Particle physics from stars

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A White Paper on keV sterile neutrino Dark Matter (2016, background): “The result of [878] is that such exotic energy loss should obey ε < 10(19) erg g−1 s−1 , (7.”
Search for New Physics with Atoms and Molecules (2017, methodology): “01 for the neutron, and Ce 1⁄4 0 for the electron (Raffelt, 1999).”
Spin-dependent macroscopic forces from new particle exchange (2006, background): “33) The limits from star cooling [36] are stronger by several orders of magnitude, but as discussed at the end of section 5.”
Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report Volume 2: The Physics Program for DUNE at LBNF (2015, unknown): “, [132, 133]).”
Supernova and neutron star limits on large extra dimensions reexamined (2003, background): “The result can be summarized by the simple criterion that the exotic energy-loss rate of a nuclear medium at a density of 3× 10(14) g cm and a temperature of 30 MeV should not exceed 10(19) erg g s [16, 17].”