Supernova neutrino detection in NOvA
The NOvA long-baseline neutrino experiment uses a pair of large, segmented, liquid-scintillator calorimeters to study neutrino oscillations, using GeV-scale neutrinos from the Fermilab NuMI beam. These detectors are also sensitive to the flux of neutrinos which are emitted during a core-collapse sup...
- Autores:
-
Acero, M. A.
- Tipo de recurso:
- Fecha de publicación:
- 2020
- Institución:
- Universidad del Atlántico
- Repositorio:
- Repositorio Uniatlantico
- Idioma:
- eng
- OAI Identifier:
- oai:repositorio.uniatlantico.edu.co:20.500.12834/952
- Acceso en línea:
- https://hdl.handle.net/20.500.12834/952
- Palabra clave:
- neutrino: burst, neutrino: supernova, core-collapse supernova, neutrino: detection
- Rights
- openAccess
- License
- http://purl.org/coar/access_right/c_abf2
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Supernova neutrino detection in NOvA |
| title |
Supernova neutrino detection in NOvA |
| spellingShingle |
Supernova neutrino detection in NOvA neutrino: burst, neutrino: supernova, core-collapse supernova, neutrino: detection |
| title_short |
Supernova neutrino detection in NOvA |
| title_full |
Supernova neutrino detection in NOvA |
| title_fullStr |
Supernova neutrino detection in NOvA |
| title_full_unstemmed |
Supernova neutrino detection in NOvA |
| title_sort |
Supernova neutrino detection in NOvA |
| dc.creator.fl_str_mv |
Acero, M. A. |
| dc.contributor.author.none.fl_str_mv |
Acero, M. A. |
| dc.subject.keywords.spa.fl_str_mv |
neutrino: burst, neutrino: supernova, core-collapse supernova, neutrino: detection |
| topic |
neutrino: burst, neutrino: supernova, core-collapse supernova, neutrino: detection |
| description |
The NOvA long-baseline neutrino experiment uses a pair of large, segmented, liquid-scintillator calorimeters to study neutrino oscillations, using GeV-scale neutrinos from the Fermilab NuMI beam. These detectors are also sensitive to the flux of neutrinos which are emitted during a core-collapse supernova through inverse beta decay interactions on carbon at energies of O(10 MeV). This signature provides a means to study the dominant mode of energy release for a core-collapse supernova occurring in our galaxy. We describe the datadriven software trigger system developed and employed by the NOvA experiment to identify and record neutrino data from nearby galactic supernovae. This technique has been used by NOvA to self-trigger on potential core-collapse supernovae in our galaxy, with an estimated sensitivity reaching out to 10 kpc distance while achieving a detection efficiency of 23% to 49% for supernovae from progenitor stars with masses of 9.6 M to 27 M , respectively. |
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2020 |
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2020-10-05 |
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2020-07-29 |
| dc.date.accessioned.none.fl_str_mv |
2022-11-15T21:13:14Z |
| dc.date.available.none.fl_str_mv |
2022-11-15T21:13:14Z |
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http://purl.org/coar/version/c_970fb48d4fbd8a85 |
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http://purl.org/coar/resource_type/c_2df8fbb1 |
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info:eu-repo/semantics/article |
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Artículo |
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publishedVersion |
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https://hdl.handle.net/20.500.12834/952 |
| dc.identifier.doi.none.fl_str_mv |
10.1088/1475-7516/2020/10/014 |
| dc.identifier.instname.spa.fl_str_mv |
Universidad del Atlántico |
| dc.identifier.reponame.spa.fl_str_mv |
Repositorio Universidad del Atlántico |
| url |
https://hdl.handle.net/20.500.12834/952 |
| identifier_str_mv |
10.1088/1475-7516/2020/10/014 Universidad del Atlántico Repositorio Universidad del Atlántico |
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eng |
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eng |
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http://purl.org/coar/access_right/c_abf2 |
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openAccess |
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Sede Norte |
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JCAP |
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Universidad del Atlántico |
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https://repositorio.uniatlantico.edu.co/bitstream/20.500.12834/952/1/2005.07155.pdf https://repositorio.uniatlantico.edu.co/bitstream/20.500.12834/952/2/license.txt |
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Acero, M. A.979f9c6a-faae-415d-b017-8ea1e9afa74c2022-11-15T21:13:14Z2022-11-15T21:13:14Z2020-10-052020-07-29https://hdl.handle.net/20.500.12834/95210.1088/1475-7516/2020/10/014Universidad del AtlánticoRepositorio Universidad del AtlánticoThe NOvA long-baseline neutrino experiment uses a pair of large, segmented, liquid-scintillator calorimeters to study neutrino oscillations, using GeV-scale neutrinos from the Fermilab NuMI beam. These detectors are also sensitive to the flux of neutrinos which are emitted during a core-collapse supernova through inverse beta decay interactions on carbon at energies of O(10 MeV). This signature provides a means to study the dominant mode of energy release for a core-collapse supernova occurring in our galaxy. We describe the datadriven software trigger system developed and employed by the NOvA experiment to identify and record neutrino data from nearby galactic supernovae. This technique has been used by NOvA to self-trigger on potential core-collapse supernovae in our galaxy, with an estimated sensitivity reaching out to 10 kpc distance while achieving a detection efficiency of 23% to 49% for supernovae from progenitor stars with masses of 9.6 M to 27 M , respectively.application/pdfengJCAPSupernova neutrino detection in NOvAneutrino: burst, neutrino: supernova, core-collapse supernova, neutrino: detectioninfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArtículohttp://purl.org/coar/version/c_970fb48d4fbd8a85http://purl.org/coar/resource_type/c_2df8fbb1BarranquillaSede Norteinfo:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2[1] R. M. Bionta et al., Observation of a neutrino burst in coincidence with supernova SN1987A in the Large Magellanic Cloud, Phys. Rev. Lett. 58 (1987) 1494.[2] KAMIOKANDE-II collaboration, Observation of a neutrino burst from the supernova SN1987A, Phys. Rev. Lett. 58 (1987) 1490.[3] E. N. Alekseev, L. N. Alekseeva, V. I. Volchenko and I. V. Krivosheina, Possible detection of a neutrino signal on 23 February 1987 at the Baksan underground scintillation telescope of the Institute of Nuclear Research, JETP Lett. 45 (1987) 589.[4] M. Aglietta et al., On the event observed in the Mont Blanc underground neutrino observatory during the occurrence of Supernova 1987a, Europhys. Lett. 3 (1987) 1315.[5] P. Antonioli et al., SNEWS: The Supernova Early Warning System, New J. Phys. 6 (2004) 114 [astro-ph/0406214].[6] NOvA collaboration, The NOvA Technical Design Report[7] P. Adamson et al., The NuMI Neutrino Beam, Nucl. Instrum. Meth. A806 (2016) 279 [1507.06690].[8] R. L. Talaga, J. J. Grudzinski, S. Phan-Budd, A. Pla-Dalmau, J. E. Fagan, C. Grozis et al., PVC Extrusion Development and Production for the NOvA Neutrino Experiment, Nucl. Instrum. Meth. A861 (2017) 77 [1601.00908].[9] S. Mufson et al., Liquid Scintillator Production for the NOvA Experiment, Nucl. Instrum. Meth. A799 (2015) 1 [1504.04035].[10] A. Norman et al., Performance of the NOvA Data Acquisition and Trigger Systems for the full 14 kT Far Detector, J. Phys. Conf. Ser. 664 (2015) 082041.[11] K. Scholberg, Supernova Neutrino Detection, Ann. Rev. Nucl. Part. Sci. 62 (2012) 81 [1205.6003][12] T. Totani, K. Sato, H. E. Dalhed and J. R. Wilson, Future detection of supernova neutrino burst and explosion mechanism, The Astrophysical Journal 496 (1998) 216[13] A. Mirizzi, I. Tamborra, H.-T. Janka, N. Saviano, K. Scholberg, R. Bollig et al., Supernova Neutrinos: Production, Oscillations and Detection, Riv. Nuovo Cim. 39 (2016) 1 [1508.00785].[14] K. Nakazato, K. Sumiyoshi, H. Suzuki, T. Totani, H. Umeda and S. Yamada, Supernova neutrino light curves and spectra for various progenitor stars: From core colllapse to proto-neutron star cooling, The Astrophysical Journal Supplement Series 205 (2013) 2.[15] A. Strumia and F. Vissani, Precise quasi-elastic neutrino/nucleon cross-section, Physics Letters B 564 (2003) 42 .[16] W. J. Marciano and Z. Parsa, Neutrino–electron scattering theory, Journal of Physics G: Nuclear and Particle Physics 29 (2003) 2629.[17] B. Armbruster, I. Blair, B. Bodmann, N. Booth, G. Drexlin, V. Eberhard et al., Measurement of the weak neutral current excitation 12C(νµ, ν0 µ ) 12C ∗ (1+, 1; 15.1 MeV ) at Eνµ = 29.8 MeV , Physics Letters B 423 (1998) 15[18] C. Andreopoulos, A. Bell, D. Bhattacharya, F. Cavanna, J. Dobson, S. Dytman et al., The GENIE neutrino Monte Carlo generator, Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 614 (2010) 87 .[19] S. Agostinelli et al., Geant4 — a simulation toolkit, Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 506 (2003) 250[20] A. Aurisano, C. Backhouse, R. Hatcher, N. Mayer, J. Musser, R. Patterson et al., The NOvA simulation chain, Journal of Physics: Conference Series 664 (2015) 072002.21] NOvA collaboration, New Constraints on Oscillation Parameters from νe Appearance and νµ Disappearance in the NOvA Experiment, Phys. Rev. D98 (2018) 032012 [1806.00096].[22] NOvA collaboration, First measurement of muon-neutrino disappearance in NOvA, Phys. Rev. D93 (2016) 051104 [1601.05037].[23] M. Baird, J. Bian, M. Messier, E. Niner, D. Rocco and K. Sachdev, Event reconstruction techniques in NOvA, Journal of Physics: Conference Series 664 (2015) 072035.[24] NOvA collaboration, The NOvA Timing System: A System for Synchronizing a Long Baseline Neutrino Experiment, J. Phys. Conf. Ser. 396 (2012) 012034.[25] A. Habig and J. Zirnstein, Integration of the Super Nova Early Warning System with the NOvA trigger, Journal of Physics: Conference Series 664 (2015) 08201526] K. Scholberg, Supernova Signatures of Neutrino Mass Ordering, J. Phys. G 45 (2018) 014002 [1707.06384].27] A. Mirizzi, G. G. Raffelt and P. Serpico, Earth matter effects in supernova neutrinos: Optimal detector locations, JCAP 0605 (2006) 012 [astro-ph/0604300].http://purl.org/coar/resource_type/c_6501ORIGINAL2005.07155.pdf2005.07155.pdfapplication/pdf2018647https://repositorio.uniatlantico.edu.co/bitstream/20.500.12834/952/1/2005.07155.pdf84c88dd2c92af18d5007636c1efcdca5MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81306https://repositorio.uniatlantico.edu.co/bitstream/20.500.12834/952/2/license.txt67e239713705720ef0b79c50b2ececcaMD5220.500.12834/952oai:repositorio.uniatlantico.edu.co:20.500.12834/9522022-11-15 16:13:15.092DSpace de la Universidad de Atlánticosysadmin@mail.uniatlantico.edu.coVMOpcm1pbm9zIGdlbmVyYWxlcyBkZWwgUmVwb3NpdG9yaW8gSW5zdGl0dWNpb25hbCBkZSBsYSBVbml2ZXJzaWRhZCBkZWwgQXRsw6FudGljbwoKRWwgKGxvcykgYXV0b3IgKGVzKSBoYW4gYXNlZ3VyYWRvIChuKSBsbyBzaWd1aWVudGUgc29icmUgbGEgb2JyYSBhIGludGVncmFyIGVuIGVsIFJlcG9zaXRvcmlvIEluc3RpdHVjaW9uYWwsIHF1ZToKCuKXjwlFcyBvcmlnaW5hbCwgZGUgc3UgZXhjbHVzaXZhIGF1dG9yw61hLCBzZSByZWFsaXrDsyBzaW4gdmlvbGFyIG8gdXN1cnBhciBkZXJlY2hvcyBkZSBhdXRvciBkZSB0ZXJjZXJvcyB5IHBvc2VlIGxhIHRpdHVsYXJpZGFkLgril48JQXN1bWlyw6FuIGxhIHJlc3BvbnNhYmlsaWRhZCB0b3RhbCBwb3IgZWwgY29udGVuaWRvIGEgbGEgb2JyYSBhbnRlIGxhIEluc3RpdHVjacOzbiB5IHRlcmNlcm9zLgril48JQXV0b3JpemFuIGEgdMOtdHVsbyBncmF0dWl0byB5IHJlbnVuY2lhcyBhIHJlY2liaXIgZW1vbHVtZW50b3MgcG9yIGxhcyBhY3RpdmlkYWRlcyBxdWUgc2UgcmVhbGljZW4gY29uIGVsbGEsIHNlZ8O6biBzdSBsaWNlbmNpYS4KCgpMYSBVbml2ZXJzaWRhZCBkZWwgQXRsw6FudGljbywgcG9yIHN1IHBhcnRlLCBzZSBjb21wcm9tZXRlIGEgYWN0dWFyIGVuIGxvcyB0w6lybWlub3MgZXN0YWJsZWNpZG9zIGVuIGxhIExleSAyMyBkZSAxOTgyIHkgbGEgRGVjaXNpw7NuIEFuZGluYSAzNTEgZGUgMTk5MywgZGVtw6FzIG5vcm1hcyBnZW5lcmFsZXMgc29icmUgbGEgbWF0ZXJpYSB5IGVsIEFjdWVyZG8gU3VwZXJpb3IgMDAxIGRlIDE3IGRlIG1hcnpvIGRlIDIwMTEsIHBvciBtZWRpbyBkZWwgY3VhbCBzZSBleHBpZGUgZWwgRXN0YXR1dG8gZGUgUHJvcGllZGFkIEludGVsZWN0dWFsIGRlIGxhIFVuaXZlcnNpZGFkIGRlbCBBdGzDoW50aWNvLgoKUG9yIMO6bHRpbW8sIGhhbiBzaWRvIGluZm9ybWFkb3Mgc29icmUgZWwgdHJhdGFtaWVudG8gZGUgZGF0b3MgcGVyc29uYWxlcyBwYXJhIGZpbmVzIGFjYWTDqW1pY29zIHkgZW4gYXBsaWNhY2nDs24gZGUgY29udmVuaW9zIGNvbiB0ZXJjZXJvcyBvIHNlcnZpY2lvcyBjb25leG9zIGNvbiBhY3RpdmlkYWRlcyBwcm9waWFzIGRlIGxhIGFjYWRlbWlhLCBiYWpvIGVsIGVzdHJpY3RvIGN1bXBsaW1pZW50byBkZSBsb3MgcHJpbmNpcGlvcyBkZSBsZXkuCgpMYXMgY29uc3VsdGFzLCBjb3JyZWNjaW9uZXMgeSBzdXByZXNpb25lcyBkZSBkYXRvcyBwZXJzb25hbGVzIHB1ZWRlbiBwcmVzZW50YXJzZSBhbCBjb3JyZW8gZWxlY3Ryw7NuaWNvIGhhYmVhc2RhdGFAbWFpbC51bmlhdGxhbnRpY28uZWR1LmNvCg== |