Relativistic Maxwell-Bloch equations are derived showing that radiating system response and coherence between emitters are preserved across reference frames, with timescales and intensity transforming as expected relativistically.
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming Regions - IX
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Milky Way radial and vertical dynamics are inconsistent with MOND and STVG but consistent with dark matter halos, disfavoring the former at high significance.
The frequency of global core g-modes in warm neutron stars can be higher or lower than in cold stars depending on the nuclear symmetry energy slope L.
High-resolution dust polarization and C18O observations in Cepheus A show gravity driving gas accretion while magnetic tension regulates turbulence, producing ordered flows at 2.1e-4 solar masses per year with coherent B-field alignment across scales.
citing papers explorer
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Relativistic Maxwell-Bloch Equations with Applications to Astrophysics
Relativistic Maxwell-Bloch equations are derived showing that radiating system response and coherence between emitters are preserved across reference frames, with timescales and intensity transforming as expected relativistically.
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Milky Way Dynamics Favor Dark Matter over Modified Gravity Models
Milky Way radial and vertical dynamics are inconsistent with MOND and STVG but consistent with dark matter halos, disfavoring the former at high significance.
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Finite temperature effects on g-modes of inviscid neutron stars
The frequency of global core g-modes in warm neutron stars can be higher or lower than in cold stars depending on the nuclear symmetry energy slope L.
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Evidence for the gravity-driven and magnetically-regularized gas flows feeding the massive protostellar cluster in Cepheus A
High-resolution dust polarization and C18O observations in Cepheus A show gravity driving gas accretion while magnetic tension regulates turbulence, producing ordered flows at 2.1e-4 solar masses per year with coherent B-field alignment across scales.