High-scale axions without isocurvature from inflationary dynamics

Kearney, John; Orlofsky, Nicholas; Pierce, Aaron

doi:10.1103/PhysRevD.93.095026

Title: High-scale axions without isocurvature from inflationary dynamics

Journal Article · 31 May 2016 · Physical Review D

DOI: https://doi.org/10.1103/PhysRevD.93.095026 · OSTI ID:1256325

Kearney, John ^[1]; Orlofsky, Nicholas ^[2]; Pierce, Aaron ^[2]

Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Univ. of Michigan, Ann Arbor, MI (United States)

Observable primordial tensor modes in the cosmic microwave background (CMB) would point to a high scale of inflation H_I. If the scale of Peccei-Quinn (PQ) breaking f_a is greater than H_I/2π, CMB constraints on isocurvature naively rule out QCD axion dark matter. This assumes the potential of the axion is unmodified during inflation. We revisit models where inflationary dynamics modify the axion potential and discuss how isocurvature bounds can be relaxed. We find that models that rely solely on a larger PQ-breaking scale during inflation f_I require either late-time dilution of the axion abundance or highly super-Planckian f_I that somehow does not dominate the inflationary energy density. Models that have enhanced explicit breaking of the PQ symmetry during inflation may allow f_a close to the Planck scale. Lastly, avoiding disruption of inflationary dynamics provides important limits on the parameter space.

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Research Organization:: Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: AC02-07CH11359; SC0007859

OSTI ID:: 1256325

Alternate ID(s):: OSTI ID: 1254888

Report Number(s):: FERMILAB-PUB-16-005-T; MCTP-16-02; arXiv:1601.03049; PRVDAQ; 1415092; TRN: US1601745

Journal Information:: Physical Review D, Vol. 93, Issue 9; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 14 works

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Natural Chaotic Inflation in Supergravity Kawasaki, M.; Yamaguchi, Masahide; Yanagida, T. arXiv https://doi.org/10.48550/arxiv.hep-ph/0004243	text	January 2000
Curvaton and QCD Axion in Supersymmetric Theories Chun, Eung Jin; Dimopoulos, Konstantinos; Lyth, David arXiv https://doi.org/10.48550/arxiv.hep-ph/0402059	text	January 2004
Supersymmetry Breaking in the Early Universe Dine, Michael; Randall, Lisa; Thomas, Scott arXiv https://doi.org/10.48550/arxiv.hep-ph/9503303	text	January 1995
Baryogenesis from Flat Directions of the Supersymmetric Standard Model Dine, Michael; Randall, Lisa; Thomas, Scott arXiv https://doi.org/10.48550/arxiv.hep-ph/9507453	text	January 1995
Can Decaying Particles Raise the Upperbound on the Peccei-Quinn Scale? Kawasaki, M.; Moroi, T.; Yanagida, T. arXiv https://doi.org/10.48550/arxiv.hep-ph/9510461	text	January 1995
What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy? Lyth, David H. arXiv https://doi.org/10.48550/arxiv.hep-ph/9606387	text	January 1996
Lattice study of classical inflaton decay Prokopec, Tomislav; Roos, Thomas G. arXiv https://doi.org/10.48550/arxiv.hep-ph/9610400	text	January 1996
Cosmic strings from preheating Tkachev, I.; Khlebnikov, S.; Kofman, L. arXiv https://doi.org/10.48550/arxiv.hep-ph/9805209	text	January 1998
Axions from wall decay Chang, S.; Hagmann, C.; Sikivie, P. arXiv https://doi.org/10.48550/arxiv.hep-ph/9808302	text	January 1998
Remarks on Cosmic String Formation during Preheating on Lattice Simulations Kasuya, S.; Kawasaki, M. arXiv https://doi.org/10.48550/arxiv.hep-ph/9903324	text	January 1999
On the Possibility of Large Axion Decay Constants Banks, Tom; Dine, Michael; Fox, Patrick J. arXiv https://doi.org/10.48550/arxiv.hep-th/0303252	text	January 2003
Planck-Scale Physics and the Peccei-Quinn Mechanism Kamionkowski, Marc; March-Russell, John arXiv https://doi.org/10.48550/arxiv.hep-th/9202003	text	January 1992
Reheating after Inflation Kofman, Lev; Linde, Andrei; Starobinsky, Alexei arXiv https://doi.org/10.48550/arxiv.hep-th/9405187	text	January 1994
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