Record W4414451607 · doi:10.22323/1.501.0486

Prospective Sensitity to WIMP Dark Matter with the IceCube Upgrade

2025· article· en· W4414451607 on OpenAlexfundno aff

Eliot Genton, Jeffrey Lazar, G. de Wasseige, C. Argüelles, Rasha Abbasi, Markus Ackermann, Jenni Adams, Sanjib Kumar Agarwalla, Juanan Aguilar, M. Ahlers, Jean-Marco Alameddine, Shoukat Ali, Najia Moureen Binte Amin, K. Andeen, Yosuke Ashida, Sofia Athanasiadou, Spencer Axani, Rishi Babu, X. Bai, Joe Baines-Holmes, Aswathi Balagopal, Steven W. Barwick, Simeon Bash, Vedant Basu, Ryan Bay, J. J. Beatty, J. Becker Tjus, Jakob Beise, Chiara Bellenghi, Bruno Benkel, S. BenZvi, David Berley, E. Bernardini, D. Besson, E. Blaufuss, Lucas Bloom, Summer Blot, Ilya Bodo, Federico Bontempo, Caterina Boscolo Meneguolo, Sebastian BOSER, O. Botner, J. Böttcher, Jim Braun, Bennett Brinson, Zoe Brisson-Tsavoussis, Ryan T. Burley, Delaney Butterfield, Michael G. Campana, Kiara Carloni, Jose Carpio, J. Krishnamoorthi, Thien Nhan Chau, Zheyang Chen, D. Chirkin, Seowon Choi, Brian Clark, Alan Coleman, Peter John Cusack Coleman, Gabriel Collin, Diego Alberto Coloma Borja, A. Connolly, J. M. Conrad, Rebecca Corley, D. F. Cowen, C. De Clercq, James DeLaunay, Diyaselis Delgado, Thomas Delmeulle, Shuyang Deng, P. Desiati, Krijn de Vries, T. DeYoung, J. C. Díaz–Vélez, Stephen DiKerby, Markus Dittmer, Alba Domi, Lincoln Draper, Lasse Dueser, Daniel Durnford, Kaustav Dutta, M. A. DuVernois, Thomas Ehrhardt, Leonhard Eidenschink, Anna Eimer, P. Eller, Enrico Ellinger, Dominik Elsässer, Ralph Engel, Hannah Erpenbeck, Waleed Esmail, Steven Eulig, John Evans, P. A. Evenson, Kwok Lung Fan, Kareem Ramadan Farrag, A. R. Fazely, Anatoli Fedynitch, Nora Feigl, C. Finley, Leander Fischer, D. B. Fox, A. Franckowiak, Satoshi Fukami, Philipp Fürst, J. S. Gallagher, Erik Ganster, Alfonso García, Gaurav Garg, L. Gerhardt, Christian Gläser, T. Glüsenkamp, Javier González, Sreetama Goswami, Alejandra Granados, Darren Grant, Shannon Gray, Sean Griffin, Spencer Griswold, Kathrine Mørch Groth, David Joseph Guevel, Christoph Günther, Pascal Gutjahr, C. Ha, Christian Haack, Allan Hallgren, L. Halve, F. Halzen, Leon Hamacher, Martin Ha Minh, Michael Handt, Kael Hanson, John Hardin, Alexander Harnisch, Patrick Hatch, A. Haungs, Jonas Häußler, K. Helbing, Jonas Hellrung, B. L. Henke, Lukas Hennig, Felix Henningsen, Lars Philipp Heuermann, Russell J. Hewett, Nils Heyer, Stephanie Hickford, Attila Hidvégi, Colton Hill, G. C. Hill, Ramy Hmaid, Kara Hoffman, Dan Hooper, Sam Hori, Kotoyo Hoshina, Matheus Hostert, Wenjie Hou, Thomas Huber, K. Hultqvist, Karolin Hymon, A. Ishihara, W. Iwakiri, Marc Jacquart, Samyak Jain, Oliver Janik, Matti Jansson, Minjin Jeong, Miaochen Jin, N. Kamp, Donghwa Kang, Woosik Kang, Xinyue Kang, Alexander Kappes, Leonora Kardum, T. Karg, Martina Karl, Albrecht Karle, Akanksha Katil, M. Kauer, J. L. Kelley, Manish Khanal, Arifa Khatee Zathul, Ali Kheirandish, H. Kimku, Joanna Kiryluk, Carolin Klein, Yukiho Kobayashi, Alina Kochocki, Ramesh Koirala, H. Kolanoski, Tomas Kontrimas, L. Köpke, Claudio Kopper, Jason Koskinen, Paras Koundal, M. Kowalski, Tetiana Kozynets, Krishnamoorthi Jayakumar, Tanvi Krishnan, Karlijn Kruiswijk, Emmett Krupczak, Anil Kumar, Emma Kun, N. Kurahashi, Neha Navnitkumar Lad, Cristina Lagunas Gualda, M. Lamoureux, M. J. Larson, Frederik Hermann Lauber, Kayla Leonard DeHolton, Agnieszka Leszczyńska, Jiyuan Liao, C. Lin, Yitong Liu, Maria Liubarska, Christy Love, L. Lu, Francesco Lucarelli, William Luszczak, Yang Lyu, Jim Madsen, Else Magnus, Kendall Mahn, Yuya Makino, Elena Manao, Sarah Mancina, Alicia Mand, Ioana Codrina Maris, Szabolcs Márka, Zsuzsa Márka, Lars Marten, Ivan Martínez-Soler, R. Maruyama, Jonathan Mauro, Finn Mayhew, Frank McNally, J. V. Mead, K. Meagher, Sarah Mechbal, Andrés Medina, Maximilian Meier, Yarno Merckx, Lukas Merten, Justin Mitchell, Logan Molchany, T. Montaruli, R. W. Moore, Yasutsugu Morii, Anke Mosbrugger, Marjon Moulai, Despina Mousadi, Emile Moyaux, Tista Mukherjee, Richard Naab, Maxwell Nakos, Uwe Naumann, Jannis Necker, Ludwig Neste, Miriam Neumann, Hans Niederhausen, M. U. Nisa, K. Noda, Andreas Noell, Alexander Novikov, A. Obertacke Pollmann, Vivian O'Dell, Alex Olivas, Jesse Osborn, Erin O’Sullivan, Veronika Palušová, Hershal Pandya, A. Parenti, Nahee Park, V. A. Parrish, Ek Narayan Paudel, Larissa Paul, C. Pérez de los Heros, Teresa Pernice, Josh F. Peterson, M. Plum, Axel Ponten, Vaidehi Poojyam, Yuriy Popovych, Maria Prado Rodriguez, B. Pries, Rachel Procter-Murphy, G. T. Przybylski, Lilly Pyras, Christoph Raab, John Rack-Helleis, N. Rad, Martin Langgård Ravn, Katherine Rawlins, Zoë Rechav, Abdul Rehman, Ian Reistroffer, Elisa Resconi, Simeon Reusch, Chang Dong Rho, W. Rhode, Leonardo Ricca, Benedikt Riedel, Adam Rifaie, Ella Roberts, Sally Robertson, Martin Rongen, Aske Rosted, C. Rott, T. Ruhe, Li Ruohan, Dirk Ryckbosch, Julian Saffer, Daniel Salazar-Gallegos, Pranav Sampathkumar, Alexander Sandrock, Grace Sanger-Johnson, Marcos Santander, Subir Sarkar, Joelle Savelberg, Marco Scarnera, Patrick Schaile, Merlin Schaufel, H. Schieler, Sebastian Schindler, Lea Schlickmann, Berit Schlüter, Felix Schlüter, Nick Schmeisser, Torsten Schmidt, Frank Schröder, L. Schumacher, Sonke Schwirn, S. Sclafani, D. Seckel, Leo Seen, Mohammad Ful Hossain Seikh, S. Seunarine, Per Arne Sevle Myhr, Riya Shah, Shefali Shefali, Nobuhiro Shimizu, Barbara Skrzypek, Robert Snihur, Jan Soedingrekso, A. Søgaard, Dennis Soldin, Philipp Soldin, Giacomo Sommani, Christian Spannfellner, G. M. Spiczak, Christian Spiering, Juliana Stachurska, M. Stamatikos, Todor Stanev, T. Stezelberger, Timo Stürwald, Thomas Stuttard, G. W. Sullivan, I. Taboada, S. Ter–Antonyan, Andrii Terliuk, Amar Thakuri, Matthias Thiesmeyer, Will Thompson, Jessie Thwaites, Serap Tilav, Kirsten Tollefson, Simona Toscano, Delia Tosi, Alexandra Trettin, Anuj Kumar Upadhyay, Karriem Upshaw, Arun Vaidyanathan, Nora Valtonen-Mattila, Janeth Valverde, J. Vandenbroucke, Thijs van Eeden, N. van Eijndhoven, Lene van Rootselaar, J. V. Santen, Félix Carbonell, Fahim Varsi, Megha Venugopal, Matthias Vereecken, Sebastian Vergara Carrasco, Stef Verpoest, Doğa Veske, Aishwarya Vijai, Joshua Villarreal, C. Walck, Andrew Wang, Elizabeth Warrick, Chris Weaver, Philip Weigel, Andreas Weindl, Jan Weldert, Alex Wen, Chris Wendt, Johannes Werthebach, Mark Weyrauch, N. Whitehorn, C. H. Wiebusch, Dawn Williams, Lucas Witthaus, Martin Wolf, Gerrit Wrede, Xianwu Xu, Juan Pablo Yáñez, Yuhua Yao, Emre Burak Yildizci, S. Yoshida, Robert Young, G. B. Yu, Shiqi Yu, Angela Zegarelli, Shuo Zhang, Zelong Zhang, Pavel Zhelnin, Perri Zilberman

Bibliographic record

Venuenot available

Typearticle

Languageen

FieldPhysics and Astronomy

TopicDark Matter and Cosmic Phenomena

Canadian institutionsnot available

FundersOffice of Experimental Program to Stimulate Competitive ResearchMarsden FundJapan Society for the Promotion of ScienceDeutsches Elektronen-SynchrotronNatural Sciences and Engineering Research Council of CanadaOffice of Polar ProgramsCollege of Engineering, Michigan State UniversityChiba UniversityAlliance de recherche numérique du CanadaHelmholtz Alliance for Astroparticle PhysicsInstitute for Global Prominent Research, Chiba UniversityRWTH Aachen UniversityKnut och Alice Wallenbergs StiftelseVillum FondenNational Research Foundation of KoreaSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungNational Science FoundationBelgian Federal Science Policy OfficeDeutsche ForschungsgemeinschaftMichigan State UniversityNational Research FoundationUniversity of Wisconsin-MadisonVetenskapsrådetU.S. Department of EnergyOffice of Advanced CyberinfrastructureEuropean CommissionWestern Canada Research GridFonds De La Recherche Scientifique - FNRSPolarforskningssekretariatetFonds Wetenschappelijk OnderzoekNvidiaMarquette University

KeywordsWIMPNeutrinoDark matterWeakly interacting massive particlesSensitivity (control systems)Range (aeronautics)Light dark matterMassive particle

DOI10.22323/1.501.0486

Abstract

fetched live from OpenAlex

While astrophysical observations imply that 85% of the matter content is unaccounted for, the nature of this dark matter (DM) component remains unknown. Weakly Interacting Massive Particles (WIMPs)—DM particles that interact at or below the weak interaction scale—could naturally explain this missing matter. These interactions with the Standard Model (SM) allow them to be gravitationally captured in celestial bodies like the Sun. Trapped DM in the solar core could subsequently annihilate, producing stable SM particles, of which only neutrinos can escape the Sun’s dense interior. Therefore, an excess of neutrinos originating from the direction of the Sun would serve as evidence of DM. The IceCube Upgrade, a dense infill of the IceCube Neutrino Observatory, will lower the energy threshold and improve sensitivity in the range from 1 to 500 GeV, thereby enhancing IceCube’s ability to detect GeV-scale DM. In this contribution, I present projections of the IceCube Upgrade’s sensitivity to the DM-proton scattering cross section for DM masses between 3 GeV and 500 GeV. These sensitivities position IceCube as the most sensitive indirect detection experiment for DM in the mass range from 3 GeV to 10 TeV.

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 machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.002

metaresearch head score (Gemma)0.004

Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated

Candidate categoriesnone

Consensus categoriesnone

DomainCandidate signal: none · Consensus signal: none

Study designCandidate signal: Simulation or modeling · Consensus signal: none

GenreCandidate signal: Empirical · Consensus signal: Empirical

Teacher disagreement score0.005

Threshold uncertainty score0.013

Distilled classifier scores by category (both heads)

Category	Codex	Gemma
Metaresearch	0.002	0.004
Meta-epidemiology (narrow)	0.001	0.000
Meta-epidemiology (broad)	0.000	0.000
Bibliometrics	0.001	0.001
Science and technology studies	0.000	0.001
Scholarly communication	0.002	0.001
Open science	0.001	0.002
Research integrity	0.001	0.001
Insufficient payload (model declined to judge)	0.004	0.001

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 head0.003

GPT teacher head0.210

Teacher spread0.207 · 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 source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.

Study designSimulation or modeling

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".

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Citations0

Published2025

Admission routes1

Has abstractyes

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