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We present a model-independent reconstruction of the early expansion and thermal histories of the universe, obtained from light element abundance measurements.
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2011
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2011
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2012
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2013
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K. M. Nollett and G. Steigman, “BBN and the CMB constrain light, electromagnetically coupled WIMPs,” PhRvD , vol. 89, no. 8, p. 083508, Apr. 2014
2014
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2017
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2018
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2018
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M. Escudero, “Neutrino decoupling beyond the Standard Model: CMB constraints on the Dark Matter mass with a fast and precise N eff
2019
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M. Valerdi, A. Peimbert, M. Peimbert, and A. Sixtos, “Determination of the Primordial Helium Abundance Based on NGC 346, an H II Region of the Small Magellanic Cloud,” ApJ , vol. 876, no. 2, p. 98, May 2019
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V. V. Klimenko, A. V. Ivanchik, P. Petitjean, P. Noterdaeme, and R. Srianand, “Estimation of the Cosmic Microwave Background Temperature from Atomic C I and Molecular CO Lines in the Interstellar Medium of Early Galaxies,” Astronomy Letters , vol. 46, no. 11, pp. 715–725, Nov. 2020
2020
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2021
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2022
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R. An, V. Gluscevic, E. Calabrese, and J. C. Hill, “What does cosmology tell us about the mass of thermal-relic dark matter?” JCAP , vol. 2022, no. 7, p. 002, Jul. 2022
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A. C. Sobotka, A. L. Erickcek, and T. L. Smith, “Was entropy conserved between BBN and recombination?” PhRvD , vol. 107, no. 2, p. 023525, Jan. 2023
2023
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