Detecting neutrinos from supernova bursts in PandaX-4T

[1]
S. Horiuchi, J. F. Beacom, and E. Dwek, Phys. Rev. D 79(8), 083013 (2009)
[2]
D. Kresse, T. Ertl, and H. T. Janka, Stellar collapse diversity and the diffuse supernova neutrino background, 2020
[3]
R. M. Bionta, G. Blewitt, C. B. Bratton et al., Phys. Rev. Lett., 58 , 1494 (1987)
[4]
K. Hirata, T. Kajita, M. Koshiba et al., Phys. Rev. Lett. 58 , 1490 (1987)
[5]
E. N. Alexeyev, L. N. Alexeyeva, I. V. Krivosheina et al., Phys. Lett. B 205(2), 209 (1988)
[6]
K. Abe et al., Astroparticle Physics, 81 , 39 (2016)
[7]
M. G. Aartsen et al., Astroparticle Physics 92, 30 (2017)
[8]
H. Y. Wei, L. Lebanowski, F. Li et al., Astroparticle Physics 75 , 38 (2016)
[9]
P. Antonioli et al., New Journal of Physics 6(1), 114 (2004)
[10]
S Al Kharusi et al., New Journal of Physics 23(3), 031201 (2021)
[11]
D. Z. Freedman, Phys. Rev. D 9 , 1389 (1974)
[12]
A. M. Suliga, J. F. Beacom, and I. Tamborra Phys. Rev. D 105, 043008 (2022)
[13]
Dmitry Akimov, J. Albert, Peibo An et al., Science 357(08), eaao0990 (2017)
[14]
E. Aprile et al., Journal of Cosmology and Astroparticle Physics 2020(11), 031 (2020)
[15]
D. S. Akerib et al., Nucl. Instrum. Meth. A 953, 163047 (2020)
[16]
Yue Meng et al. Phys. Rev. Lett. 127 , 261802 (2021)
[17]
J. Aalbers et al., Journal of Cosmology and Astroparticle Physics 2016(11), 017 (2016)
[18]
Abdusalam Abdukerim et al., PandaX-xT: a Multi-ten-tonne Liquid Xenon Observatory at the China Jinping Underground Laboratory, 2024, arXiv: 2402.03596
[19]
K. Bays et al., Phys. Rev. D 85 , 052007 (2012)
[20]
J. F. Beacom and L. E. Strigari, Phys. Rev. C 73 , 035807 (2006)
[21]
A. Mirizzi, I. Tamborra, H. Th. Janka et al., Nuovo Cimento Rivista Serie 39 (1-2), 1–112 (2016)
[22]
L. Hüdepohl, Neutrinos from the Formation, Cooling, and Black Hole Collapse of Neutron Stars, 2014
[23]
K. Nakazato, K. Sumiyoshi, H. Suzuki et al., The Astrophysical Journal Supplement Series 205 (1), 2 (2013)
[24]
H. G. Zhang, A. Abdukerim, W. Chen et al., Science China(Physics, Mechanics & Astronomy) 62, 031011 (2019)
[25]
J. Yang, X. Chen, C. He et al., Journal of Instrumentation 17 (02), T02004 (2022)
[26]
M. Tanabashi and K. Hagiwara et al. Phys. Rev. D 98 , 030001 (2018)
[27]
R. H. Helm, Phys. Rev. 104 , 1466 (1956)
[28]
J. Engel, Phys. Lett. B 264(1), 114 (1991)
[29]
T. Kozynets, S. Fallows, and C. B. Krauss, Astroparticle Physics 105, 25 (2019)
[30]
M. Th. Keil, G. G. Raffelt, and H. T. Janka, The Astrophysical Journal 590 (2), 971 (2003)
[31]
R. F. Lang, C. McCabe, S. Reichard et al., Phys. Rev. D 94 , 103009 (2016)
[32]
H. L. Li, Y. F. Li, M. Wang et al., Phys. Rev. D 97 , 063014 (2018)
[33]
J. M. Lattimer and F. D. Swesty, Nucl. Phys. A 535(2), 331 (1991)
[34]
K. Abe et al., Astroparticle Physics 89, 51 (2017)
[35]
Y. Y. Luo et al., Signal Response Model in PandaX-4T, 2024, arXiv: 2403.04239
[36]
J. Li et al., Waveform Simulation in PandaX-4T, 2013, arXiv: 2312.11072
[37]
M.Szydagiset al., Noble Element Simulation Technique v2.0, 2018
[38]
M. Szydagis, G. A. Block, C. Farquhar et al., Instruments 5(1), 13 (2021)
[39]
W. B. Ma et al., Phys. Rev. Lett. 130 , 021802 (2023)
[40]
M. Joyce, S. C. Leung, L. Molná et al., The Astrophysical Journal 902 (1), 63 (2020)
[41]
G. J. Feldman and R. D. Cousins, Phys. Rev. D 57, 3873 (1998)