Primordial magnetic field and kinetic theory with Berry curvature

Show simple item record

dc.contributor.author Bhatt, Jitesh R.
dc.contributor.author Pandey, Arun Kumar
dc.date.accessioned 2015-03-25T10:12:59Z
dc.date.available 2015-03-25T10:12:59Z
dc.date.issued 2015-03
dc.identifier.citation Bhatt, Jitesh R. and Pandey, Arun Kumar, “Primordial magnetic field and kinetic theory with Berry curvature”, arXiv, Cornell University Library, DOI: arXiv:1503.01878, Mar. 2015. en_US
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/1646
dc.description.abstract We apply the modified kinetic theory to study generation of magnetic field due to anomaly in a primordial plasma of the standard model particles at temperature T >80 TeV. It is known that achiral imbalance in such plasma can lead to instabilities responsible for the origin of the magneticfields. We have shown that inclusion of the Berry curvature term in the kinetic equation alongwith the collision term in the ralaxation approximation canlead to the chiral vorticity effect. Thiseffect was not considered in the earlier literature based on the heuristic application of the kinetictheory. But in the collisionless regime there may not be any vorticity generation. We also arguedthat the chiral imbalance in the collisionless regime remains subdominant for the primordial plasmacompared to the case where the collisions are important. en_US
dc.description.statementofresponsibility by Jitesh R. Bhatt and Arun Kumar Pandey
dc.language.iso en en_US
dc.publisher Cornell University Library en_US
dc.subject Berry curvature en_US
dc.subject Kinetic theory en_US
dc.subject Magnetic fields en_US
dc.subject Plasma en_US
dc.title Primordial magnetic field and kinetic theory with Berry curvature en_US
dc.type Preprint en_US


Files in this item

Files Size Format View

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record

Search Digital Repository


Browse

My Account