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Superheavy Thermal Dark Matter

Hyungjin Kim and Eric Kuflik
Phys. Rev. Lett. 123, 191801 – Published 8 November 2019
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Abstract

We propose a mechanism of elementary thermal dark matter with a mass up to 1014GeV, within a standard cosmological history, whose relic abundance is determined solely by its interactions with the standard model, without violating the perturbative unitarity bound. The dark matter consists of many nearly degenerate particles which scatter with the standard model bath in a nearest-neighbor chain, and maintain chemical equilibrium with the standard model bath by in-equilibrium decays and inverse decays. The phenomenology includes super heavy elementary dark matter and heavy relics that decay at various epochs in the cosmological history, with implications for the cosmic microwave background, structure formation, and cosmic ray experiments.

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  • Received 19 June 2019

DOI:https://doi.org/10.1103/PhysRevLett.123.191801

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Hyungjin Kim

  • Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 7610001, Israel

Eric Kuflik

  • Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel

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Issue

Vol. 123, Iss. 19 — 8 November 2019

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