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@ARTICLE{Abbasi:601416,
author = {Abbasi, R. and Ackermann, Markus 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, S. 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, S. and Bontempo, F. and Book, J. Y. and Borowka,
J. and Böser, S. and Botner, O. and Böttcher, J. and
Bourbeau, E. and Bradascio, F. and Braun, J. and Brinson, B.
and Bron, S. and Brostean-Kaiser, J. 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, S. 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 Hatch, P. 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, N. 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, W. Y. 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, S. 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 Moulai, M. and Mukherjee, T. and Naab, R. and Nagai, R.
and Naumann, U. and Necker, J. 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, S. 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 Thompson, W. G. and Thwaites, J. and
Tilav, S. and Tollefson, K. and Tönnis, C. and Toscano, S.
and Tosi, D. and Trettin, A. 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 Unland
Elorrieta, M. and Upshaw, K. and Valtonen-Mattila, N. and
Vandenbroucke, J. and van Eijndhoven, N. and Vannerom, D.
and van Santen, J. 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 R.,
D. 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. and Zhelnin, P.},
collaboration = {{IceCube Collaboration}},
title = {{S}earches for connections between dark matter and
high-energy neutrinos with {I}ce{C}ube},
journal = {Journal of cosmology and astroparticle physics},
volume = {10},
number = {10},
issn = {1475-7508},
address = {London},
publisher = {IOP},
reportid = {PUBDB-2024-00170, arXiv:2205.12950},
pages = {003},
year = {2023},
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 ∼ 1 PeV in mass, we constrain the
velocity-averaged annihilation cross section to be smaller
than 10$^{-23}$ cm$^{3}$/s for the exclusive
μ$^{+}$μ$^{-}$ channel and 10$^{-22}$ cm$^{3}$/s for the
bb̅ 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 bb̅ 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) / dark matter
experiments (autogen) / neutrino astronomy (autogen) /
neutrino experiments (autogen) / ultra high energy photons
and neutrinos (autogen)},
cin = {ZEU-ICE},
ddc = {530},
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)16},
eprint = {2205.12950},
howpublished = {arXiv:2205.12950},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2205.12950;\%\%$},
UT = {WOS:001118673400009},
doi = {10.1088/1475-7516/2023/10/003},
url = {https://bib-pubdb1.desy.de/record/601416},
}
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