Neutrinos

Neutrinos are light, electrically-neutral elementary particles that make up the least-understood part of the Standard Model of particle physics. Facilities like DUNE (the Deep Underground Neutrino Experiment) study neutrinos produced in the Fermilab collider as well as neutrinos arriving from cosmic events. Project 8 will measure neutrino mass by looking at neutrinos emitted when tritium decays. The CMB Stage 4 telescopes will use cosmological data to constrain the number of neutrinos and their mass. Many other neutrino facilities focus on detecting neutrinos produced in astrophysical processes, including ANITA, ARA, BEACON, GRAND, IceCube, PUEO, and RNO-G. These cosmic neutrinos can carry key information, along with electromagnetic radiation and gravitational waves, in "multi-messenger" detections of dynamic events in the universe.



IGC members who study Neutrinos

NameRoleAffiliationEmailPhoneOffice AddressAffiliated Center(s) Research Topics(s)
Tyler Anderson Faculty Physics tba109@psu.edu +1 814 865 2013 212A Osmond Laboratory CMA Cosmic Rays, Dark Matter, Neutrinos, Multimessenger Astrophysics
Mukul Bhattacharya Postdoc Astronomy, Physics mmb5946@psu.edu -- 320A Osmond Laboratory CMA Multimessenger Astrophysics, Gravitational Waves, Neutrinos, Cosmic Rays
Carmen Carmona Benitez Faculty Physics mzc267@psu.edu +1 814 865 6476 320D Osmond Laboratory CMA Dark Matter, Neutrinos
Jose Carpio Dumler Graduate Student Physics jac866@psu.edu +1 814 865 7533 -- NONE CMA Neutrinos, Multimessenger Astrophysics, Dark Matter
Douglas Cowen Faculty Physics dfc13@psu.edu +1 814 863 5943 303D Osmond Laboratory CMA Dynamic Universe, Neutrinos, Multimessenger Astrophysics
Abhishek Das Graduate Student ICDS, Physics, Astronomy ajd6518@psu.edu -- 321E Thomas Building IGC, CMA Cosmic Rays, Black Holes, Neutrinos, Gravitational Waves, Multimessenger Astrophysics, Dark Matter, Quasars
Luiz de Viveiros Faculty Physics lad57@psu.edu +1 814 865 7533 320E Osmond Laboratory CMA Neutrinos, Dark Matter
Kayla DeHolton Postdoc Physics kld5938@psu.edu -- 303A Osmond Laboratory CMA Neutrinos
Pedro Espino Postdoc Physics ple5069@psu.edu -- 320 Whitmore Laboratory IGC Neutrinos, Gravitational Waves, Multimessenger Astrophysics
Derek Fox Faculty Astronomy dbf11@psu.edu +1 814 863 4989 425 Davey Laboratory CMA, CTOC Dynamic Universe, Neutrinos, Multimessenger Astrophysics
Eduardo Gutiérrez Postdoc Physics exg5366@psu.edu +1 814 863 9605 301B Whitmore Laboratory IGC Black Holes, Multimessenger Astrophysics, Neutrinos, Gravitational Waves, Cosmic Rays
Peter Hammond Postdoc Physics pph5189@psu.edu +1 814 863 9605 307 Whitmore Laboratory IGC Neutrinos, Gravitational Waves, Multimessenger Astrophysics
Bryan Hendricks Graduate Student Physics blh5615@psu.edu 815-216-0835 204 Osmond Laboratory IGC Neutrinos
Kaeli Hughes Postdoc Astronomy, Physics kaeli@psu.edu +1 6142906343 N/A Davey Laboratory CMA Neutrinos, Cosmic Rays, Multimessenger Astrophysics
Ali Kheirandish Graduate Student Physics abk5717@psu.edu +1 814 865 7533 -- Davey Laboratory CMA Neutrinos, Multimessenger Astrophysics, Dark Matter
Ryan Krebs Graduate Student Physics rjk5416@psu.edu (814) 865-7533 322 Osmond Laboratory CMA, IGC Neutrinos, Multimessenger Astrophysics
Yuchieh Ku Graduate Student Physics yuchieh@psu.edu 8148628153 204 Osmond Laboratory IGC Neutrinos
Irina Mocioiu Faculty Physics ium4@psu.edu +1 814 865 3721 320G Osmond Laboratory CMA Neutrinos
Richard Mueller Graduate Student Physics rjm6826@psu.edu +1 814 865 7533 6E Osmond Laboratory IGC Neutrinos
Mainak Mukhopadhyay Postdoc Astronomy, Physics mkm7190@psu.edu -- 320L Osmond Laboratory CMA Multimessenger Astrophysics, Gravitational Waves, Neutrinos
Kohta Murase Faculty Physics, Astronomy kum26@psu.edu +1 814 863 9594 321B Osmond Laboratory CMA Cosmic Rays, Neutrinos, Multimessenger Astrophysics, Gravitational Waves, Dark Matter
Marco Muzio Postdoc Astronomy, Physics msm6428@psu.edu -- 322 Osmond Laboratory CMA Multimessenger Astrophysics, Neutrinos, Cosmic Rays
Peter Mészáros Faculty Physics, Astronomy nnp@psu.edu 814-863-4167 504 Davey Laboratory CMA Gravitational Waves, Neutrinos, Multimessenger Astrophysics
Surendra Padamata Graduate Student Physics ssp5361@psu.edu -- 322 Osmond Laboratory CMA Multimessenger Astrophysics, Black Holes, Cosmic Rays, Gravitational Waves, Neutrinos
Yi Qiu Graduate Student Physics yiqiu@psu.edu 8142328268 322 Whitmore Laboratory IGC Gravitational Waves, Black Holes, Neutrinos, Multimessenger Astrophysics
David Radice Faculty Astronomy, Physics dur566@psu.edu +1 814 865 7533 304 Whitmore Laboratory CMA Black Holes, Neutrinos, Multimessenger Astrophysics, Gravitational Waves
Steinn Sigurdsson Faculty Astronomy sxs540@psu.edu +1 814 863 6038 426 Davey Laboratory CMA Neutrinos, Black Holes, Multimessenger Astrophysics
Stephanie Wissel Faculty Astronomy, Physics wissel@psu.edu +1 814 863 9598 303B Osmond Laboratory CTOC, CFT, CMA Multimessenger Astrophysics, Cosmic Rays, Neutrinos
Chengchao Yuan Graduate Student Physics cxy52@psu.edu +1 814 865 0153 -- NONE CMA Neutrinos, Multimessenger Astrophysics, Cosmic Rays
Andrew Zeolla Graduate Student Physics avz5228@psu.edu 7138709006 204 Osmond Laboratory CMA Multimessenger Astrophysics, Neutrinos, Cosmic Rays
Andrew Ziegler Graduate Student Physics ziegler@psu.edu -- 6E Osmond Laboratory CMA Neutrinos

News about Neutrinos

What happens when neutron stars collide?

2024-06-18

When stars collapse, they can leave behind incredibly dense but relatively small and cold remnants called neutron stars. If two stars collapse in close proximity, the leftover binary neutron stars spiral in and eventually collide, and the interface where the two stars begin merging becomes incredibly hot. New simulations of these events show hot neutrinos — tiny, essentially massless particles that rarely interact with other matter — that are created during the collision can be briefly trapped at these interfaces and remain out of equilibrium with the cold cores of the merging stars for 2 to 3 milliseconds. During this time, the simulations show that the neutrinos can weakly interact with the matter of the stars, helping to drive the particles back toward equilibrium — and lending new insight into the physics of these powerful events.

Click here for the full article.

Additional links:


IceCube identifies seven astrophysical tau neutrino candidates.

2024-03-12

The IceCube Neutrino Observatory, a cubic-kilometer-sized neutrino telescope at the South Pole, has observed a new kind of astrophysical messenger. In a new study recently accepted for publication as an Editors' Suggestion by the journal Physical Review Letters and available online as a preprint, the IceCube collaboration, including Penn State researchers, presented the discovery of seven of the once-elusive astrophysical tau neutrinos.

Click here for the full article.

Additional links:


IceCube Observatory Produces First Image of the Milky Way using Neutrinos

2023-07-06

Our Milky Way galaxy is an awe-inspiring feature of the night sky, viewable with the naked eye as a horizon-to-horizon hazy band of stars. Now, for the first time, the IceCube Neutrino Observatory has produced an image of the Milky Way using neutrinos — tiny, ghostlike astronomical messengers that are extremely difficult to detect because they rarely interact with matter. In an article published online today (June 29), in the journal Science, the IceCube Collaboration, an international group of over 350 scientists, including Penn State researchers, presents evidence of high-energy neutrino emission from the Milky Way.

“Most of what we know about our universe and our host galaxy we have learned by observing electromagnetic radiation — this includes visible light but stretches in energy from radio waves to x-rays and gamma rays,” said Doug Cowen, professor of physics in the Penn State Eberly College of Science and a member of the IceCube Collaboration. “This new image of the Milky Way using neutrinos is completely different and allows us to explore questions about the origins and workings of our galaxy in new ways.”

The high-energy neutrinos, with energies millions to billions of times higher than those produced by the fusion reactions that power stars, were detected by the IceCube Neutrino Observatory, a gigaton detector operating at the Amundsen-Scott South Pole Station. It was built and is operated with National Science Foundation (NSF) funding and additional support from the 14 countries that host institutional members of the IceCube Collaboration. This one-of-a-kind detector encompasses a cubic kilometer of deep Antarctic ice instrumented with over 5,000 light sensors. IceCube searches for signs of high-energy neutrinos originating from our galaxy and beyond, out to the farthest reaches of the universe. “As is so often the case, significant breakthroughs in science are enabled by advances in technology,” said Denise Caldwell, director of NSF’s Physics Division. “The capabilities by the highly sensitive IceCube detector, coupled with new data analysis tools, have given us an entirely new view of our galaxy — one that had only been hinted at before. As these capabilities continue to be refined, we can look forward to watching this picture emerge with ever-increasing resolution, potentially revealing hidden features of our galaxy never before seen by humanity.”

Interactions between cosmic rays — high-energy protons and heavier nuclei, also produced in our galaxy–and galactic gas and dust inevitably produce both gamma rays and neutrinos. Given the observation of gamma rays from the galactic plane, the Milky Way was expected to be a source of high-energy neutrinos, according to the research team.

IceCube has previously detected energetic neutrinos from astrophysical sources at much greater remove than our own Milky Way galaxy, but those sources were situated in the northern sky, allowing analyzers to use the Earth as a filter to remove everything but neutrinos. Due to the orientation of the Earth in the Milky Way, many potential galactic sources of neutrinos are located in the southern sky.

“That means that analyzers had to devise other methods to reduce the background from particles raining down on the detector from cosmic-ray interactions in the atmosphere in the vicinity of the South Pole,” said Cowen. “Those particles would otherwise completely obscure the galactic neutrino signal.”

To overcome this background, IceCube collaborators at Drexel University developed analyses that select for “cascade” events, or neutrino interactions in the ice that result in localized, roughly spherical showers of light. Because the deposited energy from cascade events starts within the instrumented volume, contamination of atmospheric muons and neutrinos is reduced. Ultimately, the higher purity of the cascade events gave a better sensitivity to astrophysical neutrinos from the southern sky. However, the final breakthrough came from the implementation of machine learning methods, developed by IceCube collaborators at TU Dortmund University, that improve the identification of cascades produced by neutrinos as well as their direction and energy reconstruction. The observation of neutrinos from the Milky Way is a hallmark of the emerging critical value that machine learning provides in data analysis and event reconstruction in IceCube.

“The improved methods allowed us to retain over an order of magnitude more neutrino events with better angular reconstruction, resulting in an analysis that is three times more sensitive than the previous search,” said IceCube member, TU Dortmund physics doctoral student and co-lead analyzer Mirco Hünnefeld.

The dataset used in the study included 60,000 neutrinos spanning 10 years of IceCube data, 30 times as many events as the selection used in a previous analysis of the galactic plane using cascade events. These neutrinos were compared to previously published prediction maps of locations in the sky where the galaxy was expected to shine in neutrinos.

The maps included one made from extrapolating Fermi Large Area Telescope gamma-ray observations of the Milky Way and two alternative maps identified as KRA-gamma by the group of theorists who produced them.

“This long-awaited detection of cosmic ray-interactions in the galaxy is also a wonderful example of what can be achieved when modern methods of knowledge discovery in machine learning are consistently applied,” said Wolfgang Rhode, professor of physics at TU Dortmund University, IceCube member and Hünnefeld’s adviser.

The power of machine learning offers great future potential, bringing other observations closer within reach.

Click here for the full article.

Additional links:


Icecube Neutrinos Give First Glimpse Into the Inner Depths of an Active Galaxy

2022-11-09

UNIVERSITY PARK, Pa. — For the first time, an international team including Penn State scientists has found evidence of high-energy neutrino emission from Messier 77, also known as NGC 1068, an active galaxy in the constellation of Cetus.

Neutrinos are fundamental particles with no charge and almost no mass, and they rarely interact with other matter. High-energy neutrinos — like those detected here with energies in the teraelectron volt (TeV), or trillion-electron volt, range — can travel for billions of light-years through space without being deflected or absorbed. Thus, while they are extremely difficult to detect, they can provide accurate information about the distant universe, especially when the information the carry can be combined with information from other cosmic signals in what is called “multimessenger” astronomy.

The detection was made by the IceCube Neutrino Observatory, a massive neutrino telescope encompassing one billion tons of instrumented ice at depths from 1.5 to 2.5 kilometers below Antarctica’s surface near the South Pole.

“IceCube is a veritable discovery machine,” said Doug Cowen, professor of physics and of astronomy and astrophysics at Penn State and a long-time IceCube collaborator. “The huge detector has lived up to its promise to launch the brand-new field of high energy neutrino astronomy, and then some, now by giving us glimpses behind a black hole’s black-out curtain of matter. IceCube has once again proved that when humanity points a new instrument at the heavens — starting with Galilleo’s first telescope — our knowledge of the universe around us increases by leaps and bounds.”

This unique telescope, which explores the farthest reaches of our universe using weakly interacting neutrinos instead of light, recorded the first observation of a potential source of high-energy astrophysical neutrinos in 2017. The source of these first observations is the known blazar TXS 0506+056, which is situated in the night sky just off the left shoulder of the constellation Orion and about 4 billion light-years from Earth.

Blazars are very luminous and distant active galaxies with a powerful, relativistic jet of particles pointing directly at us. Unlike NGC 1068, the blazar TXS 0506+056 had not been studied much before the multimessenger detection of neutrinos and high-energy electromagnetic radiation that allowed follow-up measurements by almost 20 telescopes around the world. Now, the observation of neutrino emission from a different type of active galaxy brings us closer to understanding the supermassive black holes powering them.

“One neutrino can single out a source. But only an observation with multiple neutrinos will reveal the obscured core of the most energetic cosmic objects,” said Francis Halzen, a professor of physics at the University of Wisconsin–Madison, the headquarters of the National Science Foundation (NSF)´s Antarctic neutrino facility, and principal investigator of IceCube. “IceCube has accumulated some 80 neutrinos of TeV energy from NGC 1068, which are not yet enough to answer all our questions, but they definitely are the next big step towards the realization of neutrino astronomy.”

The results appear Nov. 4 in the journal Science.

Click here for the full article.

Additional links:



About our wordmark
Monica The IGC wordmark was created by Monica Rincon Ramirez, while she was a graduate student at the Institute for Gravitation and the Cosmos (IGC). Monica enjoys drawing new connections between fundamental theory and observations. Her graduate work includes specialized topics in general relativity, loop quantum gravity, and quantum fields in cosmological backgrounds. In particular, her thesis work focused on finding effective quantum corrections to gravitational phenomena from spinfoams, and applications to cosmology. She received her PhD in 2024.

The wordmark symbolizes the scope and variety of research at the IGC. The base of the image represents quantum gravity, evoking the quantum geometrical picture from spinfoams and loop quantum gravity. These are among the approaches to fundamental questions studied at the Center for Fundamental Theory. The middle of the image represents the Center for Theoretical and Observational Cosmology by galaxies embedded in a smooth surface, characteristic of spacetime in general relativity and the much larger physical scales studied in cosmology. Finally, at the top, the surface curves to an extreme, representing a supermassive black hole accompanied by an energetic jet. These elements depict an active galactic nucleus, inspired by Centaurus A. Just to the right, a pair of black holes approaches merger. This top portion of the wordmark represents the Center for Multimessenger Astrophysics, which specializes in the study of high-energy phenomena in the universe.