Skip to content
DraconiticResearch
Search Sources API
203,234 studies31 sourcesUpdated 42 min ago
PreprintarXiv licencearXiv

Study of Supernova Neutrinos at ESSnuSB

87 more authors

60 listed; 99 in total.

Abstract

In this paper, we have studied the sensitivity of the ESSnuSB far detector to supernova neutrinos. ESSnuSB is a proposed long-baseline neutrino experiment in Sweden, which will use a 538 kt water Cherenkov detector to probe the leptonic phase δCP by studying the second oscillation maximum. However, given the very large detector volume, it will have an excellent sensitivity to supernova neutrinos if a supernova explosion occurs during the run-time of ESSnuSB. Motivated by this, we first estimate the expected event rates at the ESSnuSB far detector for three different supernova flux models and then we probe its capability to distinguish these flux models. Additionally, we also investigate the impact of systematic errors and detector efficiency. Our results show that depending on the model of the supernova neutrinos, the expected number of events detected at Earth varies significantly. Our results also show that the ESSnuSB far detector may have excellent potential in distinguishing these flux models depending upon the distance of the supernova explosion, systematic errors and detector efficiency.

Related

  1. Diffuse Supernova Neutrinos with Secret Neutrino Interactions
    Praveen Bharadwaj, Utpal Chattopadhyay, Dilip Kumar Ghosh +1
    arXivPreprintarXiv licenceFull textHigh-energy astrophysicsHigh-energy & particle physicsarXiv
  2. Sensitivities of long and medium baseline experiments to sterile neutrinos and non-standard interactions
    Sambit Kumar Pusty, Trisha Guin, Rukmani Mohanta
    Physics Letters BPeer-reviewedCC BY 4.0Full textHigh-energy & particle physicsCrossref
  3. Exploring R˜2 leptoquarks and Majorana neutrinos via same-sign dimuons at the HL-LHC
    Subham Saha, Arvind Bhaskar, Manimala Mitra
    Physics Letters BPeer-reviewedCC BY 4.0Full textHigh-energy & particle physicsCrossref
  4. Cosmogenic neutrinos from FRII galaxies as potential origin of the ultra-high-energy KM3-230213A event
    Denis Allard, Bruny Baret, Noémie Globus +1
    HALPreprintLicence not statedGeneral astronomyGeneral physicsHAL
  5. Charge exchange reactions with central and tensor interactions and nuclear matrix elements associated with double-beta-decay neutrinos and astro neutrinos
    Hiroyasu Ejiri, Yoritaka Iwata
    arXivPreprintCC BY 4.0Full textNuclear physicsarXiv
BibTeX
@misc{essnusb2026study,
  title = {{Study of Supernova Neutrinos at ESSnuSB}},
  author = {ESSnuSB and J. Aguilar and M. Anastasopoulos and D. Barčot and E. Baussan and A. K. Bhattacharyya and A. Bignami and M. Blennow and M. Bogomilov and B. Bolling and E. Bouquerel and F. Bramati and A. Branca and G. Brunetti and I. Bustinduy and C. J. Carlile and J. Cederkall and T. W. Choi and S. Choubey and P. Christiansen and E. Cristaldo Morales and P. Cupiał and D. D'Ago and H. Danared and J. P. A. M. de André and M. Dracos and I. Efthymiopoulos and T. Ekelöf and M. Eshraqi and G. Fanourakis and A. Farricker and E. Fasoula and T. Fukuda and S. Gago and N. Gazis and Th. Geralis and M. Ghosh and A. Giarnetti and G. Gokbulut and C. Hagner and L. Halić and J. Hiegel and M. Hooft and K. E. Iversen and N. Jachowicz and M. Jakkapu and M. Jensen and I. Karakoulias and E. Kasimi and A. Kayis Topaksu and B. Kliček and K. Kordas and B. Kovač and A. Leisos and A. Longhin and M. López and C. Maiano and S. Marangoni and J. G. Marcos and C. Marrelli},
  howpublished = {arXiv},
  year = {2026},
  month = aug,
  doi = {10.48550/arxiv.2606.27007},
  eprint = {2606.27007},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2606.27007},
}
RIS
TY  - UNPB
TI  - Study of Supernova Neutrinos at ESSnuSB
AU  - ESSnuSB
AU  - J. Aguilar
AU  - M. Anastasopoulos
AU  - D. Barčot
AU  - E. Baussan
AU  - A. K. Bhattacharyya
AU  - A. Bignami
AU  - M. Blennow
AU  - M. Bogomilov
AU  - B. Bolling
AU  - E. Bouquerel
AU  - F. Bramati
AU  - A. Branca
AU  - G. Brunetti
AU  - I. Bustinduy
AU  - C. J. Carlile
AU  - J. Cederkall
AU  - T. W. Choi
AU  - S. Choubey
AU  - P. Christiansen
AU  - E. Cristaldo Morales
AU  - P. Cupiał
AU  - D. D'Ago
AU  - H. Danared
AU  - J. P. A. M. de André
AU  - M. Dracos
AU  - I. Efthymiopoulos
AU  - T. Ekelöf
AU  - M. Eshraqi
AU  - G. Fanourakis
AU  - A. Farricker
AU  - E. Fasoula
AU  - T. Fukuda
AU  - S. Gago
AU  - N. Gazis
AU  - Th. Geralis
AU  - M. Ghosh
AU  - A. Giarnetti
AU  - G. Gokbulut
AU  - C. Hagner
AU  - L. Halić
AU  - J. Hiegel
AU  - M. Hooft
AU  - K. E. Iversen
AU  - N. Jachowicz
AU  - M. Jakkapu
AU  - M. Jensen
AU  - I. Karakoulias
AU  - E. Kasimi
AU  - A. Kayis Topaksu
AU  - B. Kliček
AU  - K. Kordas
AU  - B. Kovač
AU  - A. Leisos
AU  - A. Longhin
AU  - M. López
AU  - C. Maiano
AU  - S. Marangoni
AU  - J. G. Marcos
AU  - C. Marrelli
PY  - 2026
DA  - 2026/08/28
PB  - arXiv
DO  - 10.48550/arxiv.2606.27007
UR  - https://arxiv.org/abs/2606.27007
AB  - In this paper, we have studied the sensitivity of the ESSnuSB far detector to supernova neutrinos. ESSnuSB is a proposed long-baseline neutrino experiment in Sweden, which will use a 538 kt water Cherenkov detector to probe the leptonic phase δ_CP by studying the second oscillation maximum. However, given the very large detector volume, it will have an excellent sensitivity to supernova neutrinos if a supernova explosion occurs during the run-time of ESSnuSB. Motivated by this, we first estimate the expected event rates at the ESSnuSB far detector for three different supernova flux models and then we probe its capability to distinguish these flux models. Additionally, we also investigate the impact of systematic errors and detector efficiency. Our results show that depending on the model of the supernova neutrinos, the expected number of events detected at Earth varies significantly. Our results also show that the ESSnuSB far detector may have excellent potential in distinguishing these flux models depending upon the distance of the supernova explosion, systematic errors and detector efficiency.
ER  -