Mostra el registre parcial de l'element
dc.contributor.author | Semikoz, Victor B. | |
dc.contributor.author | Sokoloff, D.D. | |
dc.contributor.author | Furtado Valle, José Wagner | |
dc.date.accessioned | 2015-09-28T12:22:09Z | |
dc.date.available | 2015-09-28T12:22:09Z | |
dc.date.issued | 2009 | |
dc.identifier.citation | Semikoz, Victor B. Sokoloff, D.D. Furtado Valle, José Wagner 2009 Is the baryon asymmetry of the Universe related to galactic magnetic fields? Physical Review D 80 8 083510 | |
dc.identifier.uri | http://hdl.handle.net/10550/47384 | |
dc.description.abstract | A tiny hypermagnetic field generated before the electroweak phase transition (EWPT) associated to the generation of elementary particle masses can polarize the early Universe hot plasma at huge redshifts z > 10^15. The anomalous violation of the right-handed electron current characteristic of the EWPT converts the lepton asymmetry into a baryon asymmetry. Under reasonable approximations, the magnetic field strength inferred by requiring such 'leptogenic' origin for the observed baryon asymmetry of the Universe matches the large-scale cosmological magnetic field strengths estimated from current astronomical observations. | |
dc.language.iso | eng | |
dc.relation.ispartof | Physical Review D, 2009, vol. 80, num. 8, p. 083510 | |
dc.subject | Física | |
dc.title | Is the baryon asymmetry of the Universe related to galactic magnetic fields? | |
dc.type | journal article | es_ES |
dc.date.updated | 2015-09-28T12:22:10Z | |
dc.identifier.doi | 10.1103/PhysRevD.80.083510 | |
dc.identifier.idgrec | 059499 | |
dc.rights.accessRights | open access | es_ES |