Regge trajectories and Hagedorn behavior: Hadronic realizations of dynamical dark matter
Publisher
AMER INST PHYSICSCitation
AIP Conference Proceedings 1900, 040003 (2017); https://doi.org/10.1063/1.5010121Journal
WORKSHOP ON NEUTRINO PHYSICS AND UNIFICATION, NEAR DETECTOR PHYSICS AND DARK MATTER (CETUP* 2016)Rights
Copyright © 2017, AIP Publishing LLC.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Dynamical Dark Matter (DDM) is an alternative framework for dark-matter physics in which the dark sector comprises a vast ensemble of particle species whose Standard-Model decay widths are balanced against their cosmological abundances. In this talk, we study the properties of a hitherto-unexplored class of DDM ensembles in which the ensemble constituents are the "hadronic" resonances associated with the confining phase of a strongly-coupled dark sector. Such ensembles exhibit masses lying along Regge trajectories and Hagedorn-like densities of states that grow exponentially with mass. We investigate the applicable constraints on such dark-"hadronic" DDM ensembles and find that these constraints permit a broad range of mass and confinement scales for these ensembles. We also find that the distribution of the total present-day abundance across the ensemble is highly correlated with the values of these scales. This talk reports on research originally presented in Ref. [1].Note
12 month embargo; Published Online: November 2017.ISSN
0094-243XVersion
Final published versionSponsors
CETUP* (Center for Theoretical Underground Physics and Related Areas); Department of Energy [DE-FG02-13ER41976 / DE-SC0009913]; National Science FoundationAdditional Links
http://aip.scitation.org/doi/abs/10.1063/1.5010121ae974a485f413a2113503eed53cd6c53
10.1063/1.5010121