Finite temperature corrections in SU(N, 1) supergravity

K. Enqvist; D. V. Nanopoulos; M. Quirós; K. A. Olive; M. Srednicki

doi:10.1016/0370-2693(85)91165-7

Finite temperature corrections in SU(N, 1) supergravity

K. Enqvist, D. V. Nanopoulos, M. Quirós, K. A. Olive, M. Srednicki

Physics and Astronomy (Twin Cities)

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Abstract

We compute finite temperature corrections to the scalar potential in maximally symmetric SU(N, 1) supergravity. In the large N limit, the zero temperature potential is only scaled by the thermal corrections. As an example, we apply the general result to a class of phenomenologically interesting no-scale supergravity models.

Original language	English (US)
Pages (from-to)	181-184
Number of pages	4
Journal	Physics Letters B
Volume	152
Issue number	3-4
DOIs	https://doi.org/10.1016/0370-2693(85)91165-7
State	Published - Mar 7 1985

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title = "Finite temperature corrections in SU(N, 1) supergravity",

abstract = "We compute finite temperature corrections to the scalar potential in maximally symmetric SU(N, 1) supergravity. In the large N limit, the zero temperature potential is only scaled by the thermal corrections. As an example, we apply the general result to a class of phenomenologically interesting no-scale supergravity models.",

author = "K. Enqvist and Nanopoulos, {D. V.} and M. Quir{\'o}s and Olive, {K. A.} and M. Srednicki",

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AU - Nanopoulos, D. V.

AU - Quirós, M.

AU - Olive, K. A.

AU - Srednicki, M.

PY - 1985/3/7

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N2 - We compute finite temperature corrections to the scalar potential in maximally symmetric SU(N, 1) supergravity. In the large N limit, the zero temperature potential is only scaled by the thermal corrections. As an example, we apply the general result to a class of phenomenologically interesting no-scale supergravity models.

AB - We compute finite temperature corrections to the scalar potential in maximally symmetric SU(N, 1) supergravity. In the large N limit, the zero temperature potential is only scaled by the thermal corrections. As an example, we apply the general result to a class of phenomenologically interesting no-scale supergravity models.

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Finite temperature corrections in SU(N, 1) supergravity

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