Taking the temperature of the Universe
How hot is the Universe today? How hot was it before? A new study, which has been published in the Astrophysical Journal, suggests that the mean temperature of gas in large structures of the Universe has increased ten times over the last 10 billion years, to reach about 2 million Kelvin today.
The large-scale structure of the Universe refers to the global pattern of how galaxies and galaxy clusters are distributed in space. This cosmic net formed from tiny irregularities in the matter distribution in the early Universe, which were amplified through gravitational attraction. “As the Universe evolves, gravity pulls dark matter and gas in space together into galaxies and clusters of galaxies,” said Yi-Kuan Chiang, the lead author of the study and a research fellow at the Ohio State University Center for Cosmology and AstroParticle Physics. “The drag is violent - so violent that more and more gas is shocked and heated up.”
This heated gas can then be used to measure the mean temperature of the Universe over cosmic time. In particular, the researchers used the so-called “Sunyaev-Zeldovich” effect, named after Rashid Sunyaev, director emeritus at the Max Planck Institute for Astrophysics, who first predicted this phenomenon theoretically. This effect arises when low-energy photons of the cosmic microwave background radiation are scattered by hot electrons in the large-scale structure of the Universe. The scattering transfers energy from electrons to photons, making the hot electron gas visible. The intensity of the Sunyaev-Zeldovich effect is proportional to the thermal pressure of the gas, which, in turn, is proportional to the temperature of electrons.
While this measurement is straightforward in principle, collecting the necessary data was a major undertaking. The study was done in a collaboration of researchers at the Ohio State University, the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU) at the University of Tokyo, the John Hopkins University, and the Max Planck Institute for Astrophysics. The researchers used data collected by two observatories, the Planck satellite and the Sloan Digital Sky Survey (SDSS). Planck is the European Space Agency mission, which measured the cosmic microwave background radiation. SDSS collected detailed images and light spectra of galaxies. Combining the two data sets, the scientists were able to measure the amount of thermal pressure around the locations of galaxies and clusters of galaxies.
The study determined that about 8 billion years ago (at a redshift z=1), the mean electron temperature was some 700 000 Kelvin, raising to about 2 million Kelvin today. Furthermore, the scientists determined that its evolution is almost entirely driven by the growth of structures, as gas is shock heated in collapsing large-scale structures.
Back in 2000, Eiichiro Komatsu, director at the Max Planck Institute for Astrophysics and Principal Investigator of the Cluster of Excellence ORIGINS, was also involved in a previous effort to calculate how the temperature of the Universe evolved. “For 20 years, we have been studying how to measure this using the Sunyaev-Zeldovich effect,” he remembers. “We now have finally measured the temperature of the Universe, not only thanks to the remarkable progress in observational data, but also due to the dedicated efforts of brilliant young scientists such as Yi-Kuan Chiang and Ryu Makiya. This is very satisfying,” Komatsu adds.