Hahn, S., & Hofmann, R. (2017). Cosmic microwave background as a thermal gas of SU(2) photons: Implications for the high-z cosmological model and the value of H0. Advances in high energy physics.
Chicago Style (17th ed.) CitationHahn, Steffen, and Ralf Hofmann. "Cosmic Microwave Background as a Thermal Gas of SU(2) Photons: Implications for the High-z Cosmological Model and the Value of H0." Advances in High Energy Physics 2017.
MLA (9th ed.) CitationHahn, Steffen, and Ralf Hofmann. "Cosmic Microwave Background as a Thermal Gas of SU(2) Photons: Implications for the High-z Cosmological Model and the Value of H0." Advances in High Energy Physics, 2017.
Warning: These citations may not always be 100% accurate.