Phys. Rev. Lett. 87, 251302 (2001) [4 pages]

Estimate of the Primordial Magnetic Field Helicity

Download: PDF (94 kB) or Buy this Article (Use Article Pack) Export: BibTeX or EndNote (RIS)

Tanmay Vachaspati
Department of Astronomy and Astrophysics, Tata Institute of Fundamental Research, Homi Bhabha Road, Colaba, Mumbai 400005, India
and Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, Ohio 44106-7079

Received 22 January 2001; revised 2 October 2001; published 28 November 2001

Electroweak baryogenesis proceeds via changes in the non-Abelian Chern-Simons number. It is argued that these changes generate a primordial magnetic field with left-handed helicity. The helicity density of the primordial magnetic field today is then estimated to be given by ∼102nb, where nb∼10-6/cm3 is the present cosmological baryon number density. With certain assumptions about the inverse cascade we find that the field strength at recombination is ∼10-13  G on a comoving coherence scale ∼0.1 pc.


©2001 The American Physical Society

URL: http://link.aps.org/abstract/PRL/v87/e251302
DOI: 10.1103/PhysRevLett.87.251302
PACS: 98.62.En, 98.80.Cq

[ Abstract  |  Previous article  |  Next article  |  Issue 25 ]