A Dyson sphere around a black hole

Author:

Hsiao Tiger Yu-Yang1,Goto Tomotsugu1ORCID,Hashimoto Tetsuya12ORCID,Santos Daryl Joe D1ORCID,On Alvina Y L123ORCID,Kilerci-Eser Ece4ORCID,Wong Yi Hang Valerie1ORCID,Kim Seong Jin1ORCID,Wu Cossas K-W5,Ho Simon C-C1,Lu Ting-Yi1ORCID

Affiliation:

1. Institute of Astronomy, National Tsing Hua University, 101, Section 2, Kuang-Fu Road, Hsinchu 30013, Taiwan (R.O.C.)

2. Centre for Informatics and Computation in Astronomy (CICA), National Tsing Hua University, 101, Section 2, Kuang-Fu Road, Hsinchu 30013, Taiwan (R.O.C.)

3. Mullard Space Science Laboratory, University College London, Holmbury St Mary, Surrey RH5 6NT, UK

4. Faculty of Engineering and Natural Sciences, Sabancı University, 34956 Istanbul, Turkey

5. Department of Physics, National Tsing Hua University, 101, Section 2, Kuang-Fu Road, Hsinchu 30013, Taiwan (R.O.C.)

Abstract

ABSTRACT The search for extraterrestrial intelligence (SETI) has been conducted for nearly 60 yr. A Dyson sphere, a spherical structure that surrounds a star and transports its radiative energy outwards as an energy source for an advanced civilization, is one of the main targets of SETI. In this study, we discuss whether building a Dyson sphere around a black hole is effective. We consider six energy sources: (i) the cosmic microwave background, (ii) the Hawking radiation, (iii) an accretion disc, (iv) Bondi accretion, (v) a corona, and (vi) relativistic jets. To develop future civilizations (for example, a Type II civilization), $4\times 10^{26}\, {\rm W}(1\, {\rm L_{\odot }})$ is expected to be needed. Among (iii) to (vi), the largest luminosity can be collected from an accretion disc, reaching $10^{5}\, {\rm L_{\odot }}$, enough to maintain a Type II civilization. Moreover, if a Dyson sphere collects not only the electromagnetic radiation but also other types of energy (e.g. kinetic energy) from the jets, the total collected energy would be approximately 5 times larger. Considering the emission from a Dyson sphere, our results show that the Dyson sphere around a stellar-mass black hole in the Milky Way ($10\, \rm kpc$ away from us) is detectable in the ultraviolet $(\rm 10{-}400\, {\rm nm)}$, optical $(\rm 400{-}760\, {\rm nm)}$, near-infrared ($\rm 760\, {\rm nm}{-}5\, {\rm \mu m}$), and mid-infrared ($\rm 5{-}40\, {\rm \mu m}$) wavelengths via the waste heat radiation using current telescopes such as Galaxy Evolution Explorer Ultraviolet Sky Surveys. Performing model fitting to observed spectral energy distributions and measuring the variability of radial velocity may help us to identify these possible artificial structures.

Funder

Ministry of Science and Technology of Taiwan

Ministry of Science and Technology

National Tsing Hua University

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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