Two-measure theory with third-rank antisymmetric tensor for local scale symmetry breaking

被引:0
|
作者
Guendelman, Eduardo [1 ]
Nishino, Hitoshi [2 ]
Rajpoot, Subhash [2 ]
机构
[1] Ben Gurion Univ Negev, Dept Phys, IL-84105 Beer Sheva, Israel
[2] Calif State Univ Long Beach, Dept Phys & Astron, 1250 Bellflower Blvd, Long Beach, CA 90840 USA
关键词
SUPERSYMMETRY; SUPERGRAVITY; INVARIANCE;
D O I
10.1103/PhysRevD.95.065002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a new mechanism of local scale symmetry breaking based on the scalar density Phi equivalent to (1/3!)epsilon(mu upsilon rho sigma) partial derivative(mu)A(upsilon rho sigma) with an independent third-rank tensor A(mu upsilon rho),which replaces the scalar density Phi equivalent to epsilon(mu upsilon rho sigma)epsilon(abcd)(partial derivative(mu)phi(a)) (partial derivative(upsilon)phi(b)) (partial derivative(rho)phi(c))(partial derivative(sigma)phi(d)) used in "two- measure theory." We apply this function both to globally and locally scale-invariant systems. For local scale invariance, we modify F-mu upsilon rho sigma((0)) by a certain Chern-Simons term, based on the recently developed tensor-hierarchy formulation. For a locally scale-invariant system with multiple scalars, the minimum value of the potential is realized at exactly zero value, while local scale invariance is broken by some nonzero vacuum expectation values: there exists <sigma(i)> not equal 0, there exists < F-mnrs > = f(0)epsilon(mnrs) not equal 0. For these values, the cosmological constant is maintained to be zero, despite the broken local scale invariance.
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页数:6
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