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@ARTICLE{Abbasi:596782,
author = {Abbasi, R. and Ackermann, M. and Adams, J. and Aggarwal, N.
and Aguilar, J. A. and Ahlers, 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. N. and Bai, X. and
Balagopal, V. A. and Baricevic, M. and Barwick, S. W. and
Basu, V. and Bay, R. and Beatty, J. J. and Becker, K.-H. and
Becker Tjus, J. and Beise, J. and Bellenghi, C. 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 Meneguolo,
C. Boscolo and Böser, S. and Botner, O. and Böttcher, J.
and Bourbeau, E. and Braun, J. and Brinson, B. 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, S. and Clark, B. A. and
Classen, L. and Coleman, A. and Collin, G. H. and Connolly,
A. and Conrad, J. M. and Coppin, P. and Correa, P. and
Countryman, S. and Cowen, D. F. and Dappen, C. and Dave, P.
and De Clercq, C. and DeLaunay, J. J. and Delgado López, D.
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, L. 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 Gray, S. J. and Grégoire, T. and Griffin, S.
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
Heuermann, L. and Hickford, S. and Hidvegi, A. and Hill, C.
and Hill, G. C. and Hoffman, K. D. and Hoshina, K. and Hou,
W. 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 Koskinen, D. J. and Koundal, P. and
Kovacevich, M. and Kowalski, M. and Kozynets, T. and
Kruiswijk, K. and Krupczak, E. and Kumar, A. and Kun, E. and
Kurahashi, N. and Lad, N. and Lagunas Gualda, C. and
Lamoureux, M. and Larson, M. J. and Lauber, F. and Lazar, J.
P. and Lee, J. W. and Leonard DeHolton, K. and Leszczyńska,
A. and Lincetto, M. and Liu, Q. R. and Liubarska, M. and
Lohfink, E. and Love, C. and Lozano Mariscal, C. J. 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 Marka, S. and Marka, Z. and Marsee, M. and
Martinez-Soler, I. and Maruyama, R. and Mayhew, F. 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 Merten, L. and
Micallef, J. and Mockler, D. and Montaruli, T. and Moore, R.
W. and Morii, Y. and Morse, R. and Moulai, M. and Mukherjee,
T. and Naab, R. and Nagai, R. and Naumann, U. and Nayerhoda,
A. and Necker, J. and Neumann, M. and Niederhausen, H. and
Nisa, M. U. and Noell, A. and Nowicki, S. C. and Pollmann,
A. Obertacke and Oehler, M. and Oeyen, B. and Olivas, A. and
Orsoe, R. 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
Peterson, J. and Philippen, S. and Pieper, S. and Pizzuto,
A. and Plum, M. and Popovych, Y. and Rodriguez, M. Prado and
Pries, B. and Procter-Murphy, R. and Przybylski, G. T. and
Raab, C. and Rack-Helleis, J. and Rawlins, K. 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 Rodan,
S. and Roellinghoff, G. and Rongen, M. and Rott, C. and
Ruhe, T. and Ruohan, L. and Ryckbosch, D. and Rysewyk Cantu,
D. and Athanasiadou, S. 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 Savelberg, J. and Savina, P. and
Schaufel, M. and Schieler, H. and Schindler, S. and
Schlüter, B. and Schmidt, T. 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
Søgaard, A. and Soldin, D. and Spannfellner, C. and
Spiczak, G. M. and Spiering, C. and Stamatikos, M. and
Stanev, T. and Stein, R. 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 Tung, C. F. 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 van Santen, J. and Vara, J. and Veitch-Michaelis, J. and
Verpoest, S. and Veske, D. and Walck, C. 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. and Zhelnin, P.},
collaboration = {{IceCube Collaboration}},
title = {{S}earch for sub-{T}e{V} {N}eutrino {E}mission from {N}ovae
with {I}ce{C}ube-{D}eep{C}ore},
journal = {The astrophysical journal / Part 1},
volume = {953},
number = {2},
issn = {0004-637X},
address = {London},
publisher = {Institute of Physics Publ.},
reportid = {PUBDB-2023-06273, arXiv:2212.06810},
pages = {160},
year = {2023},
note = {Published in ApJ. 21 pages, 11 figures},
abstract = {The understanding of novae, the thermonuclear eruptions on
the surfaces of white dwarf stars in binaries, has recently
undergone a major paradigm shift. Though the bolometric
luminosity of novae was long thought to arise directly from
photons supplied by the thermonuclear runaway, recent
gigaelectronvolt (GeV) gamma-ray observations have supported
the notion that a significant portion of the luminosity
could come from radiative shocks. More recently,
observations of novae have lent evidence that these shocks
are acceleration sites for hadrons for at least some types
of novae. In this scenario, a flux of neutrinos may
accompany the observed gamma rays. As the gamma rays from
most novae have only been observed up to a few GeV, novae
have previously not been considered as targets for neutrino
telescopes, which are most sensitive at and above
teraelectronvolt (TeV) energies. Here, we present the first
search for neutrinos from novae with energies between a few
GeV and 10 TeV using IceCube-DeepCore, a densely
instrumented region of the IceCube Neutrino Observatory with
a reduced energy threshold. We search both for a correlation
between gamma-ray and neutrino emission as well as between
optical and neutrino emission from novae. We find no
evidence for neutrino emission from the novae considered in
this analysis and set upper limits for all gamma-ray
detected novae.},
keywords = {energy: threshold (INSPIRE) / neutrino: flux (INSPIRE) /
white dwarf: surface (INSPIRE) / neutrino: detector
(INSPIRE) / gamma ray (INSPIRE) / GeV (INSPIRE) / TeV
(INSPIRE) / acceleration (INSPIRE) / binary (INSPIRE) /
observatory (INSPIRE) / star (INSPIRE) / site (INSPIRE) /
optical (INSPIRE) / bolometer (INSPIRE) / correlation
(INSPIRE) / IceCube (INSPIRE) / nucleus (INSPIRE) / hadron
(INSPIRE)},
cin = {ZEU-ICE},
ddc = {520},
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 = {2212.06810},
howpublished = {arXiv:2212.06810},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2212.06810;\%\%$},
UT = {WOS:001053469100001},
doi = {10.3847/1538-4357/acdc1b},
url = {https://bib-pubdb1.desy.de/record/596782},
}
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