IKKT thermodynamics and early universe cosmology

被引:2
|
作者
Laliberte, Samuel [1 ]
Brahma, Suddhasattwa [2 ]
机构
[1] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
[2] Univ Edinburgh, Higgs Ctr Theoret Phys, Sch Phys & Astron, Edinburgh EH9 3FD, Scotland
基金
加拿大自然科学与工程研究理事会;
关键词
Cosmological models; M(atrix) Theories; Models of Quantum Gravity; SUPERSTRINGS; MODEL; BREAKING;
D O I
10.1007/JHEP11(2023)161
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
Matrix theory is a proposed non-perturbative definition of superstring theory in which space is emergent. Recently, it was shown that space-time can emerge with a scale-invariant spectrum of cosmological perturbations which is sourced by thermal fluctuations of the BFSS model at finite temperature. Inspired by these results, we begin a study of the IKKT model at finite temperature. We find that in this model, which is closely related to the BFSS model at finite temperature, thermal fluctuations can also source a scale-invariant spectrum of scalar and tensor fluctuations.
引用
收藏
页数:24
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