Energy distribution and radiation of Q-bubble dark matter on the quantum space-time background

Yi YU; Jun YAN

doi:10.1360/SSPMA2017-00364

SCIENTIA SINICA Physica, Mechanica & Astronomica

SCIENTIA SINICA Physica, Mechanica & Astronomica, Volume 48, Issue 4: 049801(2018) https://doi.org/10.1360/SSPMA2017-00364

Energy distribution and radiation of Q-bubble dark matter on the quantum space-time background

Yi YU, Jun YAN^*

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ReceivedDec 22, 2017
AcceptedJan 23, 2018
PublishedFeb 11, 2018

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Abstract

Energy distribution and radiation phenomena of Q-bubble dark matter on the quantum space-time background are studied in this paper. Under the quantum gravitational energy scale, the energy and energy level difference of Q-bubble are calculated respectively for energy and momentum correction dispersion relations. Moreover, the energy and energy level difference in the pertubation case are also calculated. We analysed radiation particles’ law of dark matter bubbles under the Lorentz symmetry breaking and the pertubation situation, and found that the radiated energy increases with quantum space-time effect increases, and it also increases with the bubble potential energy increases. These physical effects may be confirmed in the further dark matter observations and experiments.

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四川省教育厅自然科学基金(编号:)

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03.65.Ge	Solutions of wave equations: bound states
03.65.Pm	Relativistic wave equations
04.60.Bc	Phenomenology of quantum gravity
95.35.+d	Dark matter (stellar, interstellar, galactic, and cosmological) (see also 95.30.Cq Elementary particle processes; for brown dwarfs, see 97.20.Vs; for galactic halos, see 98.35.Gi or 98.62.Gq; for models of the early Universe, see 98.80.Cq

Energy distribution and radiation of Q-bubble dark matter on the quantum space-time background

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