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Title: Constraining D-foam via the 21-cm line

Abstract

We have suggested earlier that D-particles, which are stringy space-time defects predicted in brane-inspired models of the Universe, might constitute a component of dark matter, and that they might contribute to the masses of singlet fermions that could provide another component. Interactions of the quantum-fluctuating D-particles with matter induce vector forces that are mediated by a massless effective U(1) gauge field, the “D-photon,” which is distinct from the ordinary photon and has different properties from dark photons. We discuss the form of interactions of D-matter with conventional matter induced by D-photon exchange and calculate their strength, which depends on the density of D-particles. Observations of the hydrogen 21 cm line at redshifts ≳15 can constrain these interactions and the density of D-matter in the early Universe.

Authors:
; ;
Publication Date:
Research Org.:
Texas A & M Univ., College Station, TX (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1491769
Alternate Identifier(s):
OSTI ID: 1611532
Grant/Contract Number:  
FG02-13ER42020; SC0010813
Resource Type:
Published Article
Journal Name:
Physical Review D
Additional Journal Information:
Journal Name: Physical Review D Journal Volume: 99 Journal Issue: 1; Journal ID: ISSN 2470-0010
Publisher:
American Physical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics; Physics; Dynamical symmetry breaking models; Extensions of fermion sector; Particle dark matter

Citation Formats

Ellis, John, Mavromatos, Nick E., and Nanopoulos, Dimitri V. Constraining D-foam via the 21-cm line. United States: N. p., 2019. Web. doi:10.1103/PhysRevD.99.015031.
Ellis, John, Mavromatos, Nick E., & Nanopoulos, Dimitri V. Constraining D-foam via the 21-cm line. United States. https://doi.org/10.1103/PhysRevD.99.015031
Ellis, John, Mavromatos, Nick E., and Nanopoulos, Dimitri V. Tue . "Constraining D-foam via the 21-cm line". United States. https://doi.org/10.1103/PhysRevD.99.015031.
@article{osti_1491769,
title = {Constraining D-foam via the 21-cm line},
author = {Ellis, John and Mavromatos, Nick E. and Nanopoulos, Dimitri V.},
abstractNote = {We have suggested earlier that D-particles, which are stringy space-time defects predicted in brane-inspired models of the Universe, might constitute a component of dark matter, and that they might contribute to the masses of singlet fermions that could provide another component. Interactions of the quantum-fluctuating D-particles with matter induce vector forces that are mediated by a massless effective U(1) gauge field, the “D-photon,” which is distinct from the ordinary photon and has different properties from dark photons. We discuss the form of interactions of D-matter with conventional matter induced by D-photon exchange and calculate their strength, which depends on the density of D-particles. Observations of the hydrogen 21 cm line at redshifts ≳15 can constrain these interactions and the density of D-matter in the early Universe.},
doi = {10.1103/PhysRevD.99.015031},
journal = {Physical Review D},
number = 1,
volume = 99,
place = {United States},
year = {2019},
month = {1}
}

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