Opening up the QCD axion window
Abstract
We present a new mechanism to deplete the energy density of the QCD axion, making decay constants as high as fa ≃ 1017 GeV viable for generic initial conditions. In our setup, the axion couples to a massless dark photon with a coupling that is moderately stronger than the axion coupling to gluons. Dark photons are produced copiously through a tachyonic instability when the axion field starts oscillating, and an exponential suppression of the axion density can be achieved. For a large part of the parameter space this dark radiation component of the universe can be observable in upcoming CMB experiments. Such dynamical depletion of the axion density ameliorates the isocurvature bound on the scale of inflation. The depletion also amplifies the power spectrum at scales that enter the horizon before particle production begins, potentially leading to axion miniclusters.
- Authors:
-
- Harvard Univ., Cambridge, MA (United States). Dept. of Physics
- Stanford Univ., CA (United States). Stanford Institute for Theoretical Physics
- Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States). Center for Theoretical Physics
- Publication Date:
- Research Org.:
- Stanford Univ., CA (United States); Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1499139
- Grant/Contract Number:
- SC0012012; SC0012567; SC0015476
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of High Energy Physics (Online)
- Additional Journal Information:
- Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2018; Journal Issue: 3; Journal ID: ISSN 1029-8479
- Publisher:
- Springer Berlin
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
Citation Formats
Agrawal, Prateek, Marques-Tavares, Gustavo, and Xue, Wei. Opening up the QCD axion window. United States: N. p., 2018.
Web. doi:10.1007/jhep03(2018)049.
Agrawal, Prateek, Marques-Tavares, Gustavo, & Xue, Wei. Opening up the QCD axion window. United States. doi:10.1007/jhep03(2018)049.
Agrawal, Prateek, Marques-Tavares, Gustavo, and Xue, Wei. Thu .
"Opening up the QCD axion window". United States. doi:10.1007/jhep03(2018)049. https://www.osti.gov/servlets/purl/1499139.
@article{osti_1499139,
title = {Opening up the QCD axion window},
author = {Agrawal, Prateek and Marques-Tavares, Gustavo and Xue, Wei},
abstractNote = {We present a new mechanism to deplete the energy density of the QCD axion, making decay constants as high as fa ≃ 1017 GeV viable for generic initial conditions. In our setup, the axion couples to a massless dark photon with a coupling that is moderately stronger than the axion coupling to gluons. Dark photons are produced copiously through a tachyonic instability when the axion field starts oscillating, and an exponential suppression of the axion density can be achieved. For a large part of the parameter space this dark radiation component of the universe can be observable in upcoming CMB experiments. Such dynamical depletion of the axion density ameliorates the isocurvature bound on the scale of inflation. The depletion also amplifies the power spectrum at scales that enter the horizon before particle production begins, potentially leading to axion miniclusters.},
doi = {10.1007/jhep03(2018)049},
journal = {Journal of High Energy Physics (Online)},
number = 3,
volume = 2018,
place = {United States},
year = {2018},
month = {3}
}
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Figures / Tables:
Figure 1: Current bounds and future experimental reach for axion couplings to photons de ned in eq. (2.1). Blue shaded regions show the current constraints which are independent of a dark matter interpretation, while the red shaded region are constraints from axion haloscopes. Sensitivity of future experiments is shown bymore »
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