Cosmological decoherence from thermal gravitons

被引:6
作者
Bao, Ning [1 ,2 ,3 ]
Chatwin-Davies, Aidan [4 ]
Pollack, Jason [5 ]
Remmen, Grant N. [1 ,2 ]
机构
[1] Univ Calif Berkeley, Ctr Theoret Phys, 366 Le Conte Hall 7300, Berkeley, CA 94720 USA
[2] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
[3] Brookhaven Natl Lab, Computat Sci Initiat, 98 Rochester St, Upton, NY 11973 USA
[4] Katholieke Univ Leuven, Inst Theoret Phys, Celestijnenlaan 200D, B-3001 Leuven, Belgium
[5] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V6T 1Z1, Canada
基金
欧洲研究理事会; 加拿大自然科学与工程研究理事会; 美国国家科学基金会;
关键词
Classical Theories of Gravity; Models of Quantum Gravity; Quantum Dissipative Systems; COUPLED ANHARMONIC-OSCILLATORS; FALSE VACUUM; QUANTUM; HISTORIES; FATE;
D O I
10.1007/JHEP08(2020)065
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 study the effects of gravitationally-driven decoherence on tunneling processes associated with false vacuum decays, such as the Coleman-De Luccia instanton. We compute the thermal graviton-induced decoherence rate for a wave function describing a perfect fluid of nonzero energy density in a finite region. When the effective cosmological constant is positive, the thermal graviton background sourced by a de Sitter horizon provides an unavoidable decoherence effect, which may have important consequences for tunneling processes in cosmological history. We discuss generalizations and consequences of this effect and comment on its observability and applications to black hole physics.
引用
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页数:28
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