Moon as a Giant Detector for Neutrino Streams from Pulsars

Oleg Borisovich Khavroshkin; Vladislav Vladimirovich Tsyplakov

doi:doi:10.11648/j.ijass.20170506.11

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Moon as a Giant Detector for Neutrino Streams from Pulsars

Oleg Borisovich Khavroshkin, Vladislav Vladimirovich Tsyplakov

Received: 6 November 2017 Accepted: 28 January 2018 Published: 29 January 2018

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Abstract

Unaddressed existence of extraterrestrial sources of high energy neutrinos was discovered in 2013y. But the most promising addition to supernovae includes objects such as pulsars and closes multiple systems. Relying mainly on its own experience in the search and registration of the seismic response at frequencies of pulsars and close binary stars on Earth and the Moon and using the results to detect solar neutrinos work on the study of modulated neutrino fluxes were continued. The study of the spectra of lunar seismic noise revealed a number of significant spectral peaks that match the frequency to 3-4 significant figures with the frequencies of sending energy pulses from pulsars. At the same time availability of registration of seismic peaks and their characteristics are strongly associated with the shape and depth of the radioactive geological structures of the lithosphere of the Moon. That is the energy of interaction modulated beam of neutrinos from the pulsar radioactive elements Moon differently converted into energy of seismic noise. There have also been recorded seismic peaks well coincides with the period of close binary stars. Some of the peaks previously were registered not only as a purely seismic frequency, but as the frequency inherent to radioactive laboratory sources. It is further confirms their astrophysical neutrino origin and similar search becomes the part of high-energy neutrino astronomy.

DOI	10.11648/j.ijass.20170506.11
Published in	International Journal of Astrophysics and Space Science (Volume 5, Issue 6, December 2017)
Page(s)	85-99
Creative Commons	This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.
Copyright	Copyright © The Author(s), 2024. Published by Science Publishing Group

Keywords

Solar Neutrino Stream, ANRI-Absorption, Free Solar Oscillation, Neutrino Stream from Pulsars, Radioactivity Lunar Zones

References

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Oleg Borisovich Khavroshkin, Vladislav Vladimirovich Tsyplakov. (2018). Moon as a Giant Detector for Neutrino Streams from Pulsars. International Journal of Astrophysics and Space Science, 5(6), 85-99. https://doi.org/10.11648/j.ijass.20170506.11

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Oleg Borisovich Khavroshkin; Vladislav Vladimirovich Tsyplakov. Moon as a Giant Detector for Neutrino Streams from Pulsars. Int. J. Astrophys. Space Sci. 2018, 5(6), 85-99. doi: 10.11648/j.ijass.20170506.11

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AMA Style

Oleg Borisovich Khavroshkin, Vladislav Vladimirovich Tsyplakov. Moon as a Giant Detector for Neutrino Streams from Pulsars. Int J Astrophys Space Sci. 2018;5(6):85-99. doi: 10.11648/j.ijass.20170506.11

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@article{10.11648/j.ijass.20170506.11,
  author = {Oleg Borisovich Khavroshkin and Vladislav Vladimirovich Tsyplakov},
  title = {Moon as a Giant Detector for Neutrino Streams from Pulsars},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {5},
  number = {6},
  pages = {85-99},
  doi = {10.11648/j.ijass.20170506.11},
  url = {https://doi.org/10.11648/j.ijass.20170506.11},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20170506.11},
  abstract = {Unaddressed existence of extraterrestrial sources of high energy neutrinos was discovered in 2013y. But the most promising addition to supernovae includes objects such as pulsars and closes multiple systems. Relying mainly on its own experience in the search and registration of the seismic response at frequencies of pulsars and close binary stars on Earth and the Moon and using the results to detect solar neutrinos work on the study of modulated neutrino fluxes were continued. The study of the spectra of lunar seismic noise revealed a number of significant spectral peaks that match the frequency to 3-4 significant figures with the frequencies of sending energy pulses from pulsars. At the same time availability of registration of seismic peaks and their characteristics are strongly associated with the shape and depth of the radioactive geological structures of the lithosphere of the Moon. That is the energy of interaction modulated beam of neutrinos from the pulsar radioactive elements Moon differently converted into energy of seismic noise. There have also been recorded seismic peaks well coincides with the period of close binary stars. Some of the peaks previously were registered not only as a purely seismic frequency, but as the frequency inherent to radioactive laboratory sources. It is further confirms their astrophysical neutrino origin and similar search becomes the part of high-energy neutrino astronomy.},
 year = {2018}
}

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TY  - JOUR
T1  - Moon as a Giant Detector for Neutrino Streams from Pulsars
AU  - Oleg Borisovich Khavroshkin
AU  - Vladislav Vladimirovich Tsyplakov
Y1  - 2018/01/29
PY  - 2018
N1  - https://doi.org/10.11648/j.ijass.20170506.11
DO  - 10.11648/j.ijass.20170506.11
T2  - International Journal of Astrophysics and Space Science
JF  - International Journal of Astrophysics and Space Science
JO  - International Journal of Astrophysics and Space Science
SP  - 85
EP  - 99
PB  - Science Publishing Group
SN  - 2376-7022
UR  - https://doi.org/10.11648/j.ijass.20170506.11
AB  - Unaddressed existence of extraterrestrial sources of high energy neutrinos was discovered in 2013y. But the most promising addition to supernovae includes objects such as pulsars and closes multiple systems. Relying mainly on its own experience in the search and registration of the seismic response at frequencies of pulsars and close binary stars on Earth and the Moon and using the results to detect solar neutrinos work on the study of modulated neutrino fluxes were continued. The study of the spectra of lunar seismic noise revealed a number of significant spectral peaks that match the frequency to 3-4 significant figures with the frequencies of sending energy pulses from pulsars. At the same time availability of registration of seismic peaks and their characteristics are strongly associated with the shape and depth of the radioactive geological structures of the lithosphere of the Moon. That is the energy of interaction modulated beam of neutrinos from the pulsar radioactive elements Moon differently converted into energy of seismic noise. There have also been recorded seismic peaks well coincides with the period of close binary stars. Some of the peaks previously were registered not only as a purely seismic frequency, but as the frequency inherent to radioactive laboratory sources. It is further confirms their astrophysical neutrino origin and similar search becomes the part of high-energy neutrino astronomy.
VL  - 5
IS  - 6
ER  -

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Author Information

Oleg Borisovich Khavroshkin

Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia
Vladislav Vladimirovich Tsyplakov

Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia

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APA Style

Oleg Borisovich Khavroshkin, Vladislav Vladimirovich Tsyplakov. (2018). Moon as a Giant Detector for Neutrino Streams from Pulsars. International Journal of Astrophysics and Space Science, 5(6), 85-99. https://doi.org/10.11648/j.ijass.20170506.11

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ACS Style

Oleg Borisovich Khavroshkin; Vladislav Vladimirovich Tsyplakov. Moon as a Giant Detector for Neutrino Streams from Pulsars. Int. J. Astrophys. Space Sci. 2018, 5(6), 85-99. doi: 10.11648/j.ijass.20170506.11

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AMA Style

Oleg Borisovich Khavroshkin, Vladislav Vladimirovich Tsyplakov. Moon as a Giant Detector for Neutrino Streams from Pulsars. Int J Astrophys Space Sci. 2018;5(6):85-99. doi: 10.11648/j.ijass.20170506.11

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@article{10.11648/j.ijass.20170506.11,
  author = {Oleg Borisovich Khavroshkin and Vladislav Vladimirovich Tsyplakov},
  title = {Moon as a Giant Detector for Neutrino Streams from Pulsars},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {5},
  number = {6},
  pages = {85-99},
  doi = {10.11648/j.ijass.20170506.11},
  url = {https://doi.org/10.11648/j.ijass.20170506.11},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20170506.11},
  abstract = {Unaddressed existence of extraterrestrial sources of high energy neutrinos was discovered in 2013y. But the most promising addition to supernovae includes objects such as pulsars and closes multiple systems. Relying mainly on its own experience in the search and registration of the seismic response at frequencies of pulsars and close binary stars on Earth and the Moon and using the results to detect solar neutrinos work on the study of modulated neutrino fluxes were continued. The study of the spectra of lunar seismic noise revealed a number of significant spectral peaks that match the frequency to 3-4 significant figures with the frequencies of sending energy pulses from pulsars. At the same time availability of registration of seismic peaks and their characteristics are strongly associated with the shape and depth of the radioactive geological structures of the lithosphere of the Moon. That is the energy of interaction modulated beam of neutrinos from the pulsar radioactive elements Moon differently converted into energy of seismic noise. There have also been recorded seismic peaks well coincides with the period of close binary stars. Some of the peaks previously were registered not only as a purely seismic frequency, but as the frequency inherent to radioactive laboratory sources. It is further confirms their astrophysical neutrino origin and similar search becomes the part of high-energy neutrino astronomy.},
 year = {2018}
}

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TY  - JOUR
T1  - Moon as a Giant Detector for Neutrino Streams from Pulsars
AU  - Oleg Borisovich Khavroshkin
AU  - Vladislav Vladimirovich Tsyplakov
Y1  - 2018/01/29
PY  - 2018
N1  - https://doi.org/10.11648/j.ijass.20170506.11
DO  - 10.11648/j.ijass.20170506.11
T2  - International Journal of Astrophysics and Space Science
JF  - International Journal of Astrophysics and Space Science
JO  - International Journal of Astrophysics and Space Science
SP  - 85
EP  - 99
PB  - Science Publishing Group
SN  - 2376-7022
UR  - https://doi.org/10.11648/j.ijass.20170506.11
AB  - Unaddressed existence of extraterrestrial sources of high energy neutrinos was discovered in 2013y. But the most promising addition to supernovae includes objects such as pulsars and closes multiple systems. Relying mainly on its own experience in the search and registration of the seismic response at frequencies of pulsars and close binary stars on Earth and the Moon and using the results to detect solar neutrinos work on the study of modulated neutrino fluxes were continued. The study of the spectra of lunar seismic noise revealed a number of significant spectral peaks that match the frequency to 3-4 significant figures with the frequencies of sending energy pulses from pulsars. At the same time availability of registration of seismic peaks and their characteristics are strongly associated with the shape and depth of the radioactive geological structures of the lithosphere of the Moon. That is the energy of interaction modulated beam of neutrinos from the pulsar radioactive elements Moon differently converted into energy of seismic noise. There have also been recorded seismic peaks well coincides with the period of close binary stars. Some of the peaks previously were registered not only as a purely seismic frequency, but as the frequency inherent to radioactive laboratory sources. It is further confirms their astrophysical neutrino origin and similar search becomes the part of high-energy neutrino astronomy.
VL  - 5
IS  - 6
ER  -

Copy | Download