The DOI matches its Crossref record; 36 of the 36 references it cites were found in a registry or an index.
What is the lowest possible reheating temperature?
Open accessAbstract
We study models in which the universe exits reheating at temperatures in the MeV regime. By combining light element abundance measurements with cosmic microwave background and large scale structure data we find a fairly robust lower limit on the reheating temperature of ${T}_{\mathrm{RH}}\ensuremath{\gtrsim}4\mathrm{MeV}$ at 95% C.L. However, if the heavy particle whose decay reheats the universe has a direct decay mode to neutrinos, there are some small islands left in parameter space where a reheating temperature as low as 1 MeV is allowed. The derived lower bound on the reheating temperature also leads to very stringent bounds on models with n large extra dimensions. For $n=2$ the bound on the compactification scale is $M\ensuremath{\gtrsim}2000\mathrm{TeV},$ and for $n=3$ it is 100 TeV. These are currently the strongest available bounds on such models.
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Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
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Cosmological parameters from SDSS and WMAP
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Hagiwara, K., Hikasa, K., Nakamura, K., Tanabashi, M., Aguilar-Benitez, M., Amsler, C., Barnett, R. M., Burchat, P. R., Carone, C. D., Caso, C., et al. (2002) · Physical Review D · doi:10.1103/physrevd.66.010001 · Cited by 3,099
The 2dF Galaxy Redshift Survey: spectra and redshifts
Colless, M., Dalton, G., Maddox, S., Sutherland, W., Norberg, P., Cole, S., Bland-Hawthorn, J., Bridges, T., Cannon, R., Collins, C., et al. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04902.x · Cited by 2,367
A Line-of-Sight Integration Approach to Cosmic Microwave Background Anisotropies
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The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
Tegmark, M., Blanton, M. R., Strauss, M. A., Hoyle, F., Schlegel, D., Scoccimarro, R., Vogeley, M. S., Weinberg, D. H., Zehavi, I., Berlind, A., et al. (2004) · The Astrophysical Journal · doi:10.1086/382125 · Cited by 1,787
The 2dF Galaxy Redshift Survey: the power spectrum and the matter content of the Universe
Percival, W. J., Baugh, C. M., Bland-Hawthorn, J., Bridges, T., Cannon, R., Cole, S., Colless, M., Collins, C., Couch, W., Dalton, G., et al. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04827.x · Cited by 835
Largest temperature of the radiation era and its cosmological implications
Giudice, G. F., Kolb, E. W., & Riotto, A. (2001) · Physical Review D · doi:10.1103/physrevd.64.023508 · Cited by 682
The 2dF Galaxy Redshift Survey: the bias of galaxies and the density of the Universe
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Cited by
New experimental approaches in the search for axion-like particles
Irastorza, I. G., & Redondo, J. (2018) · Progress in Particle and Nuclear Physics · doi:10.1016/j.ppnp.2018.05.003 · Cited by 745
Bounds on very low reheating scenarios after Planck
de Salas, P. F., Lattanzi, M., Mangano, G., Miele, G., Pastor, S., & Pisanti, O. (2015) · Physical Review D · doi:10.1103/physrevd.92.123534 · Cited by 321
Neutralino with the right cold dark matter abundance in (almost) any supersymmetric model
Gelmini, G., & Gondolo, P. (2006) · Physical Review D · doi:10.1103/physrevd.74.023510 · Cited by 305
What does inflation really predict?
Tegmark, M. (2005) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2005/04/001 · Cited by 216
Visinelli, L., & Gondolo, P. (2009) · Physical Review D · doi:10.1103/physrevd.80.035024 · Cited by 209
Metadata
- Authors
- Hannestad, S.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2004-08-09
- Volume
- 70
- Issue
- 4
- ISSN
- 0556-2821 (ISSN-L)
- 1550-7998
- 1550-2368
- OpenAlex
- W2006830043
- Cited by
- 531
- References
- 36
- FWCI
- 8.47
- Type
- journal article
- Language
- en
- Open access
- green
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