by Staff Writers
Amsterdam, Netherlands (SPX) Feb 05, 2016
The puzzling excess of gamma rays from the center of the Milky Way probably originates from rapidly rotating neutron stars, or millisecond pulsars, and not from dark matter annihilation, as previously claimed.
This is the conclusion of new data analyzes by two independent research teams from the University of Amsterdam (UvA) and Princeton University/Massachusetts Institute of Technology. The researchers' findings are published in Physical Review Letters.
In 2009 observations with the Fermi Large Area Telescope revealed an excess of high-energy photons, or gamma rays, around 2 GeV (giga-electron volts) at the center of our galaxy. It was long speculated that this gamma ray excess could be a signal of dark matter annihilation. If true, it would constitute a breakthrough in fundamental physics and a major step forward in our understanding of the matter constituents of the universe.
However, many other hypotheses have emerged in recent years, suggesting the gamma ray excess in the center of our galaxy might have a more ordinary, astrophysical cause. Possible origins for the observed gamma ray excess range from the activity of the supermassive black hole in the center of our Milky Way and star formation in the central molecular zone to the combined emission of a new dim source population in the galactic bulge.
Millisecond pulsars, or rapidly rotating neutron stars, were often formed billions of years ago. They are among the most extreme objects in the galaxy. A population of hundreds or thousands of these millisecond pulsars must be lurking in the galactic center, hidden from detection due to present day instrument sensitivity. Future radio surveys with existing and upcoming telescopes (e.g., Green Bank Telescope, Square Kilometre Array) will be able to further test this hypothesis in the coming years.
According to Weniger, lead author of one of the papers, this is a win-win situation: "Either we find hundreds or thousands of millisecond pulsars in the upcoming decade, shedding light on the history of the Milky Way, or we find nothing. In the latter case, a dark matter explanation for the gamma ray excess will become much more obvious."
Mariangela Lisanti, assistant professor at Princeton University and one of the authors of the second paper, adds: "The results of our analysis probably mean that what we are seeing is evidence for a new population of astrophysical sources in the center of the galaxy. That in itself is something new and surprising."
References: "Strong Support for the Millisecond Pulsar Origin of the Galactic Center GeV Excess," Richard Bartels, Suraj Krishnamurthy and Christoph Weniger, 2016 Feb. 4, Physical Review Letters - "Evidence for Unresolved Gamma-Ray Point Sources in the Inner Galaxy," Samuel K. Lee, Mariangela Lisanti, Benjamin R. Safdi, Tracy R. Slatyer and Wei Xue, 2016 Feb. 4, Physical Review Letters
University of Amsterdam
Stellar Chemistry, The Universe And All Within It
|The content herein, unless otherwise known to be public domain, are Copyright 1995-2017 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. Privacy Statement|