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Standard cosmology predicts that prior to matter-radiation equality about 41% of the energy density was in free-streaming neutrinos.
1902
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2004
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J. F. Beacom, N. F. Bell and S. Dodelson, Neutrinoless universe , Phys. Rev. Lett. 93
2004
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G. Mangano, G. Miele, S. Pastor, T. Pinto, O. Pisanti and P. D. Serpico, Relic neutrino decoupling including flavor oscillations , Nucl. Phys. B729
2005
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Z. Chacko, L. J. Hall, S. J. Oliver and M. Perelstein, Late time neutrino masses, the LSND experiment and the cosmic microwave background , Phys. Rev. Lett. 94
2005
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S. Hannestad and G. Raffelt, Constraining invisible neutrino decays with the cosmic microwave background , Phys. Rev. D72
2005
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2016
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2017
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A. Berlin and N. Blinov, Thermal Dark Matter Below an MeV , Phys. Rev. Lett. 120
2018
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J. Halverson and P. Langacker, TASI Lectures on Remnants from the String Landscape , PoS TASI2017
2018
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2019
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A. Berlin and N. Blinov, Thermal neutrino portal to sub-MeV dark matter , Phys. Rev. D99
2019
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2020
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P. Virtanen, R. Gommers, T. E. Oliphant, M. Haberland, T. Reddy, D. Cournapeau et al., SciPy 1.0: Fundamental Algorithms for Scientific Computing in Python , Nature Methods 17
2020
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