
| dc.date.available | 2008-08-04T04:23:37Z | |
| dc.date.issued | 1996-01 | |
| dc.identifier.citation | Physics Letters B, Vol. 365, No. 1 - 4, pp.175 - 177 | en |
| dc.identifier.issn | 0370-2693 | |
| dc.identifier.uri | http://hdl.handle.net/2248/2976 | |
| dc.description | Restricted Access | |
| 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 | |
| dc.format.mimetype | application/pdf | |
| 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 | |
| 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 |