Moon as a Giant Detector for Neutrino Streams from Pulsars

Oleg Borisovich Khavroshkin; Vladislav Vladimirovich Tsyplakov

doi:doi:10.11648/j.ijass.20170506.11

| Peer-Reviewed

Moon as a Giant Detector for Neutrino Streams from Pulsars

Oleg Borisovich Khavroshkin, Vladislav Vladimirovich Tsyplakov

Published in International Journal of Astrophysics and Space Science (Volume 5, Issue 6)

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

Views: Downloads:

Download PDF

Share This Article

Twitter
Linked In
Facebook

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.

Published in	International Journal of Astrophysics and Space Science (Volume 5, Issue 6)
DOI	10.11648/j.ijass.20170506.11
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), 2018. Published by Science Publishing Group

Keywords

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

References

[1]	Sadeh D., Ben Menahem A., Meidav M. Possible detection of gravitational waves from pulsars: Preprint TAUP-270-72. 1972.
[2]	Stanyukovich K. P, Khavroshkin O. B, Tsyplakov V.V. Detection of gravitational waves from pulsars / / Astronomer. circular. Bureau of Astronomical Communications of the USSR Academy of Sciences. 1974. № 824. 3 p.
[3]	Pleskach N. K. Quasi-harmonic oscillations of the microseismic background in the frequency range 1-5 Hz // Dokl. AN SSSR. 1977. Vol. 232, No. 3. P. 558-561.
[4]	Samokhin A. A. The effect of laser radiation on absorbing condensed media, Tr. IOFAN. M., 1988. T.13.
[5]	Gusev V. E., Karabutov A. A. Laser optoacoustics. M., 1991.
[6]	O. Khavroshkin, V. Tsyplakov, Nonlinear Seismology: Space Component, Saarbrücken: Palmarium Academic Publishing, 2013, 516 pp., ISBN 978-3-659-98415-0
[7]	Chamberlain J. Physics of auroras and radiation of the atmosphere. M.: I. L, 1963. 777 p.
[8]	Elvey C. T. Aurora borealis // Adv. Electronics and Electron Physics. 1957. N 9. P. 1–42.
[9]	O. Khavroshkin, V. Tsyplakov. Nonlinear seismoacoustics in cosmogony and astrophysics. RANS, Otd. Cosmogony. M. 2008, 48p.
[10]	K. Shpiring. Neutrino high-energy astronomy: a glimpse of the promised land. Physics-Uspekhi, Vol.184, No. 5, 2014, pp.510-523.
[11]	Oleg Khavroshkin, Vladislav Tsyplakov. RADIOACTIVITY OF NUCLEI IN A CENTRIFUGAL FORCE FIELD. The Natural Science (NS) Vol. 3, No.8, 733-737 (2011).
[12]	Oleg Khavroshkin, Vladislav Tsyplakov. Sun, Earth, radioactive ore: common periodicity. The Natural Science (NS) Vol. 5, No. 9, 1001 -1005, (2013).
[13]	Khavroshkin OB, Tsyplakov VV. Radioactivity, solar neutrinos, interactions. Engineering Physics.-2013, No. 8, pp 53-62.
[14]	Khavroshkin OB, Tsyplakov VV Natural radioactivity as an open system. Engineering Physics.-2013, No. 12, pp.40-44.
[15]	Nikolaev A. V., Khavroshkin OB, Tsyplakov VV. Structure of astrophysics component of seismic emission. Engineering Physics. 2016, No. 9, pp.69-73.
[16]	Bullen, KE, Introduction to Theoretical Seismology. Moscow: Mir, 1966, 460p.
[17]	Nikolaev AV, LN Rykunov, OE Starovoit, OB Khavroshkin, VV Tsyplakov. Nonlinear features of natural oscillations of the Earth. Academy of Sciences of the USSR, DNC, POI. Dynamic processes in discrete geophysical systems. Sat. works. Vladivostok, 1986, 138p.
[18]	Lin'kov EM, Tipisev S. Ya. Observation of long-period oscillations of the Earth by a seismograph with a photoelectric converter. Academy of Sciences of the USSR, DNC, POI. Dynamic processes in discrete geophysical systems. Sat. works. Vladivostok, 1986, 138s.
[19]	Ness NF, J. Harrison, LB Slichter. Observation of the Earth's own oscillations.- In.: Own oscillations of the Earth. Moscow: Mir, 1954, 60-79 pp.
[20]	Korchagin F. G., S. A. Chebotov. Some results of high-precision studies of deformation of the earth's surface. AN SSSR, DVO, TOI. Application of long-base laser interferometers in geophysics. Theses of reports, Vladivostok, 1987, 75p.
[21]	Antonova LM, Savina NG Analysis of low-frequency oscillations of the Earth recorded by a laser deformograph. Ibid.
[22]	A. V. Davydov, G. I. Dolgikh, W. H. Kopvillem, A. M. Zapolsky. The study of the background of the Earth's own oscillations. Part II. Ibid.
[23]	O. Khavroshkin, V. Tsyplakov, Introduction to Nonlinear Seismology, Saarbrücken: Palmarium Academic Publishing, 2013, 400 pp., ISBN 978-3-659-98197-5.
[24]	Man`ko V. I. (RAS). Reports at seminars of theoretical physics under the guidance of prof. AA Rukhadze. IOP RAS.
[25]	Alan Smith, I. A. Crawford, Robert Anthony Gowen, R. Ambrosi, M. Anand, B. Banerdt, N. Bannister, N. Bowles, C. Braithwaite and P. Brown, et al. Experimental Astronomy. Volume 33, Numbers 2-3 (2012), 587-644, DOI: 10.1007/s10686-011-9250-5Original Article Lunar Net—a proposal in response to an ESA M3 call in 2010 for a medium sized mission.
[26]	ATNF Pulsar Catalogue.
[27]	O. Khavroshkin, V. Tsyplakov. Hydrogen maser: solar periodicity. Engineering Physics.-2014, No. 3, p. p.25-34.
[28]	LV Grunskaya and co-authors, articles in the journal "Space, Time and Fundamental Interactions". April - June (2), 2014 Section "Part III. Identification of periodic components with frequencies of astrophysical processes in time series of the vertical component of the electric field strength of the boundary layer of the Earth's atmosphere ". www.profill.ru
[29]	Khavroshkin OB, Tsarev VA, Tsyplakov VV, Chechin VA Interaction of neutrino beams with a seismically active medium. M., 1985. 16c. (Representative / FANSSSR, No. 167).
[30]	Amaldi E., Coccia E., Frasca S. et al. Background of possible terrestrial origin. III.//Nuovo cim. C. 1989. Vol. 4, № 3. P. 299-308, 401-457.
[31]	Ryazhskaya OG, Ryasny VG Letters in the ZhETF, 1988, 47, 236.
[32]	Vavilov Yu. N., TZ Verbitsky, OB Khavroshkin. Analysis of the indications of the underground acoustic device on February 23, 1987. Letters to the JETP, vol. 50, no. 10, p. 411-412. 1988, 47, 236.
[33]	O. B. Khavroshkin, V. V. Tsyplakov. New problems of extraterrestrial seismology. Problems of geophysics of the XXI century. Sat. works in 2 books, Book 2, Managing editor, ch. - corr. RAS A. V. Nikolaev. RAS, United Institute of Physics of the Earth. O. Yu. Shmidt. M., "Science", 2003, pp.. 281-324.

Cite This Article

Plain Text BibTeX RIS

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

Copy | Download

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

Copy | Download

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

Copy | Download

@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}
}

Copy | Download

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

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

Download PDF

Sections

Plain Text BibTeX RIS

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

Copy | Download

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

Copy | Download

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

Copy | Download

@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}
}

Copy | Download

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