Research supports role of supernovas in measuring pace at which the universe expands

DETROIT - A team of research scientists led by David Cinabro, professor of physics and astronomy in the College of Liberal Arts and Sciences at Wayne State University, recently published a paper marking the importance of type 1a supernovas in measuring the pace at which the universe expands. Type 1a supernovas are among the very brightest cosmic explosions visible, signaling the death of stars, and their importance to cosmology cannot be understated.

The findings of the study - published in the Monthly Notices of the Royal Astronomical Society by Cinabro's team at Wayne State University, Daniel Scolnic, a postdoctoral scholar at the University of Chicago's Kavli Institute for Cosmological Physics, Rick Kessler, a senior researcher at the Kavli Institute, and undergraduate students Ashley Li and Jake Miller - support a theory that the expansion of the universe is accelerating and is attributable to a mysterious force known as dark energy - an unknown form of energy hypothesized to permeate all of space. The findings counter recent headlines that Type 1a supernovae cannot be used as an accurate measure for the expansion of the universe.

"Observations just before the turn of the century provided the first clear evidence of an accelerated expansion of the universe," said Cinabro. "Subsequent observations combined with the clustering of galaxies and the cosmic microwave background further point towards this acceleration being caused by a mysterious anti-gravity-like force called Dark Energy."

According to Cinabro, these observations depend on the assumption that the light output of type 1a supernovas relatively near to the earth can be described in the same way as those that are much further away. The observations of two distinct types of type 1a supernovas with different amounts of light output by Peter Milne of the University of Arizona and his collaborators in 2015 called this underpinning assumption into question.

Checking this observation with publicly available observations of type 1a supernova is not so easy, commented Cinabro.

"Milne and his collaborators observed two peaks in the brightness of type 1a supernova in the ultraviolet part of the light spectrum using instruments on the Swift satellite," said Cinabro. "Most of the existing type 1a supernova data have been observed with ground-based telescopes which have difficulty viewing in ultraviolet light due to the earth's atmosphere, which would fuzzily smear together two ultraviolet peaks in the light from nearby type 1a supernova as claimed by Milne and collaborators."

Based on the researcher's observations, more distant supernova have their ultraviolet light red-shifted - or stretched into lower frequencies or longer wavelengths - into the visible. The high-quality visible-light observations of type 1a supernovas from the SuperNova Legacy Survey (SNLS) and the Sloan Digital Sky Survey (SDSS) for more distant explosions do not exhibit the two peak structure expected if the earlier results were correct.

"Rather we observe a single, broad distribution of type 1a supernova brightness in the ultraviolet agreeing with earlier assumptions and existing models of type 1a supernova explosions," concluded Cinabro.

About Wayne State University

Wayne State University is one of the nation's pre-eminent public research universities in an urban setting. Through its multidisciplinary approach to research and education, and its ongoing collaboration with government, industry and other institutions, the university seeks to enhance economic growth and improve the quality of life in the city of Detroit, state of Michigan and throughout the world. For more information about research at Wayne State University, visit

Research background

"Search for Type 1a supernova NUV-Optical Subclasses," by David Cinabro and Jake Miller (Wayne State University); and Daniel Scolnic and Ashley Li (Kavli Institute for Cosmological Physics at the University of Chicago); and Richard Kessler (Kavli Institute for Cosmological Physics at University of Chicago and the Department of Astronomy and Astrophysics at the University of Chicago). Monthly Notices of the Royal Astronomical Society, November 2016. DOI: 10.1093/mnras/stw3109

Funding for this research was provided by the Kavli Institute for Cosmological Physics at the University of Chicago, Kavli Foundation, Fred Kavli, Space Telescope Science Institute, and National Aeronautics and Space Administration.

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