@misc{snowglobes,
	Author = {{SNOwGLoBES contributors}},
	Date-Added = {2020-05-22 22:43:03 +0200},
	Date-Modified = {2020-05-22 22:50:31 +0200},
	Journal = {GitHub repository},
	Publisher = {GitHub},
	Title = {SNOwGLoBES code: SuperNova Observatories with GLoBES},
	Url = {https://github.com/SNOwGLoBES/snowglobes},
	Year = {2020}}

@article{Askins2020,
	Abstract = {New developments in liquid scintillators, high-efficiency, fast photon detectors, and chromatic photon sorting have opened up the possibility for building a large-scale detector that can discriminate between Cherenkov and scintillation signals. Such a detector could reconstruct particle direction and species using Cherenkov light while also having the excellent energy resolution and low threshold of a scintillator detector. Situated deep underground, and utilizing new techniques in computing and reconstruction, this detector could achieve unprecedented levels of background rejection, enabling a rich physics program spanning topics in nuclear, high-energy, and astrophysics, and across a dynamic range from hundreds of keV to many GeV. The scientific program would include observations of low- and high-energy solar neutrinos, determination of neutrino mass ordering and measurement of the neutrino CP-violating phase {\$}{\$}{$\backslash$}delta {\$}{\$}δ, observations of diffuse supernova neutrinos and neutrinos from a supernova burst, sensitive searches for nucleon decay and, ultimately, a search for neutrinoless double beta decay, with sensitivity reaching the normal ordering regime of neutrino mass phase space. This paper describes Theia, a detector design that incorporates these new technologies in a practical and affordable way to accomplish the science goals described above.},
	Author = {Askins, M. and Bagdasarian, Z. and Barros, N. and Beier, E. W. and Blucher, E. and Bonventre, R. and Bourret, E. and Callaghan, E. J. and Caravaca, J. and Diwan, M. and Dye, S. T. and Eisch, J. and Elagin, A. and Enqvist, T. and Fischer, V. and Frankiewicz, K. and Grant, C. and Guffanti, D. and Hagner, C. and Hallin, A. and Jackson, C. M. and Jiang, R. and Kaptanoglu, T. and Klein, J. R. and Kolomensky, Yu. G. and Kraus, C. and Krennrich, F. and Kutter, T. and Lachenmaier, T. and Land, B. and Lande, K. and Learned, J. G. and Lozza, V. and Ludhova, L. and Malek, M. and Manecki, S. and Maneira, J. and Maricic, J. and Martyn, J. and Mastbaum, A. and Mauger, C. and Moretti, F. and Napolitano, J. and Naranjo, B. and Nieslony, M. and Oberauer, L. and Orebi Gann, G. D. and Ouellet, J. and Pershing, T. and Petcov, S. T. and Pickard, L. and Rosero, R. and Sanchez, M. C. and Sawatzki, J. and Seo, S. H. and Smiley, M. and Smy, M. and Stahl, A. and Steiger, H. and Stock, M. R. and Sunej, H. and Svoboda, R. and Tiras, E. and Trzaska, W. H. and Tzanov, M. and Vagins, M. and Vilela, C. and Wang, Z. and Wang, J. and Wetstein, M. and Wilking, M. J. and Winslow, L. and Wittich, P. and Wonsak, B. and Worcester, E. and Wurm, M. and Yang, G. and Yeh, M. and Zimmerman, E. D. and Zsoldos, S. and Zuber, K.},
	Date-Added = {2020-05-22 22:06:05 +0200},
	Date-Modified = {2020-05-22 22:26:19 +0200},
	Doi = {10.1140/epjc/s10052-020-7977-8},
	Isbn = {1434-6052},
	Journal = {The European Physical Journal C},
	Number = {5},
	Pages = {416},
	Title = {{THEIA: An advanced optical neutrino detector}},
	Url = {https://doi.org/10.1140/epjc/s10052-020-7977-8},
	Volume = {80},
	Year = {2020}}

@article{Armbruster1998,
	Author = {Armbruster, B and others},
	Collaboration = {KARMEN},
	Date-Added = {2020-04-22 15:48:53 +0200},
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	Doi = {10.1016/S0370-2693(98)00087-2},
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@article{Donnelly1979,
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	Date-Added = {2020-04-22 15:04:17 +0200},
	Date-Modified = {2020-04-22 15:04:18 +0200},
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@article{Askins2015,
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	Date-Added = {2020-04-22 14:30:01 +0200},
	Date-Modified = {2020-05-26 14:06:31 +0200},
	Eprint = {1502.01132},
	Month = {2},
	Note = {\href{https://arxiv.org/abs/1502.01132}{\texttt{arXiv:1502.01132}}},
	Primaryclass = {physics.ins-det},
	Title = {{The Physics and Nuclear Nonproliferation Goals of WATCHMAN: A WAter CHerenkov Monitor for ANtineutrinos}},
	Year = {2015}}

@article{Kolbe2002,
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	Date-Added = {2020-04-22 14:06:37 +0200},
	Date-Modified = {2020-04-22 14:06:37 +0200},
	Doi = {10.1103/PhysRevD.66.013007},
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	Date-Added = {2020-04-22 13:47:50 +0200},
	Date-Modified = {2020-04-22 13:59:54 +0200},
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	Date-Added = {2020-04-22 13:47:44 +0200},
	Date-Modified = {2020-04-22 13:59:54 +0200},
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	Date-Added = {2020-04-22 13:47:29 +0200},
	Date-Modified = {2020-04-22 13:59:54 +0200},
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@article{Dighe2003,
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	Date-Added = {2020-04-22 13:47:19 +0200},
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	Title = {{Suppression of the multi-azimuthal-angle instability in dense neutrino gas during supernova accretion phase}},
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@article{Chakraborty2016,
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	Journal = {Nucl. Phys.},
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	Primaryclass = {hep-ph},
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	Title = {{Collective neutrino flavor conversion: Recent developments}},
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	Year = {2016}}

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	Primaryclass = {hep-ph},
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	Title = {{Self-induced spectral splits in supernova neutrino fluxes}},
	Volume = {D76},
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@article{Dasgupta2009,
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	Title = {{Multiple Spectral Splits of Supernova Neutrinos}},
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	Title = {{Fast Pairwise Conversion of Supernova Neutrinos: A Dispersion-Relation Approach}},
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	Year = {2017}}

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	Pages = {035502},
	Primaryclass = {hep-ph},
	Slaccitation = {%%CITATION = HEP-PH/0211306;%%},
	Title = {{Radiative corrections to low-energy neutrino reactions}},
	Volume = {C67},
	Year = {2003}}

@article{Strumia2003,
	Abstract = {Quasielastic antineutrino/proton and neutrino/neutron scatterings can be well approximated by simple formulae, valid around MeV or GeV energies. We obtain a single expression valid in the whole range, and discuss its relevance for studies of supernova neutrinos, which reach intermediate energies.},
	Annote = {Herleitung d\sigma / dE für Kapitel 4.2},
	Author = {A. Strumia and F. Vissani},
	Date-Added = {2020-04-22 13:37:39 +0200},
	Date-Modified = {2020-04-22 13:59:54 +0200},
	Doi = {10.1016/s0370-2693(03)00616-6},
	Journal = {Phys. Lett.},
	Pages = {42--54},
	Title = {Precise quasielastic neutrino/nucleon cross-section},
	Volume = {B564},
	Year = {2003}}

@phdthesis{Migenda2019,
	Archiveprefix = {arXiv},
	Author = {Jost Migenda},
	Date-Added = {2020-04-22 13:33:32 +0200},
	Date-Modified = {2020-05-22 22:16:21 +0200},
	Eprint = {2002.01649},
	Note = {\href{https://arxiv.org/abs/2002.01649}{\texttt{arXiv:2002.01649}}},
	School = {University of Sheffield},
	Title = {{Supernova Model Discrimination with Hyper-Kamiokande}},
	Year = {2019}}

@article{Fukuda2003,
	Abstract = {Super-Kamiokande is the world's largest water Cherenkov detector, with net mass 50,000 tons. During the period April, 1996 to July, 2001, Super-Kamiokande I collected 1678 live-days of data, observing neutrinos from the Sun, Earth's atmosphere, and the K2K long-baseline neutrino beam with high efficiency. These data provided crucial information for our current understanding of neutrino oscillations, as well as setting stringent limits on nucleon decay. In this paper, we describe the detector in detail, including its site, configuration, data acquisition equipment, online and offline software, and calibration systems which were used during Super-Kamiokande I.},
	Author = {S. Fukuda and others},
	Date-Added = {2020-04-22 13:22:05 +0200},
	Date-Modified = {2020-04-22 13:59:54 +0200},
	Journal = {Nucl. Instrum. Meth.},
	Pages = {418--462},
	Title = {{The Super-Kamiokande detector}},
	Volume = {A501},
	Year = {2003}}

@article{HKDR2018,
	Archiveprefix = {arXiv},
	Author = {Abe, K. and others},
	Collaboration = {Hyper-Kamiokande},
	Date-Added = {2020-04-22 13:21:45 +0200},
	Date-Modified = {2020-04-22 13:21:45 +0200},
	Eprint = {1805.04163},
	Note = {\href{https://arxiv.org/abs/1805.04163}{\texttt{arXiv:1805.04163}}},
	Primaryclass = {physics.ins-det},
	Slaccitation = {%%CITATION = ARXIV:1805.04163;%%},
	Title = {{Hyper-Kamiokande Design Report}},
	Year = {2018}}

@article{Nakazato2013,
	Archiveprefix = {arXiv},
	Author = {Nakazato, Ken'ichiro and Sumiyoshi, Kohsuke and Suzuki, Hideyuki and Totani, Tomonori and Umeda, Hideyuki and Yamada, Shoichi},
	Date-Added = {2020-04-22 13:21:09 +0200},
	Date-Modified = {2020-04-22 13:21:09 +0200},
	Doi = {10.1088/0067-0049/205/1/2},
	Eprint = {1210.6841},
	Journal = {Astrophys. J. Suppl.},
	Pages = {2},
	Primaryclass = {astro-ph.HE},
	Slaccitation = {%%CITATION = ARXIV:1210.6841;%%},
	Title = {{Supernova Neutrino Light Curves and Spectra for Various Progenitor Stars: From Core Collapse to Proto-neutron Star Cooling}},
	Volume = {205},
	Year = {2013}}

@article{Virtanen2020,
	Adsurl = {https://rdcu.be/b08Wh},
	Author = {{Virtanen}, Pauli and {Gommers}, Ralf and {Oliphant}, Travis E. and {Haberland}, Matt and {Reddy}, Tyler and {Cournapeau}, David and {Burovski}, Evgeni and {Peterson}, Pearu and {Weckesser}, Warren and {Bright}, Jonathan and {van der Walt}, Stéfan J. and {Brett}, Matthew and {Wilson}, Joshua and {Jarrod Millman}, K. and {Mayorov}, Nikolay and {Nelson}, Andrew R.~J. and {Jones}, Eric and {Kern}, Robert and {Larson}, Eric and {Carey}, CJ and {Polat}, İlhan and {Feng}, Yu and {Moore}, Eric W. and {VanderPlas}, Jake and {Laxalde}, Denis and {Perktold}, Josef and {Cimrman}, Robert and {Henriksen}, Ian and {Quintero}, E.~A. and {Harris}, Charles R and {Archibald}, Anne M. and {Ribeiro}, Antônio H. and {Pedregosa}, Fabian and {van Mulbregt}, Paul and {SciPy 1.0 Contributors}},
	Date-Added = {2020-04-22 13:20:32 +0200},
	Date-Modified = {2020-04-22 14:45:04 +0200},
	Doi = {10.1038/s41592-019-0686-2},
	Journal = {Nature Methods},
	Pages = {261--272},
	Title = {{SciPy 1.0: Fundamental Algorithms for Scientific Computing in Python}},
	Volume = {17},
	Year = {2020}}

@article{Walt2011,
	Archiveprefix = {arXiv},
	Author = {van der Walt, Stéfan and Colbert, S. Chris and Varoquaux, Gaël},
	Date-Added = {2020-04-22 13:19:27 +0200},
	Date-Modified = {2020-04-22 13:19:27 +0200},
	Doi = {10.1109/MCSE.2011.37},
	Eprint = {1102.1523},
	Journal = {Comput. Sci. Eng.},
	Number = {2},
	Pages = {22-30},
	Primaryclass = {cs.MS},
	Slaccitation = {%%CITATION = ARXIV:1102.1523;%%},
	Title = {{The NumPy Array: A Structure for Efficient Numerical Computation}},
	Volume = {13},
	Year = {2011}}