dc.contributor.author |
Gupta V. |
|
dc.contributor.author |
Rajasekaran G. |
|
dc.date.accessioned |
2023-10-13T12:37:32Z |
|
dc.date.available |
2023-10-13T12:37:32Z |
|
dc.date.issued |
1969 |
|
dc.identifier |
10.1016/0550-3213(69)90276-4 |
|
dc.identifier.issn |
5503213 |
|
dc.identifier.uri |
https://dspace.imsc.res.in/xmlui/handle/123456789/806 |
|
dc.identifier.uri |
https://doi.org/10.1016/0550-3213(69)90276-4 |
|
dc.description.abstract |
We consider the commutation relations of the vector and axial-vector current densities. Assuming that the commutators of the time components are given (with no Schwinger terms) we derive conditions imposed by covariance on the Schwinger terms in the commutators of the space-time and space-space components of the currents. © 1969. |
|
dc.language.iso |
en |
|
dc.relation.ispartof |
Nuclear Physics, Section B, Vol. 10, Issue. 1 |
|
dc.rights |
Copyrighted by the Publisher |
|
dc.source |
Nuclear Physics, Section B |
|
dc.title |
Restrictions on Schwinger terms due to Lorentz covariance |
|
dc.description.pages |
11 - 16 |
|
dc.relation.url |
https://doi.org/10.1016/0550-3213(69)90276-4 |
|
dc.type |
Article |
|