Time non-locality in dark matter and LSS

Abstract We explore the intriguing phenomenon of time non-locality in the evolution of dark matter and Large Scale Structure (LSS). Recently in [1], it was shown that time non-locality emerges in bias tracer fluctuations, which are SO(3) scalars in real space, at fifth order in the perturbation expansion in dark matter overdensity. We demonstrate that by breaking the symmetry down to SO(2), which is the case whenever line-of-sight effects become important, such as for flux fluctuations in the Lyman α forest, the temporal non-locality appears at the third order in expansion. Additionally, within the framework of EFTofLSS, we demonstrate that time non-locality manifests in the effective stress tensor of dark matter, which is a second rank tensor under SO(3) transformations, again at the third order in dark matter overdensity. Furthermore, we highlight the effectiveness of the standard Π basis [2] in handling time non-local operators.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2025-10-01
DOI
https://doi.org/10.1088/1475-7516/2025/10/018
Citations
1
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
1.15
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article

Time non-locality in dark matter and LSS

Arhum Ansari, Sachin Jain, Arka Banerjee, Shaunak Padhyegurjar
1 citations
Journal of Cosmology and Astroparticle Physics
Cosmology and Gravitation Theories
1.15
article

Time non-locality in dark matter and LSS

Arhum Ansari, Sachin Jain, Arka Banerjee, Shaunak Padhyegurjar
article en
1 citations

Abstract

Abstract We explore the intriguing phenomenon of time non-locality in the evolution of dark matter and Large Scale Structure (LSS). Recently in [1], it was shown that time non-locality emerges in bias tracer fluctuations, which are SO(3) scalars in real space, at fifth order in the perturbation expansion in dark matter overdensity. We demonstrate that by breaking the symmetry down to SO(2), which is the case whenever line-of-sight effects become important, such as for flux fluctuations in the Lyman α forest, the temporal non-locality appears at the third order in expansion. Additionally, within the framework of EFTofLSS, we demonstrate that time non-locality manifests in the effective stress tensor of dark matter, which is a second rank tensor under SO(3) transformations, again at the third order in dark matter overdensity. Furthermore, we highlight the effectiveness of the standard Π basis [2] in handling time non-local operators.

Journal of Cosmology and Astroparticle PhysicsVol. 2025(10)
Indian Institute of Science Education and Research Pune (IN), Indian Institute of Science Education and Research, Bhopal (IN)
Openalex Percentile: Top 16%
Cosmology and Gravitation Theories
1.15
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