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For a class of macroscopic dark matter models, inelastic scattering of dark matter off a nucleus can generate electromagnetic signatures with GeV-scale energy.
1905
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1906
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Y. Bai and J. Berger, Nucleus Capture by Macroscopic Dark Matter
1912
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G. Rosen, Particlelike Solutions to Nonlinear Complex Scalar Field Theories with Positive-Definite Energy Densities
1968
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R. Friedberg, T. D. Lee, and A. Sirlin, A Class of Scalar-Field Soliton Solutions in Three Space Dimensions
1976
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1982
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1992
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1998
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G. J. Feldman and R. D. Cousins, A Unified approach to the classical statistical analysis of small signals
1998
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R. Mahbubani, M. Redi, and A. Tesi, Dark Nucleosynthesis: Cross-sections and Astrophysical Signals
2007
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J.-P. Hong, S. Jung, and K.-P. Xie, Fermi-ball dark matter from a first-order phase transition
2008
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M. B. Wise and Y. Zhang, Stable Bound States of Asymmetric Dark Matter
2017
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2018
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D. M. Grabowska, T. Melia, and S. Rajendran, Detecting Dark Blobs
2018
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2018
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2015
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G. Krnjaic and K. Sigurdson, Big Bang Darkleosynthesis
2015
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E. Hardy, R. Lasenby, J. March-Russell, and S. M. West, Big Bang Synthesis of Nuclear Dark Matter
2015
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D. M. Jacobs, G. D. Starkman, and B. W. Lynn, Macro Dark Matter
2015
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2015
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X. Liang and A. Zhitnitsky, Axion field and the quark nugget’s formation at the QCD phase transition
2016
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Cited in the paper.
2019
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2019
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M. Redi and A. Tesi, Cosmological Production of Dark Nuclei
2019
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2019
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2021
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2022
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