Impact of Dynamical Collapse Models on Inflationary Cosmology

被引:8
|
作者
Gundhi, A. [1 ,2 ]
Gaona-Reyes, J. L. [1 ,2 ]
Carlesso, M. [3 ]
Bassi, A. [1 ,2 ]
机构
[1] Univ Trieste, Dept Phys, Str Costiera 11, I-34151 Trieste, Italy
[2] Ist Nazl Fis Nucl, Trieste Sect, Via Valerio 2, I-34127 Trieste, Italy
[3] Queens Univ, Sch Math & Phys, Ctr Theoret Atom Mol & Opt Phys, Belfast BT7 1NN, Antrim, North Ireland
基金
英国工程与自然科学研究理事会; 欧盟地平线“2020”;
关键词
CONTINUOUS SPONTANEOUS LOCALIZATION; WAVE-FUNCTION; GRAVITATIONAL-WAVES; QUANTUM; REDUCTION; PERTURBATIONS; GRAVITY; BOUNDS; DECOHERENCE;
D O I
10.1103/PhysRevLett.127.091302
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Inflation solves several cosmological problems at the classical and quantum level, with a strong agreement between the theoretical predictions of well-motivated inflationary models and observations. In this Letter, we study the corrections induced by dynamical collapse models, which phenomenologically solve the quantum measurement problem, to the power spectrum of the comoving curvature perturbation during inflation and the radiation-dominated era. We find that the corrections are strongly negligible for the reference values of the collapse parameters.
引用
收藏
页数:7
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