Kate Scholberg

Kate Scholberg

Arts & Sciences Distinguished Professor of Physics

Professor of Physics

Associate Chair of Physics

Associate of the Duke Initiative for Science & Society

Bass Fellow

Office Location: 
273 Physics Bldg, Durham, NC 27708
Front Office Address: 
Box 90305, Durham, NC 27708-0305
(919) 660-2962


Prof. Scholberg's broad research interests include experimental elementary particle physics, astrophysics and cosmology. Her main specific interests are in neutrino physics: she studies neutrino oscillations with the Super-Kamiokande experiment, a giant underground water Cherenkov detector located in a mine in the Japanese Alps. Super-K was constructed to search for proton decay and to study neutrinos from the sun, from cosmic ray collisions in the atmosphere, and from supernovae. On Super-K, Prof. Scholberg's primary involvement is with the atmospheric neutrino data analysis, which in 1998 yielded the first convincing evidence for neutrino oscillation (implying the existence of non-zero neutrino mass).

One of the most important questions that we may be able to answer with neutrino oscillation experiments over the next couple of decades is the question of CP (charge conjugation-parity) violation in neutrinos. It's now well known that processes involving quarks violate CP symmetry; it's suspected that the same is true for leptons (such as neutrinos), but leptonic CP violation is as yet unobserved. We hope that understanding of CP violation, along with knowledge of the other neutrino parameters, may lead to insight into the question of the observed matter-antimatter asymmetry of the universe. The long-term program neutrino oscillation physics aims to answer these questions.

The next steps in neutrino oscillation research involve artificial beams of neutrinos sent hundreds of kilometers from accelerator laboratories to underground detectors. The T2K ("Tokai to Kamioka") high-intensity beam experiment sends neutrinos 300 km from an accelerator at the J-PARC facility in Japan to Super-K, and is currently exploring unknown oscillation parameters. The DUNE (Deep Underground Neutrino Experiment) is a planned next-generation U.S.-based international experiment designed to observe neutrinos beamed from Fermilab to a large liquid argon detector at a new underground facility in South Dakota.  One of Prof. Scholberg's particular interests on DUNE is the detector's sensitivity to the huge bursts of neutrinos from core-collapse supernovae.

Prof. Scholberg serves as spokesperson of COHERENT, a multi-detector experiment with the primary physics goal of measuring CEvNS (Coherent Elastic Neutrino Nucleus Scattering) using the high-intensity neutrinos produced by the Spallation Neutron Source at Oak Ridge National Laboratory in Tennessee.   CEvNS was measured for the first time by the collaboration in 2017.

Prof. Scholberg was a co-founder of SNEWS, the SuperNova Early Warning System, an inter-experiment collaboration of detectors with Galactic supernova sensitivity. Neutrinos from a core collapse will precede the photon signal by hours; therefore coincident observation of a burst in several neutrino detectors will be a robust early warning of a visible supernova. The goals of SNEWS are to provide the astronomical community with a prompt alert of a Galactic core collapse, as well as to optimize global sensitivity to supernova neutrino physics.

Education & Training

  • Ph.D., California Institute of Technology 1996

  • M.S., California Institute of Technology 1991

  • B.Sc., McGill University (Canada) 1989

Ambrosio, M., et al. “The observation of up-going charged particles produced by high energy muons in underground detectors.” Astroparticle Physics, vol. 9, no. 2, Jan. 1998, pp. 105–17. Scopus, doi:10.1016/S0927-6505(98)00010-3. Full Text

Ambrosio, M., et al. “Real time supernova neutrino burst detection with MACRO.” Astroparticle Physics, vol. 8, no. 3, Jan. 1998, pp. 123–33. Scopus, doi:10.1016/S0927-6505(97)00032-7. Full Text

Shiozawa, M., et al. “Search for proton decay via p→e+π0 in a large water cherenkov detector.” Physical Review Letters, vol. 81, no. 16, Jan. 1998, pp. 3319–23. Scopus, doi:10.1103/PhysRevLett.81.3319. Full Text

Giglietto, N., et al. “Performance of the MACRO detector at Gran Sasso: Moon shadow and seasonal variations.” Nuclear Physics B  Proceedings Supplements, vol. 61, no. 3 SUPPL., Jan. 1998, pp. 180–84. Scopus, doi:10.1016/S0920-5632(97)00559-8. Full Text

Ambrosio, M., et al. “Magnetic monopole search with the MACRO detector at Gran Sasso.” Physics Letters, Section B: Nuclear, Elementary Particle and High Energy Physics, vol. 406, no. 3, Aug. 1997, pp. 249–55. Scopus, doi:10.1016/S0370-2693(97)00684-9. Full Text

Ambrosio, M., et al. “High energy cosmic ray physics with the MACRO experiment at Gran Sasso.” Nuclear Physics B  Proceedings Supplements, vol. 52, no. 3, Elsevier BV, Feb. 1997, pp. 172–75. Crossref, doi:10.1016/s0920-5632(96)00869-9. Full Text

Ambrosio, M., et al. “Seasonal variations in the underground muon intensity as seen by MACRO.” Astroparticle Physics, vol. 7, no. 1–2, Jan. 1997, pp. 109–24. Scopus, doi:10.1016/S0927-6505(97)00011-X. Full Text

Ambrosio, M., et al. “High energy cosmic ray physics with underground muons in MACRO. I. Analysis methods and experimental results.” Physical Review D  Particles, Fields, Gravitation and Cosmology, vol. 56, no. 3, Jan. 1997, pp. 1407–17. Scopus, doi:10.1103/PhysRevD.56.1407. Full Text

Ambrosio, M., et al. “High energy cosmic ray physics with underground muons in MACRO. II. Primary spectra and composition.” Physical Review D  Particles, Fields, Gravitation and Cosmology, vol. 56, no. 3, Jan. 1997, pp. 1418–36. Scopus, doi:10.1103/PhysRevD.56.1418. Full Text