The Pierre Auger Collaboration has found evidence that the highest energy cosmic rays are produced by active galactic nuclei. This international collaboration of physicists announced in the cover story of the November 9th (2007) issue of Science Magazine that they observe a statistically significant correlation between the arrival directions of the highest energy cosmic rays and positions of these objects that are less than 240 million light years from Earth. Active galactic nuclei are believed to be supermassive black holes that are consuming gas and dust at the centers of some galaxies. The correlation is based on 27 particles, with energy in excess of 10 Joules each, which were recorded while the observatory was being constructed in Argentina. The array of detectors in Argentina has now reached its full size of 3000 square kilometers, and a northern site for the Auger Observatory is planned for southeast Colorado. The Penn State team involved in this project include Sanjeevi Atulugama, Jose Bellido, Stephane Coutu, Adrienne Criss, Michael Roberts and Paul Sommers. Paul Sommers was also elected co-spokesperson for the Pierre Auger Collaboration beginning in November 2007.
The Center for Particle and Gravitational Astrophysics is engaged in a bold synergistic approach to understanding high energy processes in the universe. Our faculty at Penn State are prominent participants seven major international projects which make observations using extremely high energy protons and nuclei, neutrinos, gamma-rays, X-rays and gravitational waves. These projects are, respectively, the Pierre Auger Cosmic Ray Observatory, the IceCube Neutrino Observatory, the Swift Gamma-Ray Burst Explorer satellite, the Chandra X-ray Observatory, the XMM-Newton X-ray Observatory, the Laser Interferometric Gravitational Wave Observatory (LIGO) and the North American Nanohertz Observatory for Gravitational-waves (NANOGrav).
Our faculty are also involved in developing future facilities such as the International X-ray Observatory, the Large Synoptic Survey Telescope (LSST) and the Joint Astrophysics Nascent Universe Satellite (JANUS). Two projects in TeV gamma ray astronomy are the High Altitude Water Cherenkov (HAWC) observatory and the Advanced Gamma-ray Imaging System (AGIS). There is also ongoing work with the Fermi satellite, the VERITAS high energy gamma ray observatory, the Cosmic Ray Energetics and Mass (CREAM), the Cosmic Ray Electron Synchrotron Telescope (CREST) high-altitude balloon, and in the former Laser Interferometer Space Antenna (LISA) project, now called NGO.
Penn State is the only U.S. institution participating in both Auger and IceCube, the premier ground-based projects of high energy particle astrophysics. Potentially observable sources for both Auger and IceCube include super-massive black holes at the center of active galaxies, and the explosive phenomena that give rise to gamma ray bursts (GRBs). Some GRBs are believed to be especially violent supernova explosions, while others are probably mergers of collapsed stars in binary systems.
The Swift GRB Explorer satellite is presently providing the best gamma ray and X-ray observations of GRB explosions. Swift has been successfully operating for a number of years, its mission control center being at Penn State. Chandra and XMM have been successfully operating for over a decade and are leading to substantial advances in understanding the demography, physics, and ecology of supermassive and stellar mas black holes, active galaxies and supernovae. LIGO is undergoing a major upgrade towards achieving its ultimate sensitivity.
Commensurate with these significant experimental efforts, Penn State also plays a leading role in the theoretical and numerical modeling of fundamental high energy interactions as well as astrophysical phenomena such as black holes, gamma-ray bursts, the high energy Universe and the formation of the first objects and large scale structures in the Universe.
GRBs, and the mergers of super-massive black holes in the cores of galaxies and quasars are also likely sources of detectable gravitational waves. Our Center will be studying GRBs and active galaxies by observing strong-interaction protons and nuclei, weak-interaction neutrinos, electromagnetic radiation, and gravitational waves. Together we cover all four forces of nature. We have initiated a specific multi-messenger observational program called the Astrophysical Multimessenger Observatory Network (AMON), which aims to utilize all four forces to detect sub-threshold signals from the above described cosmic sources. This multi-force approach to high energy astrophysics is a pioneering venture in which the one-dimensional electromagnetic spectrum of conventional astronomy is supplemented with three other windows to the Universe. The discovery potential is enormous.
Together with the Center for Fundamental Theory, the Center for Theoretical and Observational Cosmology and the Institute for Gravitation and the Cosmos, the synergy between our various specialties and the breadth of knowledge to be gained through collaborations provide exciting prospects for making breakthroughs in our understanding of the Cosmos.