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Record W4377291653 · doi:10.3847/2041-8213/acd2c9

Constraining High-energy Neutrino Emission from Supernovae with IceCube

2023· article· en· W4377291653 on OpenAlexaff
Rasha Abbasi, M. Ackermann, J. Adams, Sanjib Kumar Agarwalla, J. A. Aguilar, M. Ahlers, Jean-Marco Alameddine, N. M. Amin, K. Andeen, G. Anton, C. Argüelles, Yosuke Ashida, S. Athanasiadou, Spencer Axani, X. Bai, Aswathi Balagopal, M. Baricevic, S. W. Barwick, Vedant Basu, R. Bay, J. J. Beatty, Karl H. Becker, J. Becker Tjus, Jakob Beise, Chiara Bellenghi, S. BenZvi, D. Berley, E. Bernardini, D. Besson, G. Binder, D. Bindig, E. Blaufuss, Summer Blot, Federico Bontempo, Julia Book, Caterina Boscolo Meneguolo, S. Böser, O. Botner, J. Böttcher, Etienne Bourbeau, J. Braun, Bennett Brinson, Jannes Brostean-Kaiser, Ryan T. Burley, Raffaela Busse, Delaney Butterfield, Michael Campana, K. Carloni, Erin Carnie-Bronca, S. Chattopadhyay, Kunal Deoskar, Z. Chen, D. Chirkin, S. Choi, Brian Clark, Lew Classen, Alan Coleman, G. H. Collin, A. Connolly, J. M. Conrad, Paul Coppin, Pablo Correa, S. T. Countryman, D. F. Cowen, Pranav Dave, C. De Clercq, James DeLaunay, Diyaselis Delgado, H.-P. Dembinski, Abhishek Desai, P. Desiati, K. D. de Vries, G. de Wasseige, T. DeYoung, A. Diaz, J. C. Díaz–Vélez, Markus Dittmer, Alba Domi, Hrvoje Dujmović, M. A. DuVernois, Thomas Ehrhardt, P. Eller, R. Engel, Hannah Erpenbeck, John Evans, P. A. Evenson, Kwok Lung Fan, Ke Fang, A. R. Fazely, Anatoli Fedynitch, Nora Feigl, Sebastian Fiedlschuster, C. Finley, Leander Fischer, D. B. Fox, A. Franckowiak, Edward Friedman, Alexander Fritz, Philipp Fürst, T. K. Gaisser, J. S. Gallagher, Erik Ganster, Alfonso Garcia, S. Garrappa, L. Gerhardt, Christian Gläser, Theo Glauch, T. Glüsenkamp, N. Goehlke, J. G. González, D. Grant, S. J. Gray, S. Griffin, Spencer Griswold, C. Günther, Pascal Gutjahr, Christian Haack, A. Hallgren, R. Halliday, L. Halve, F. Halzen, H. Hamdaoui, Martin Ha Minh, K. Hanson, John Hardin, Alexander Harnisch, P. Hatch, A. Haungs, K. Helbing, Jonas Hellrung, Felix Henningsen, Lars Philipp Heuermann, S. Hickford, Attila Hidvégi, Colton Hill, G. C. Hill, K. D. Hoffman, K. Hoshina, Wenjie Hou, Thomas Huber, K. Hultqvist, Mirco Hünnefeld, Raamis Hussain, Karolin Hymon, S. In, N. Iovine, A. Ishihara, M. Jacquart, Matti Jansson, G. S. Japaridze, Krishnamoorthi Jayakumar, Minjin Jeong, Miaochen Jin, B. J. P. Jones, Donghwa Kang, Woosik Kang, X. Kang, A. Kappes, David Kappesser, Leonora Kardum, T. Karg, Martina Karl, A. Karle, U. Katz, M. Kauer, J. L. Kelley, A. Khatee Zathul, Ali Kheirandish, Ken'ichi Kin, J. Kiryluk, S. R. Klein, Alina Kochocki, Ramesh Koirala, H. Kolanoski, Tomas Kontrimas, L. Köpke, Claudio Kopper, D. J. Koskinen, Paras Koundal, Michael Kovacevich, M. Kowalski, Tetiana Kozynets, Karlijn Kruiswijk, Emmett Krupczak, Anil Kumar, Emma Kun, N. Kurahashi, N. N. Lad, Cristina Lagunas Gualda, M. Lamoureux, M. J. Larson, Frederik Hermann Lauber, Jeffrey Lazar, J. W. Lee, Kayla Leonard DeHolton, Agnieszka Leszczyńska, Massimiliano Lincetto, Qinrui Liu, Maria Liubarska, Elisa Lohfink, C. Love, L. Lu, Francesco Lucarelli, Andrew Ludwig, William Luszczak, Yang Lyu, W. Y., J. Madsen, K. B. M. Mahn, Yuya Makino, Sarah Mancina, W. Marie Sainte, Ioana Codrina Mariş, Szabolcs Márka, Z. Márka, M. Marsee, Ivan Martínez-Soler, R. Maruyama, Finn Mayhew, Thomas McElroy, Frank McNally, J. V. Mead, K. Meagher, Sarah Mechbal, Andrés Medina, Maximilian Meier, S. Meighen-Berger, Yarno Merckx, Lukas Merten, Jessie Micallef, D. Mockler, T. Montaruli, R. W. Moore, Y. Morii, R. Morse, Marjon Moulai, Tridib Mukherjee, Richard Naab, R. Nagai, M. Nakos, Uwe Naumann, Jannis Necker, M. Neumann, Hans Niederhausen, M. U. Nisa, A. Noell, Sarah Nowicki, A. Obertacke Pollmann, Vivian O'Dell, M. Oehler, Bob Oeyen, A. Olivas, R. Orsoe, John W. Osborn, Erin O’Sullivan, Hershal Pandya, N. Park, Grant Parker, Ek Narayan Paudel, L. Paul, C. Pérez de los Heros, Josh Peterson, Saskia Philippen, Sarah Pieper, A. Pizzuto, M. Plum, Yuriy Popovych, Maria Prado Rodriguez, B. Pries, R. Procter-Murphy, G. T. Przybylski, Christoph Raab, John Rack-Helleis, K. Rawlins, Zoë Rechav, Abdul Rehman, Patrick Reichherzer, Giovanni Renzi, E. Resconi, Simeon Reusch, W. Rhode, M. Richman, Benedikt Riedel, E. J. Roberts, S. Robertson, S. Rodan, Gerrit Roellinghoff, Martin Rongen, C. Rott, T. Ruhe, L. Ruohan, D. Ryckbosch, I. Safa, Julian Saffer, Daniel Salazar-Gallegos, P. Sampathkumar, S. E. Sanchez Herrera, Alexander Sandrock, M. Santander, Sourav Sarkar, S. Sarkar, J. Savelberg, Pierpaolo Savina, Merlin Schaufel, H. Schieler, S. Schindler, B. Schlüter, T. Schmidt, Judith Schneider, Frank Schröder, L. Schumacher, Georg Schwefer, S. Sclafani, D. Seckel, S. Seunarine, Ankur Sharma, S. Shefali, Nobuhiro Shimizu, M. Silva, Barbara Skrzypek, B. Smithers, R. Snihur, Jan Soedingrekso, A. Søgaard, Dennis Soldin, Giacomo Sommani, Christian Spannfellner, G. M. Spiczak, C. Spiering, M. Stamatikos, Todor Stanev, A. Stasik, Robert Stein, T. Stezelberger, T. Stürwald, Thomas Stuttard, G. W. Sullivan, I. Taboada, S. Ter–Antonyan, W. G. Thompson, Jessie Thwaites, S. Tilav, Kirsten Tollefson, Christoph Tönnis, S. Toscano, D. Tosi, Alexander Trettin, C. F. Tung, Roxanne Turcotte, Jean Pierre Twagirayezu, B. Ty, Martin Unland Elorrieta, A. K. Upadhyay, K. Upshaw, Nora Valtonen-Mattila, J. Vandenbroucke, N. van Eijndhoven, D. Vannerom, J. V. Santen, J. Vara, J. Veitch-Michaelis, M. Venugopal, Stef Verpoest, Doğa Veske, C. Walck, T. B. Watson, C. Weaver, Philip Weigel, A. Weindl, Jan Weldert, C. Wendt, Johannes Werthebach, Mark Weyrauch, N. Whitehorn, C. H. Wiebusch, N. Willey, D. R. Williams, Martin Wolf, Gerrit Wrede, Johan Wilfried Wulff, Xiaolin Xu, Emre Burak Yildizci, S. Yoshida, G. B. Yu, S. Yu, Tianlu Yuan, Z. Zhang, P. Zhelnin

Bibliographic record

VenueThe Astrophysical Journal Letters · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of AlbertaQueen's University
FundersOffice of Experimental Program to Stimulate Competitive ResearchDeutsches Elektronen-SynchrotronCollege of Engineering, Michigan State UniversityHelmholtz Alliance for Astroparticle PhysicsFonds Wetenschappelijk OnderzoekOffice of Advanced CyberinfrastructureDeutsche ForschungsgemeinschaftBelgian Federal Science Policy OfficeBundesministerium für Bildung und ForschungUniversity of Wisconsin-MadisonMarquette UniversityMichigan State UniversityOffice of Polar ProgramsFonds De La Recherche Scientifique - FNRSU.S. Department of EnergyNational Science Foundation
KeywordsSupernovaNeutrinoPhysicsAstrophysicsEnergy (signal processing)Neutrino astronomyAstronomyNeutrino detectorNuclear physicsNeutrino oscillation

Abstract

fetched live from OpenAlex

Abstract Core-collapse supernovae are a promising potential high-energy neutrino source class. We test for correlation between seven years of IceCube neutrino data and a catalog containing more than 1000 core-collapse supernovae of types IIn and IIP and a sample of stripped-envelope supernovae. We search both for neutrino emission from individual supernovae as well as for combined emission from the whole supernova sample, through a stacking analysis. No significant spatial or temporal correlation of neutrinos with the cataloged supernovae was found. All scenarios were tested against the background expectation and together yield an overall p -value of 93%; therefore, they show consistency with the background only. The derived upper limits on the total energy emitted in neutrinos are 1.7 × 10 48 erg for stripped-envelope supernovae, 2.8 × 10 48 erg for type IIP, and 1.3 × 10 49 erg for type IIn SNe, the latter disfavoring models with optimistic assumptions for neutrino production in interacting supernovae. We conclude that stripped-envelope supernovae and supernovae of type IIn do not contribute more than 14.6% and 33.9%, respectively, to the diffuse neutrino flux in the energy range of about [ 10 3 –10 5 ] GeV, assuming that the neutrino energy spectrum follows a power-law with an index of −2.5. Under the same assumption, we can only constrain the contribution of type IIP SNe to no more than 59.9%. Thus, core-collapse supernovae of types IIn and stripped-envelope supernovae can both be ruled out as the dominant source of the diffuse neutrino flux under the given assumptions.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.742
Threshold uncertainty score0.737

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.009
GPT teacher head0.201
Teacher spread0.192 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designBench or experimental
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations30
Published2023
Admission routes1
Has abstractyes

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