Abstract
The transition from the radio to the millimeter and submillimeter ranges is very promising for studies of galactic nuclei, as well as detailed studies of processes related to supermassive black holes, wormholes, and possible manifestations of multi-element Universe (Multiverse) models. This is shown by observations with the largest interferometer available—RadioAstron observatory—that will be used for the scientific program forMillimetron observatory. Observations have also shown the promise of this range for studies of the formation and evolution of planetary systems and searches for manifestations of intelligent life. This is caused by the requirements to use a large amount of condensedmatter and energy in large-scale technological activities. This range can also be used efficiently in the organisation of optimal channels for the transmission of information.
Similar content being viewed by others
References
I. S. Shklovskii, Selected Works (Nauka, Moscow, 2009), Vol. 2 [in Russian].
L. I. Matveenko, N. S. Kardashev, and G. B. Sholomitskii, Izv. Vyssh. Uchebn. Zaved., Radiofiz. 8 (4) (1965).
V. V. Andreyanov, N. S. Kardashev, and V. V. Khartov, Cosmic Res. 52, 319 (2014).
N. S. Kardashev, V. V. Khartov, V. V. Abramov, V. Yu. Avdeev, A. V. Alakoz, Yu. A. Aleksandrov, S. Ananthakrishnan, V. V. Andreyanov, A. S. Andrianov, N. M. Antonov, M. I. Artyukhov, M. Yu. Arkhipov, W. Baan, N. G. Babakin, N. Bartel’, V. E. Babyshkin, et al., Astron. Rep. 57, 195 (2013).
N. S. Kardashev, A. V. Alakoz, A. S. Andrianov, M. I. Artyukhov, et al., Vestn. NPO im. S. A. Lavochkina, No. 3, 4 (2016).
N. S. Kardashev, I. D. Novikov, V. N. Lukash, S. V. Pilipenko, E. V. Mikheeva, D. V. Bisikalo, D. S. Wiebe, A. G. Doroshkevich, A. V. Zasov, I. I. Zinchenko, P. B. Ivanov, V. I. Kostenko, T. I. Larchenkova, S. F. Likhachev, I. F. Malov, et al., Phys. Usp. 57, 1199 (2014).
R. C. Henry, Astrophys. J. 516, 49 (1999).
B. Carr, Universe or Multiverse (Cambridge Univ. Press, Cambridge, 2007).
Y. Garriga, A. Vilenkin, and J. Zhang, J. Cosmol. Astropart. Phys., No. 2, 064 (2016).
N. S. Kardashev, PhIAS Preprint No. 65 (Lebedev Phys. Inst. Akad. Sci., Moscow, 1999).
N. S. Kardashev, I. D. Novikov, and A. A. Shatskii, Astron. Rep. 50, 601 (2006).
J. M. Stone, D. P. Marrone, C. D. Dowell, B. Schulz, C. O. Heinke, and F. Yuzef-Zadeh, Astrophys. J. 825, 32 (2016).
A. G. Doroshkevich, N. S. Kardashev, D. I. Novikov, and I. D. Novikov, Astron. Rep. 52, 616 (2008).
D. I. Novikov, A. G. Doroshkevich, I. D. Novikov, and A. A. Shatskii, Astron. Rep. 53, 1079 (2009).
A. A. Shatskii, I. D. Novikov, and N. S. Kardashev, Phys. Usp. 51, 457 (2008).
N. S. Kardashev, L. N. Lipatova, I. D. Novikov, and A. A. Shatskiy, Astron. Rep. 59, 89 (2015).
M. Y. Timofeev, N. S. Kardashev, and V. G. Promyslov, Acta Astron. 46, 655 (2000).
V. I. Slysh, in The Search for Extraterrestrial Life: Recent Developments, Ed. by M. Papagiahhis (Dordrecht, Reidell, 1985), p.315.
R. A. Carrigan, Jr., Astrohys. J. 698, 2075 (2009).
N. S. Kardashev, Nature 278, 28 (1979).
I. S. Shklovskii, Nauka i Zhizn’, No. 1, 60 (1965).
Author information
Authors and Affiliations
Corresponding author
Additional information
Original Russian Text © N.S. Kardashev, 2017, published in Astronomicheskii Zhurnal, 2017, Vol. 94, No. 4, pp. 301–307.
Based on a talk presented at the international conference “All-Wave Astronomy. Shklovskii-100” in honor of the 100th anniversary of the birthday of I.S. Shklovskii (Moscow, Russia, June 20–22, 2016). Printed by recommendation of the Scientific Organizing Committee of the conference.
Rights and permissions
About this article
Cite this article
Kardashev, N.S. RadioAstron and millimetron space observatories: Multiverse models and the search for life. Astron. Rep. 61, 310–316 (2017). https://doi.org/10.1134/S1063772917040096
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1063772917040096