KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars

Asakura, K.; Gando, A.; Gando, Y.; Hachiya, T.; Hayashida, S.; Ikeda, H.; Inoue, K.; Ishidoshiro, K.; Ishikawa, T.; Ishio, S.; Koga, M.; Matsuda, S.; Mitsui, T.; Motoki, D.; Nakamura, K.; Obara, S.; Oura, T.; Shimizu, I.; Shirahata, Y.; Shirai, J.; Suzuki, A.; Tachibana, H.; Tamae, K.; Ueshima, K.; Watanabe, H.; Xu, B. D.; Kozlov, A.; Takemoto, Y.; Yoshida, S.; Fushimi, K.; Piepke, A.; Banks, T. I.; Berger, B. E.; Fujikawa, B. K.; O’Donnell, T.; Learned, J. G.; Maricic, J.; Matsuno, S.; Sakai, M.; Winslow, L. A.; Efremenko, Y.; Karwowski, H. J.; Markoff, D. M.; Tornow, W.; Detwiler, J. A.; Enomoto, S.; Decowski, M. P.

doi:10.3847/0004-637X/818/1/91

Title: KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars

Authors:: Asakura, K.; Gando, A.; Gando, Y.; Hachiya, T.; Hayashida, S.; Ikeda, H.; Inoue, K.; Ishidoshiro, K.; Ishikawa, T.; Ishio, S.; Koga, M.; Matsuda, S.; Mitsui, T.; Motoki, D.; Nakamura, K.; Obara, S.; Oura, T.; Shimizu, I.; Shirahata, Y.; Shirai, J. more »« less

Publication Date:: 2016-02-10

Research Org.:: Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)

Sponsoring Org.:: USDOE Office of Science (SC), Nuclear Physics (NP); Nuclear Science Division

Contributing Org.:: The KamLAND Collaboration

OSTI Identifier:: 1379082

Alternate Identifier(s):: OSTI ID: 1469138

Report Number(s):: LBNL-1004322
Journal ID: ISSN 1538-4357; ark:/13030/qt8gq4z5tf

Grant/Contract Number:: AC02-05CH11231; FG03-00ER41138; FG02-01ER41166

Resource Type:: Accepted Manuscript

Journal Name:: The Astrophysical Journal (Online)

Additional Journal Information:: Journal Name: The Astrophysical Journal (Online); Journal Volume: 818; Journal Issue: 1; Journal ID: ISSN 1538-4357

Publisher:: Institute of Physics (IOP)

Country of Publication:: United States

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; neutrinos; supernovae: general

Citation Formats


                    Asakura, K., Gando, A., Gando, Y., Hachiya, T., Hayashida, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Ishikawa, T., Ishio, S., Koga, M., Matsuda, S., Mitsui, T., Motoki, D., Nakamura, K., Obara, S., Oura, T., Shimizu, I., Shirahata, Y., Shirai, J., Suzuki, A., Tachibana, H., Tamae, K., Ueshima, K., Watanabe, H., Xu, B. D., Kozlov, A., Takemoto, Y., Yoshida, S., Fushimi, K., Piepke, A., Banks, T. I., Berger, B. E., Fujikawa, B. K., O’Donnell, T., Learned, J. G., Maricic, J., Matsuno, S., Sakai, M., Winslow, L. A., Efremenko, Y., Karwowski, H. J., Markoff, D. M., Tornow, W., Detwiler, J. A., Enomoto, S., and Decowski, M. P. KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars.  United States: N. p., 2016. 
Web.  doi:10.3847/0004-637X/818/1/91.

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                    Asakura, K., Gando, A., Gando, Y., Hachiya, T., Hayashida, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Ishikawa, T., Ishio, S., Koga, M., Matsuda, S., Mitsui, T., Motoki, D., Nakamura, K., Obara, S., Oura, T., Shimizu, I., Shirahata, Y., Shirai, J., Suzuki, A., Tachibana, H., Tamae, K., Ueshima, K., Watanabe, H., Xu, B. D., Kozlov, A., Takemoto, Y., Yoshida, S., Fushimi, K., Piepke, A., Banks, T. I., Berger, B. E., Fujikawa, B. K., O’Donnell, T., Learned, J. G., Maricic, J., Matsuno, S., Sakai, M., Winslow, L. A., Efremenko, Y., Karwowski, H. J., Markoff, D. M., Tornow, W., Detwiler, J. A., Enomoto, S., & Decowski, M. P. KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars.  United States.  https://doi.org/10.3847/0004-637X/818/1/91

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                    Asakura, K., Gando, A., Gando, Y., Hachiya, T., Hayashida, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Ishikawa, T., Ishio, S., Koga, M., Matsuda, S., Mitsui, T., Motoki, D., Nakamura, K., Obara, S., Oura, T., Shimizu, I., Shirahata, Y., Shirai, J., Suzuki, A., Tachibana, H., Tamae, K., Ueshima, K., Watanabe, H., Xu, B. D., Kozlov, A., Takemoto, Y., Yoshida, S., Fushimi, K., Piepke, A., Banks, T. I., Berger, B. E., Fujikawa, B. K., O’Donnell, T., Learned, J. G., Maricic, J., Matsuno, S., Sakai, M., Winslow, L. A., Efremenko, Y., Karwowski, H. J., Markoff, D. M., Tornow, W., Detwiler, J. A., Enomoto, S., and Decowski, M. P. Wed .  
"KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars".  United States.  https://doi.org/10.3847/0004-637X/818/1/91.  https://www.osti.gov/servlets/purl/1379082.

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@article{osti_1379082,

  title        = {KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars},

  author       = {Asakura, K. and Gando, A. and Gando, Y. and Hachiya, T. and Hayashida, S. and Ikeda, H. and Inoue, K. and Ishidoshiro, K. and Ishikawa, T. and Ishio, S. and Koga, M. and Matsuda, S. and Mitsui, T. and Motoki, D. and Nakamura, K. and Obara, S. and Oura, T. and Shimizu, I. and Shirahata, Y. and Shirai, J. and Suzuki, A. and Tachibana, H. and Tamae, K. and Ueshima, K. and Watanabe, H. and Xu, B. D. and Kozlov, A. and Takemoto, Y. and Yoshida, S. and Fushimi, K. and Piepke, A. and Banks, T. I. and Berger, B. E. and Fujikawa, B. K. and O’Donnell, T. and Learned, J. G. and Maricic, J. and Matsuno, S. and Sakai, M. and Winslow, L. A. and Efremenko, Y. and Karwowski, H. J. and Markoff, D. M. and Tornow, W. and Detwiler, J. A. and Enomoto, S. and Decowski, M. P.},

  abstractNote = {},

  doi          = {10.3847/0004-637X/818/1/91},

  journal      = {The Astrophysical Journal (Online)},

  number       = 1,

  volume       = 818,

  place        = {United States},

  year         = {2016},

  month        = {2}

}

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Figure 1: Time evolution of the $\bar{v}_e$ luminosity of pre-SN just before collapse(Odrzywolek & Heger 2010) and of SN after collapse(Nakazato et al. 2013). Note the timescale of the horizontal axis, which is linear after the collapse but logarithmic before collapse.

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${}^{7}{Be}$ solar neutrino measurement with KamLAND

Journal Article Gando, A. ; Gando, Y. ; Hanakago, H. ; ... - Physical Review C, Nuclear Physics

We report a measurement of the neutrino-electron elastic scattering rate of 862 keV ⁷Be solar neutrinos based on a 165.4 kt d exposure of KamLAND. The observed rate is 582±94(kt d)^₋1, which corresponds to an 862-keV ⁷Be solar neutrino flux of (3.26±0.52)×10⁹cm^₋2s^₋1, assuming a pure electron-flavor flux. Comparing this flux with the standard solar model prediction and further assuming three-flavor mixing, a ν_e survival probability of 0.66±0.15 is determined from the KamLAND data. Lastly, utilizing a global three-flavor oscillation analysis, we obtain a total ⁷Be solar neutrino flux of (5.82±1.02)×10⁹cm^₋2s^₋1, which is consistent with the standard solar model predictions.
https://doi.org/10.1103/PhysRevC.92.055808

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journal, November 2013

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journal, March 2015

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journal, January 2004

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journal, October 2015

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journal, January 2015

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journal, October 2004

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journal, April 2009

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journal, April 1987

Supernova neutrino detection in Borexino
journal, February 2002

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journal, May 2014

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journal, April 2012

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journal, August 2013

Constraints on $θ_{13}$ from a three-flavor oscillation analysis of reactor antineutrinos at KamLAND
journal, March 2011

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journal, March 2008

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journal, October 2009

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journal, December 2015

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journal, April 2009

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journal, April 1987

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journal, July 1988

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journal, January 1996

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journal, July 2015

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journal, February 2008

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journal, February 2013

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journal, March 2011

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journal, June 2004

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journal, July 2009

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journal, March 2014

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journal, November 2012

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journal, July 2003

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journal, May 2009

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journal, November 2014

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journal, June 2012

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journal, January 2001

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journal, June 2005

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journal, December 2011

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journal, July 2011

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journal, August 2011

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text, January 2013

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text, January 2008

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text, January 2009

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text, January 2012

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text, January 2013

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text, January 2013

A compact ultra-clean system for deploying radioactive sources inside the KamLAND detector
text, January 2014

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text, January 2014

Coherent Network Analysis of Gravitational Waves from Three-Dimensional Core-Collapse Supernova Models
text, January 2015

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text, January 2003

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text, January 2004

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journal, March 2018

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journal, June 2016

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journal, February 2020

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journal, June 2016

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journal, November 2016

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journal, October 2017

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journal, December 2017

Neutrino Spectra from Nuclear Weak Interactions in sd -Shell Nuclei under Astrophysical Conditions
journal, January 2018

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journal, November 2019

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journal, January 2020

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text, January 2016

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text, January 2016

Neutrinos from beta processes in a presupernova: probing the isotopic evolution of a massive star
text, January 2017

Pulsational Pair-instability Supernovae. II. Neutrino Signals from Pulsations and their Detection by Terrestrial Neutrino Detectors
text, January 2020