Gauge invariance and equations of motion for closed string modes

We continue earlier discussions on loop variables and the exact renormalization group on the string world sheet for closed and open string backgrounds. The world sheet action with a UV regulator is written in a generally background covariant way by introducing a background metric. It is shown that t...

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Main Author: B. Sathiapalan
Format: Article
Language:English
Published: Elsevier 2014-12-01
Series:Nuclear Physics B
Online Access:http://www.sciencedirect.com/science/article/pii/S0550321314002983
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spelling doaj-1b5daafd2fe448e896bb15f1748cee492020-11-24T23:07:49ZengElsevierNuclear Physics B0550-32131873-15622014-12-01889C26129810.1016/j.nuclphysb.2014.09.020Gauge invariance and equations of motion for closed string modesB. SathiapalanWe continue earlier discussions on loop variables and the exact renormalization group on the string world sheet for closed and open string backgrounds. The world sheet action with a UV regulator is written in a generally background covariant way by introducing a background metric. It is shown that the renormalization group gives background covariant equations of motion – this is the gauge invariance of the graviton. Interaction is written in terms of gauge invariant and generally covariant field strength tensors. The basic idea is to work in Riemann normal coordinates and covariantize the final equation. It turns out that the equations for massive modes are gauge invariant only if the space–time curvature of the (arbitrary) background is zero. The exact RG equations give quadratic equations of motion for all the modes including the physical graviton. The level (2,2¯) massive field equations are used to illustrate the techniques. At this level there are mixed symmetry tensors. Gauge invariant interacting equations can be written down. In flat space an action can also be written for the free theory.http://www.sciencedirect.com/science/article/pii/S0550321314002983
collection DOAJ
language English
format Article
sources DOAJ
author B. Sathiapalan
spellingShingle B. Sathiapalan
Gauge invariance and equations of motion for closed string modes
Nuclear Physics B
author_facet B. Sathiapalan
author_sort B. Sathiapalan
title Gauge invariance and equations of motion for closed string modes
title_short Gauge invariance and equations of motion for closed string modes
title_full Gauge invariance and equations of motion for closed string modes
title_fullStr Gauge invariance and equations of motion for closed string modes
title_full_unstemmed Gauge invariance and equations of motion for closed string modes
title_sort gauge invariance and equations of motion for closed string modes
publisher Elsevier
series Nuclear Physics B
issn 0550-3213
1873-1562
publishDate 2014-12-01
description We continue earlier discussions on loop variables and the exact renormalization group on the string world sheet for closed and open string backgrounds. The world sheet action with a UV regulator is written in a generally background covariant way by introducing a background metric. It is shown that the renormalization group gives background covariant equations of motion – this is the gauge invariance of the graviton. Interaction is written in terms of gauge invariant and generally covariant field strength tensors. The basic idea is to work in Riemann normal coordinates and covariantize the final equation. It turns out that the equations for massive modes are gauge invariant only if the space–time curvature of the (arbitrary) background is zero. The exact RG equations give quadratic equations of motion for all the modes including the physical graviton. The level (2,2¯) massive field equations are used to illustrate the techniques. At this level there are mixed symmetry tensors. Gauge invariant interacting equations can be written down. In flat space an action can also be written for the free theory.
url http://www.sciencedirect.com/science/article/pii/S0550321314002983
work_keys_str_mv AT bsathiapalan gaugeinvarianceandequationsofmotionforclosedstringmodes
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