UA Scientists among IceCube Collaborators Pushing Neutrinos to Astronomy’s Forefront

An image of an "event" recorded by the IceCube detector is superimposed atop Bryant-Denny Stadium to provide a size comparison in this photo illustration. When a neutrino collides with an ice molecule inside the detector, light is radiated. This light can be detected by one of the 5,160 sensors encompassed within a cubic kilometer of ice (IceCube Collaboration/Google Maps).
An image of an “event” recorded by the IceCube detector is superimposed atop Bryant-Denny Stadium to provide a size comparison in this photo illustration. When a neutrino collides with an ice molecule inside the detector, light is radiated. This light can be detected by one of the 5,160 sensors encompassed within a cubic kilometer of ice (IceCube Collaboration/Google Maps).

MADISON, Wisc. — The IceCube Neutrino Observatory, a particle detector buried in the Antarctic ice, is a demonstration of the power of the human passion for discovery, where scientific ingenuity meets technological innovation. Today, nearly 25 years after the pioneering idea of detecting neutrinos in ice, the IceCube Collaboration, including University of Alabama researchers, announces the observation of 28 very high-energy particle events that constitute the first solid evidence for astrophysical neutrinos from cosmic accelerators.

“We believe we are seeing, for the first time, extremely high-energy neutrinos from a source outside of our solar system,” said Dr. Dawn Williams, an associate professor of physics at The University of Alabama, who serves as the project’s calibration coordinator.

“It is gratifying to finally see what we have been looking for,” said Dr. Francis Halzen, principal investigator of IceCube and the Hilldale and Gregory Breit Distinguished Professor of Physics at the University of Wisconsin–Madison.  This is the dawn of a new age of astronomy.”

Details of the research appear in a manuscript publishing Nov. 22 in Science. Williams was among the article’s many co-authors, which also included Drs. Patrick Toale, UA assistant professor of physics,  Dr. Pavel Zarzhitsky, a former UA post-doctoral researcher, and UA graduate students,  Michael Larson, James Pepper and Donglian Xu.

Because they rarely interact with matter, the nearly massless subatomic particles called neutrinos can carry information about the workings of the highest-energy and most distant phenomena in the universe. Billions of neutrinos pass through every square centimeter of the Earth every second, but the vast majority originate either in the sun or in the Earth’s atmosphere.

Far rarer are neutrinos from the outer reaches of our galaxy or beyond, which have long been theorized to provide insights into the powerful cosmic objects where high-energy cosmic rays may originate: supernovas, black holes, pulsars, active galactic nuclei and other extreme extragalactic phenomena.

IceCube, run by the international IceCube Collaboration and headquartered at the Wisconsin IceCube Particle Astrophysics Center at UW–Madison, was designed to accomplish two major scientific goals: measure the flux, or rate, of high-energy neutrinos and try to identify some of their sources.

The analysis presented in Science reveals the first high-energy neutrino flux ever observed, a highly statistically significant signal that meets expectations for neutrinos originating in cosmic accelerators.

“Its an interesting energy window into astronomy,” UA’s Williams said. “The energy of our neutrinos is higher than the energy of any neutrinos that have ever been observed before.”

One theory is these high-energy neutrinos may share a source with high-energy cosmic rays, Williams said. The origin of those rays is said to be one of physics’ most enduring mysteries.

“The highest energy cosmic rays that have been detected have the equivalent energy of  a mosquito,” said UA’s Toale. “These are elementary particles. This is a tremendous amount of energy for such a tiny object. The question is, how do they get this energy? One of the ideas is that they are accelerated much like our man-made accelerators. But, this is millions of times higher in energy than what we can produce in a lab.”

“IceCube is a wonderful and unique astrophysical telescope – it is deployed deep in the Antarctic ice but looks over the entire Universe, detecting neutrinos coming through the Earth from the northern skies, as well as from around the southern skies,” says Vladimir Papitashvili of the National Science Foundation Division of Polar Programs.

“The IceCube Neutrino Observatory has opened a new era in neutrino astrophysical observations,” adds Jim Whitmore of the NSF’s Physics Division, who with Papitashvili manages operation of the observatory and the associated U.S. research projects. “It is in the forefront of the entire field of neutrino astronomy, now delivering observations that have been long-awaited by both theorists and experimentalists.”

The 28 high-energy neutrinos were found in data collected by the IceCube detector from May 2010 to May 2012 and analyzed for neutrino events exceeding 50 teraelectronvolts coming from anywhere in the sky. The events cannot be explained by other neutrino fluxes, such as those from atmospheric neutrinos, nor by other high-energy events, such as muons produced by the interaction of cosmic rays in the atmosphere. Preliminary results of this analysis were presented May 15 at the IceCube Particle Astrophysics Symposium at UW–Madison.

“Now that we have the full detector we have the sensitivity to see these events. After seeing hundreds of thousands of atmospheric neutrinos, we have finally found something different,” Halzen explains. “We’ve been waiting for this for so long.”

IceCube is composed of 5,160 digital optical modules suspended along 86 strings embedded in a cubic kilometer of ice beneath the South Pole. The National Science Foundation-supported observatory detects neutrinos through the tiny flashes of blue light, called Cherenkov light, produced when neutrinos interact in the ice.

The IceCube detector was completed in December 2010 after seven years of construction. It was built on time and on budget and in its first two years has performed above its design specifications.

“The success of IceCube builds on the efforts of hundreds of people around the world,” says Botner. “IceCube collaborators made it all happen – from the design and the deployment in a harsh environment, proving the feasibility of the concept, to data harvesting and physics analysis. All required concerted efforts that ultimately have led to the observations presented in this paper. Now the collaboration is addressing a further challenge: how to make IceCube a big contributor to astronomy.”

UA’s portion of the funding connected with this research comes from an approximate $500,000 NSF grant awarded to Williams that continues through 2015.

The IceCube Neutrino Observatory was built under a NSF Major Research Equipment and Facilities Construction grant, with assistance from partner funding agencies around the world. The NSF’s Division of Polar Programs and Physics Division continue to support the project with a Maintenance and Operations grant, along with international support from participating institutes and their funding agencies. UW–Madison is the lead institution, and the international collaboration includes 250 physicists and engineers from the U.S., Germany, Sweden, Belgium, Switzerland, Japan, Canada, New Zealand, Australia, U.K. and Korea.

The scientific paper may be accessed by clicking here.

UA’s department of physics and astronomy is part of the College of Arts and Sciences, the University’s largest division and the largest liberal arts college in the state. Students from the College have won numerous national awards including Rhodes Scholarships, Goldwater Scholarships and memberships on the USA Today Academic All American Team.


Silvia Bravo Gallart, outreach specialist, Wisconsin IceCube Particle Astrophysics Center, 608/263-9108,; Chris Bryant, UA media relations, 205/348-8323,


Dr. Dawn Williams,; Dr. Patrick Toale, 205/348-5823,