de Sitter swampland conjecture and the Higgs potential

被引:110
|
作者
Denef, Frederik [1 ]
Hebecker, Arthur [2 ]
Wrase, Timm [3 ]
机构
[1] Columbia Univ, Dept Phys, 538 West 120th St, New York, NY 10027 USA
[2] Heidelberg Univ, Inst Theoret Phys, Philosophenweg 19, D-69120 Heidelberg, Germany
[3] TU Vienna, Inst Theoret Phys, Wiedner Hauptstr 8-10-136, A-1040 Vienna, Austria
关键词
STRING THEORY; COMPACTIFICATIONS; VACUA; NO;
D O I
10.1103/PhysRevD.98.086004
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
According to a conjecture recently put forward in [1], the scalar potential V of any consistent theory of quantum gravity satisfies a bound vertical bar del vertical bar/V >= O(1). This forbids de Sitter solutions and supports quintessence models of cosmic acceleration. Here, we point out that in the simplest models incorporating the standard model in addition to quintessence, with the two sectors decoupled as suggested by observations, the proposed bound is violated by 50 orders of magnitude. However, a very specific coupling between quintessence and just the Higgs sector may still be allowed and consistent with the conjecture.
引用
收藏
页数:6
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