Massive free-field spectra in moving frames cannot be represented by a scalar temperature with dipole anisotropy, forcing the use of a four-vector temperature.
The Cosmic Neutrino Background
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The cosmic neutrino background is like the cosmic microwave background, but less photon-y and more neutrino-ey. The CNB is also less talked about than the CMB, mostly because it's nearly impossible to detect directly. But if it could be detected, it would be interesting in several ways that are discussed.
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Lorentz Transformation of the Energy Spectrum of the Equilibrium State of Massive Free Fields
Massive free-field spectra in moving frames cannot be represented by a scalar temperature with dipole anisotropy, forcing the use of a four-vector temperature.