Supersymmetry and gravitational quadrupoles

被引:4
|
作者
Giannakis, I
Liu, JT
Porrati, M
机构
[1] Rockefeller Univ, Dept Phys, New York, NY 10021 USA
[2] NYU, Dept Phys, New York, NY 10003 USA
[3] CERN, Div Theory, CH-1211 Geneva, Switzerland
[4] Univ Michigan, Randall Lab Phys, Ann Arbor, MI 48109 USA
基金
美国国家科学基金会;
关键词
D O I
10.1016/S0370-2693(99)01264-2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We derive model independent, non-perturbative supersymmetric sum rules for the gravitational quadrupole moments of arbitrary-spin particles in any N = 1 supersymmetric theory. These sum rules select a ''preferred'' value of h = 1 where the "h-factor" is the gravitational quadrupole analog of the gyromagnetic ratio or g-factor. This value of h = 1 corresponds identically to the preferred field theory value obtained by tree-level unitarity considerations. The presently derived h-factor sum rule complements and generalizes previous work on electromagnetic moments where g = 2 was shown to be preferred by both supersymmetric sum rule and tree-level unitarity arguments. (C) 1999 Published by Elsevier Science B.V. All rights reserved.
引用
收藏
页码:129 / 135
页数:7
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