Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-26T03:19:58.119Z Has data issue: false hasContentIssue false
  • English
  • Français

Dyson swarms of von Neumann probes: prospects and predictions

Published online by Cambridge University Press:  30 October 2020

Emir Haliki Open the ORCID record for Emir Haliki [Opens in a new window]
Emir Haliki*
Affiliation:
Department of Physics, Faculty of Science, Ege University, PO Box 35040, Izmir, Turkey
*
Author for correspondence: Emir Haliki, E-mail: [email protected]
Get access Rights & Permissions [Opens in a new window]

Abstract

According to the Kardashev scale, possible Type-II and above civilizations could use energy sources of the universe in different ways. Self-replicator von Neumann probes believed to invade any galaxies in various studies could also have uses for gaining energy, in which Dyson swarm structures are likely to consist of probes that could emit energy from any luminous celestial object is to be considered first. On addressing some possible dynamical properties of probes, the study has examined in which size and populations they could enfold a star and how they could have observational evidences according to relevant star's energy output. On the basis of our solar system, it has also been shown using a weighted-directed network structure what kind of population and route they could have in case of spreading to the nearest-neighbouring stars.

Keywords

Dyson swarmextraterrestrial intelligenceKardashev scalemilling motionnetworksVon Neumann probes
Type
Research Article
Information
International Journal of Astrobiology , Volume 19 , Issue 6 , December 2020 , pp. 474 - 481
Check for updates
Copyright
Copyright © The Author(s), 2020. Published by Cambridge University Press

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Akpinar, O, Haliki, E, Ucar, FB and Haliki Uztan, A (2014) Star network analysis of sequence based identified Yarrowia lipolytica strains. Turkish Journal of Biochemistry 39, 78.CrossRefGoogle Scholar
Alkemade, F and Castaldi, C (2005) Strategies for the diffusion of innovations on social networks. Computational Economics 25, 3.CrossRefGoogle Scholar
Bedin, LR, King, IR, Anderson, J, Piotto, G, Salaris, M, Cassisi, S and Serenelli, A (2008) Reaching the end of the white dwarf cooling sequence in NGC 6791. The Astrophysical Journal 678, 1279.CrossRefGoogle Scholar
Bodman, EH and Quillen, A (2016) KIC 8462852: transit of a large comet family. The Astrophysical Journal Letters 819, L34.CrossRefGoogle Scholar
Burns, JA (1976) Elementary derivation of the perturbation equations of celestial mechanics. American Journal of Physics 44, 944.10.1119/1.10237CrossRefGoogle Scholar
Carrigan, RA Jr (2009) IRAS-based whole-sky upper limit on Dyson spheres. The Astrophysical Journal 698, 2075.10.1088/0004-637X/698/2/2075CrossRefGoogle Scholar
DeBiase, MRL and Enterprises, D (2008) Effects of collisions upon a partial Dyson sphere. Earth 10, 10.Google Scholar
Diaz, FRC (2000) The VASIMR rocket. Scientific American 283, 90.CrossRefGoogle Scholar
Dyson, FJ (1960) Search for artificial stellar sources of infrared radiation. Science 131, 1667.CrossRefGoogle ScholarPubMed
Forgan, DH (2019) Predator-prey behaviour in self-replicating interstellar probes. International Journal of Astrobiology 18, 552.CrossRefGoogle Scholar
Gago, S, Hurajová, J and Madaras, T (2012) Notes on the betweenness centrality of a graph. Mathematica Slovaca 62, 1.CrossRefGoogle Scholar
Haliki, E (2019) Broadcast network model of pulsars as beacons of extraterrestrial civilizations. International Journal of Astrobiology 18, 455.CrossRefGoogle Scholar
Harrop, BL and Schulze-Makuch, D (2010) The solar wind power satellite as an alternative to a traditional Dyson sphere and its implications for remote detection. International Journal of Astrobiology 9, 89.CrossRefGoogle Scholar
Herbst, E (2001) The chemistry of interstellar space. Chemical Society Reviews 30, 168.CrossRefGoogle Scholar
Inoue, M and Yokoo, H (2011) Type III Dyson sphere of highly advanced civilizations around a super massive black hole. Journal of the British Interplanetary Society 64, 58.Google Scholar
Kardashev, NS (1964) Transmission of information by extraterrestrial civilizations. Soviet Astronomy 8, 217.Google Scholar
Kessler, DJ, Johnson, NL, Liou, JC and Matney, M (2010) The Kessler syndrome: implications to future space operations. Advances in the Astronautical Sciences 137, 2010.Google Scholar
Kolon, C and Schwartz, IB (2018) The dynamics of interacting swarms. arXiv. 1803.08817v1.Google Scholar
Lasota, JP, Gourgoulhon, E, Abramowicz, M, Tchekhovskoy, A and Narayan, R (2014) Extracting black-hole rotational energy: the generalized Penrose process. Physical Review D 89, 024041.CrossRefGoogle Scholar
Li, W (2015) Collective motion of swarming agents evolving on a sphere manifold: a fundamental framework and characterization. Scientific Reports 5, 13603.10.1038/srep13603CrossRefGoogle ScholarPubMed
Lingam, M (2016) Interstellar travel and galactic colonization: insights from percolation theory and the yule process. Astrobiology 16, 418.10.1089/ast.2015.1411CrossRefGoogle ScholarPubMed
Lukeman, R, Li, YX and Edelstein-Keshet, L (2009) A conceptual model for milling formations in biological aggregates. Bulletin of Mathematical Biology 71, 352.10.1007/s11538-008-9365-7CrossRefGoogle ScholarPubMed
Osmanov, Z (2019) On the interstellar Von Neumann micro self-reproducing probes. International Journal of Astrobiology (published online).Google Scholar
Osmanov, Z (2020) On a spectral pattern of the Von-Neumann probes. arXiv. 2007.00693v3.Google Scholar
Osmanov, Z and Berezhiani, VI (2018) On the possibility of the Dyson spheres observable beyond the infrared spectrum. International Journal of Astrobiology 17, 356.CrossRefGoogle Scholar
Osmanov, Z and Berezhiani, VI (2019) Anomalous variability of Dyson megastructures. Journal of the British Interplanetary Society 72, 254.Google Scholar
Schuetz, M, Vakoch, DA, Shostak, S and Richards, J (2016) Optical SETI observations of the anomalous star KIC 8462852. The Astrophysical Journal Letters 825, L5.CrossRefGoogle Scholar
Schumm, P, Scoglio, C, Gruenbacher, D and Easton, T (2007) Epidemic spreading on weighted contact networks. 2nd Bio-Inspired Models of Network, Information and Computing Systems IEEE, 201.Google Scholar
Sguera, V, Bassani, L, Landi, R, Bazzano, A, Bird, AJ, Dean, AJ, Malizia, A, Masetti, N and Ubertini, P (2008) INTEGRAL and Swift/XRT observations of the SFXT IGR J16479–4514: from quiescence to fast flaring activity. Astronomy & Astrophysics 487, 619.CrossRefGoogle Scholar
Shaw, E, Tudor, V and Winkworth, D (2012) A4_3 habitable Dyson sphere. Physics Special Topics 11, 1.Google Scholar
Stickland, DJ and Lloyd, C (2000) The strange case of theta 1 Orionis. The Observatory 120, 141.Google Scholar
Vandermeer, J (2010) How populations grow: the exponential and logistic equations. Nature Education Knowledge 3, 15.Google Scholar
Von Neumann, J (1966) Theory of Self-Reproducing Automata, 1st Edn. Urbana: University of Illinois Press, p. 388.Google Scholar
Wiley, KB (2011) The Fermi paradox, self-replicating probes, and the interstellar transportation bandwidth. arXiv. 1111.6131.Google Scholar
Witkowski, O and Ikegami, T (2016) Emergence of swarming behavior: foraging agents evolve collective motion based on signaling. PloS One 11, e0152756.CrossRefGoogle ScholarPubMed
Wright, JT (2020) Dyson spheres. Serbian Astronomical Journal 200, 1.CrossRefGoogle Scholar
Zackrisson, E, Korn, AJ, Wehrhahn, A and Reiter, J (2018) SETI with Gaia: the observational signatures of nearly complete Dyson spheres. The Astrophysical Journal 862, 21.CrossRefGoogle Scholar