A small weak scale from a small cosmological constant

被引:43
作者
Arvanitaki, Asimina [1 ]
Dimopoulos, Savas [2 ]
Gorbenko, Victor [2 ]
Huang, Junwu [2 ]
Ken Van Tilburg [2 ,3 ,4 ]
机构
[1] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada
[2] Stanford Univ, Stanford Inst Theoret Phys, Stanford, CA 94305 USA
[3] NYU, Dept Phys, Ctr Cosmol & Particle Phys, 550 1St Ave, New York, NY 10003 USA
[4] Inst Adv Study, Sch Nat Sci, Princeton, NJ 08540 USA
基金
加拿大自然科学与工程研究理事会;
关键词
Phenomenology of Field Theories in Higher Dimensions; Phenomenology of Large extra dimensions; ATOMIC CLOCK; STABILIZATION;
D O I
10.1007/JHEP05(2017)071
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We propose a framework in which Weinberg's anthropic explanation of the cosmological constant problem also solves the hierarchy problem. The weak scale is selected by chiral dynamics that controls the stabilization of an extra dimension. When the Higgs vacuum expectation value is close to a fermion mass scale, the radius of an extra dimension becomes large, and develops an enhanced number of vacua available to scan the cosmological constant down to its observed value. At low energies, the radion necessarily appears as an unnaturally light scalar, in a range of masses and couplings accessible to fifth-force searches as well as scalar dark matter searches with atomic clocks and gravitational-wave detectors. The fermion sector that controls the size of the extra dimension consists of a pair of electroweak doublets and several singlets. These leptons satisfy approximate mass relations related to the weak scale and are accessible to the LHC and future colliders.
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页数:57
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