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@ARTICLE{Abbasi:491467,
author = {Abbasi, R. and Ackermann, M. and Adams, J. and Aguilar, J.
A. and Ahlers, M. and Ahrens, M. and Alameddine, J. M. and
Alves, Jr. A. A. and Amin, N. M. and Andeen, K. and
Anderson, T. and Anton, G. and Argüelles, C. and Ashida, Y.
and Athanasiadou, Sofia and Axani, S. and Bai, X. and
Balagopal, V. A. and Baricevic, M. and Barwick, S. W. and
Basu, V. and Baur, S. and Bay, R. and Beatty, J. J. and
Becker, K.-H. and Becker Tjus, J. and Beise, J. and
Bellenghi, C. and Benda, S. and BenZvi, S. and Berley, D.
and Bernardini, E. and Besson, D. Z. and Binder, G. and
Bindig, D. and Blaufuss, E. and Blot, Summer and Bontempo,
F. and Book, J. Y. and Borowka, J. and Böser, S. and
Botner, O. and Böttcher, J. and Bourbeau, E. and Bradascio,
Federica and Braun, J. and Brinson, B. and Bron, S. and
Brostean-Kaiser, Jannes and Burley, R. T. and Busse, R. S.
and Campana, M. A. and Carnie-Bronca, E. G. and Chen, C. and
Chen, Z. and Chirkin, D. and Choi, K. and Clark, B. A. and
Clark, K. and Classen, L. and Coleman, A. and Collin, G. H.
and Connolly, A. and Conrad, J. M. and Coppin, P. and
Correa, P. and Cowen, D. F. and Cross, R. and Dappen, C. and
Dave, P. and De Clercq, C. and DeLaunay, J. J. and López,
D. Delgado and Dembinski, H. and Deoskar, K. and Desai, A.
and Desiati, P. and de Vries, K. D. and de Wasseige, G. and
DeYoung, T. and Diaz, A. and Díaz-Vélez, J. C. and
Dittmer, M. and Dujmovic, H. and DuVernois, M. A. and
Ehrhardt, T. and Eller, P. and Engel, R. and Erpenbeck, H.
and Evans, J. and Evenson, P. A. and Fan, K. L. and Fazely,
A. R. and Fedynitch, A. and Feigl, N. and Fiedlschuster, S.
and Fienberg, A. T. and Finley, C. and Fischer, Leander and
Fox, D. and Franckowiak, A. and Friedman, E. and Fritz, A.
and Fürst, P. and Gaisser, T. K. and Gallagher, J. and
Ganster, E. and Garcia, A. and Garrappa, Simone and
Gerhardt, L. and Ghadimi, A. and Glaser, C. and Glauch, T.
and Glüsenkamp, T. and Goehlke, N. and Gonzalez, J. G. and
Goswami, S. and Grant, D. and Grégoire, T. and Griswold, S.
and Günther, C. and Gutjahr, P. and Haack, C. and Hallgren,
A. and Halliday, R. and Halve, L. and Halzen, F. and
Hamdaoui, H. and Ha Minh, M. and Hanson, K. and Hardin, J.
and Harnisch, A. A. and Haungs, A. and Helbing, K. and
Hellrung, J. and Henningsen, F. and Hettinger, E. C. and
Heuermann, L. and Hickford, S. and Hignight, J. and Hill, C.
and Hill, G. C. and Hoffman, K. D. and Hoshina, K. and Hou,
W. and Huber, M. and Huber, T. and Hultqvist, K. and
Hünnefeld, M. and Hussain, R. and Hymon, K. and In, S. and
Iovine, N. and Ishihara, A. and Jansson, M. and Japaridze,
G. S. and Jeong, M. and Jin, M. and Jones, B. J. P. and
Kang, D. and Kang, W. and Kang, X. and Kappes, A. and
Kappesser, D. and Kardum, L. and Karg, T. and Karl, M. and
Karle, A. and Katz, U. and Kauer, M. and Kelley, J. L. and
Kheirandish, A. and Kin, K. and Kiryluk, J. and Klein, S. R.
and Kochocki, A. and Koirala, R. and Kolanoski, H. and
Kontrimas, T. and Köpke, L. and Kopper, C. and Kopper, S.
and Koskinen, D. J. and Koundal, P. and Kovacevich, M. and
Kowalski, Marek and Kozynets, T. and Krupczak, E. and Kun,
E. and Kurahashi, N. and Lad, Neha Navnitkumar and Gualda,
C. Lagunas and Larson, M. J. and Lauber, F. and Lazar, J. P.
and Lee, J. W. and Leonard, K. and Leszczyńska, A. and
Lincetto, M. and Liu, Q. R. and Liubarska, M. and Lohfink,
E. and Mariscal, C. J. Lozano and Lu, L. and Lucarelli, F.
and Ludwig, A. and Luszczak, W. and Lyu, Y. and Ma, Wing Yan
and Madsen, J. and Mahn, K. B. M. and Makino, Y. and
Mancina, S. and Sainte, W. Marie and Mariş, I. C. and
Martinez-Soler, I. and Maruyama, R. and McCarthy, S. and
McElroy, T. and McNally, F. and Mead, J. V. and Meagher, K.
and Mechbal, Sarah and Medina, A. and Meier, M. and
Meighen-Berger, S. and Merckx, Y. and Micallef, J. and
Mockler, D. and Montaruli, T. and Moore, R. W. and Morse, R.
and Mukherjee, T. and Naab, Richard and Nagai, R. and
Naumann, U. and Necker, Jannis David and Nguyễn, L. V. and
Niederhausen, H. and Nisa, M. U. and Nowicki, S. C. and
Pollmann, A. Obertacke and Oehler, M. and Oeyen, B. and
Olivas, A. and Osborn, J. and O'Sullivan, E. and Pandya, H.
and Pankova, D. V. and Park, N. and Parker, G. K. and
Paudel, E. N. and Paul, L. and de los Heros, C. Pérez and
Peters, L. and Peterson, J. and Philippen, S. and Pieper, S.
and Pizzuto, A. and Plum, M. and Popovych, Y. and Porcelli,
A. and Rodriguez, M. Prado and Pries, B. and Przybylski, G.
T. and Raab, C. and Rack-Helleis, J. and Raissi, A. and
Rameez, M. and Rawlins, K. and Rea, I. C. and Rechav, Z. and
Rehman, A. and Reichherzer, P. and Renzi, G. and Resconi, E.
and Reusch, Simeon and Rhode, W. and Richman, M. and Riedel,
B. and Roberts, E. J. and Robertson, S. and Roellinghoff, G.
and Rongen, M. and Rott, C. and Ruhe, T. and Ryckbosch, D.
and Cantu, D. Rysewyk and Safa, I. and Saffer, J. and
Salazar-Gallegos, D. and Sampathkumar, P. and Herrera, S. E.
Sanchez and Sandrock, A. and Santander, M. and Sarkar, S.
and Sarkar, S. and Satalecka, K. and Schaufel, M. and
Schieler, H. and Schindler, S. and Schmidt, T. and
Schneider, A. and Schneider, J. and Schröder, F. G. and
Schumacher, L. and Schwefer, G. and Sclafani, S. and Seckel,
D. and Seunarine, S. and Sharma, A. and Shefali, S. and
Shimizu, N. and Silva, M. and Skrzypek, B. and Smithers, B.
and Snihur, R. and Soedingrekso, J. and Sogaard, A. and
Soldin, D. and Spannfellner, C. and Spiczak, G. M. and
Spiering, C. and Stamatikos, M. and Stanev, T. and Stein,
Robert and Stettner, J. and Stezelberger, T. and Stürwald,
T. and Stuttard, T. and Sullivan, G. W. and Taboada, I. and
Ter-Antonyan, S. and Thwaites, J. and Tilav, S. and
Tollefson, K. and Tönnis, C. and Toscano, S. and Tosi, D.
and Trettin, Alexander and Tselengidou, M. and Tung, C. F.
and Turcati, A. and Turcotte, R. and Twagirayezu, J. P. and
Ty, B. and Unland Elorrieta, M. A. and Upshaw, K. and
Valtonen-Mattila, N. and Vandenbroucke, J. and van
Eijndhoven, N. and Vannerom, D. and Santen, Jakob van and
Veitch-Michaelis, J. and Verpoest, S. and Walck, C. and
Wang, W. and Watson, T. B. and Weaver, C. and Weigel, P. and
Weindl, A. and Weldert, J. and Wendt, C. and Werthebach, J.
and Weyrauch, M. and Whitehorn, N. and Wiebusch, C. H. and
Willey, N. and Williams, D. R. and Wolf, M. and Wrede, G.
and Wulff, J. and Xu, X. W. and Yanez, J. P. and Yildizci,
E. and Yoshida, S. and Yu, S. and Yuan, T. and Zhang, Z.},
collaboration = {{IceCube Collaboration}},
title = {{S}earches for {C}onnections between {D}ark {M}atter and
{H}igh-{E}nergy {N}eutrinos with {I}ce{C}ube},
reportid = {PUBDB-2023-00176, arXiv:2205.12950},
year = {2022},
note = {28 pages, 8 figures},
abstract = {In this work, we present the results of searches for
signatures of dark matter decay or annihilation into
Standard Model particles, and secret neutrino interactions
with dark matter. Neutrinos could be produced in the decay
or annihilation of galactic or extragalactic dark matter.
Additionally, if an interaction between dark matter and
neutrinos exists then dark matter will interact with
extragalactic neutrinos. In particular galactic dark matter
will induce an anisotropy in the neutrino sky if this
interaction is present. We use seven and a half years of the
High-Energy Starting Event (HESE) sample data, which
measures neutrinos in the energy range of approximately 60
TeV to 10 PeV, to study these phenomena. This all-sky event
selection is dominated by extragalactic neutrinos. For dark
matter of $\sim$ 1 PeV in mass, we constrain the
velocity-averaged annihilation cross section to be smaller
than $10^{-23}$cm$^3$/s for the exclusive $\mu^+\mu^-$
channel and $10^{-22}$ cm$^3$/s for the $b\bar b$ channel.
For the same mass, we constrain the lifetime of dark matter
to be larger than $10^{28}$ s for all channels studied,
except for decaying exclusively to $b\bar b$ where it is
bounded to be larger than $10^{27}$ s. Finally, we also
search for evidence of astrophysical neutrinos scattering on
galactic dark matter in two scenarios. For fermionic dark
matter with a vector mediator, we constrain the
dimensionless coupling associated with this interaction to
be less than 0.1 for dark matter mass of 0.1 GeV and a
mediator mass of $10^{-4}~$ GeV. In the case of scalar dark
matter with a fermionic mediator, we constrain the coupling
to be less than 0.1 for dark matter and mediator masses
below 1 MeV.},
keywords = {dark matter: leptonic decay (INSPIRE) / muon: pair
production (INSPIRE) / bottom: pair production (INSPIRE) /
dark matter: annihilation (INSPIRE) / neutrino: cosmic
radiation (INSPIRE) / galaxy: dark matter (INSPIRE) / dark
matter: signature (INSPIRE) / dark matter: scalar (INSPIRE)
/ fermion: dark matter (INSPIRE) / dark matter: lifetime
(INSPIRE) / neutrino: interaction (INSPIRE) / dark matter:
mass (INSPIRE) / dark matter: decay (INSPIRE) / cross
section: annihilation (INSPIRE) / neutrino: scattering
(INSPIRE) / mediation (INSPIRE) / IceCube (INSPIRE) /
anisotropy (INSPIRE) / coupling constant: upper limit
(INSPIRE) / experimental results (INSPIRE)},
cin = {ZEU-ICE},
cid = {I:(DE-H253)ZEU-ICE-20160806},
pnm = {613 - Matter and Radiation from the Universe (POF4-613)},
pid = {G:(DE-HGF)POF4-613},
experiment = {EXP:(DE-H253)IceCube-20150101},
typ = {PUB:(DE-HGF)25},
eprint = {2205.12950},
howpublished = {arXiv:2205.12950},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2205.12950;\%\%$},
doi = {10.3204/PUBDB-2023-00176},
url = {https://bib-pubdb1.desy.de/record/491467},
}
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