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Title: Life versus dark energy: How an advanced civilization could resist the accelerating expansion of the universe

Abstract

We present that the presence of dark energy in our universe is causing space to expand at an accelerating rate. As a result, over the next approximately 100 billion years, all stars residing beyond the Local Group will fall beyond the cosmic horizon and become not only unobservable, but entirely inaccessible, thus limiting how much energy could one day be extracted from them. Here, we consider the likely response of a highly advanced civilization to this situation. In particular, we argue that in order to maximize its access to useable energy, a sufficiently advanced civilization would chose to expand rapidly outward, build Dyson Spheres or similar structures around encountered stars, and use the energy that is harnessed to accelerate those stars away from the approaching horizon and toward the center of the civilization. We find that such efforts will be most effective for stars with masses in the range of $$M\sim (0.2-1) M_{\odot}$$, and could lead to the harvesting of stars within a region extending out to several tens of Mpc in radius, potentially increasing the total amount of energy that is available to a future civilization by a factor of several thousand. Lastly, we also discuss the observable signatures of a civilization elsewhere in the universe that is currently in this state of stellar harvesting.

Authors:
ORCiD logo [1]
  1. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, IL (United States)
Publication Date:
Research Org.:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1462730
Alternate Identifier(s):
OSTI ID: 1637151
Report Number(s):
arXiv:1806.05203; FERMILAB-PUB-18-254-A
Journal ID: ISSN 2212-6864; 1677930; TRN: US1902209
Grant/Contract Number:  
AC02-07CH11359; FG02-13ER41958; SC0009924
Resource Type:
Accepted Manuscript
Journal Name:
Physics of the Dark Universe
Additional Journal Information:
Journal Volume: 22; Journal Issue: C; Journal ID: ISSN 2212-6864
Publisher:
Elsevier
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS

Citation Formats

Hooper, Dan. Life versus dark energy: How an advanced civilization could resist the accelerating expansion of the universe. United States: N. p., 2018. Web. doi:10.1016/j.dark.2018.09.005.
Hooper, Dan. Life versus dark energy: How an advanced civilization could resist the accelerating expansion of the universe. United States. https://doi.org/10.1016/j.dark.2018.09.005
Hooper, Dan. Thu . "Life versus dark energy: How an advanced civilization could resist the accelerating expansion of the universe". United States. https://doi.org/10.1016/j.dark.2018.09.005. https://www.osti.gov/servlets/purl/1462730.
@article{osti_1462730,
title = {Life versus dark energy: How an advanced civilization could resist the accelerating expansion of the universe},
author = {Hooper, Dan},
abstractNote = {We present that the presence of dark energy in our universe is causing space to expand at an accelerating rate. As a result, over the next approximately 100 billion years, all stars residing beyond the Local Group will fall beyond the cosmic horizon and become not only unobservable, but entirely inaccessible, thus limiting how much energy could one day be extracted from them. Here, we consider the likely response of a highly advanced civilization to this situation. In particular, we argue that in order to maximize its access to useable energy, a sufficiently advanced civilization would chose to expand rapidly outward, build Dyson Spheres or similar structures around encountered stars, and use the energy that is harnessed to accelerate those stars away from the approaching horizon and toward the center of the civilization. We find that such efforts will be most effective for stars with masses in the range of $M\sim (0.2-1) M_{\odot}$, and could lead to the harvesting of stars within a region extending out to several tens of Mpc in radius, potentially increasing the total amount of energy that is available to a future civilization by a factor of several thousand. Lastly, we also discuss the observable signatures of a civilization elsewhere in the universe that is currently in this state of stellar harvesting.},
doi = {10.1016/j.dark.2018.09.005},
journal = {Physics of the Dark Universe},
number = C,
volume = 22,
place = {United States},
year = {Thu Sep 20 00:00:00 EDT 2018},
month = {Thu Sep 20 00:00:00 EDT 2018}
}

Journal Article:

Citation Metrics:
Cited by: 2 works
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Figures / Tables:

Figure 1 Figure 1: A cartoon summarizing the prospects for an advanced civilization to transport usable stars to a central location, assuming that such efforts begin in the present epoch (t = 0). Blue, yellow and red symbols represent stars with masses of 2, 1 and 0.2$M$ , respectively. The colored linesmore » denote the (co-moving) distances those stars have travelled after 1 Gyr, 10 Gyr or 100 Gyr, adopting a maximum speed of 10% of the speed of light and assuming that approximately 100% of the collected energy is converted into kinetic energy of the star ($η$ = 1). The results shown apply to the case in which each star is encountered as it begins its main sequence evolution. The thick black line in the $t$ = 100 Gyr frame represents the horizon at that time in cosmic history. Very distant stars with either very low or high masses will not be collected, as they will either fall beyond the cosmic horizon or evolve beyond the main sequence before reaching their destination.« less

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Works referenced in this record:

Search for Artificial Stellar Sources of Infrared Radiation
journal, June 1960


The Infrared Detectability of Dyson Civilizations
journal, April 1966

  • Sagan, Carl; Walker, Russell G.
  • The Astrophysical Journal, Vol. 144
  • DOI: 10.1086/148718

Are the Dyson rings around pulsars detectable?
journal, June 2017


Searching for Exoplanets around X-Ray Binaries with Accreting White Dwarfs, Neutron Stars, and Black Holes
journal, May 2018


SETI with Gaia : The Observational Signatures of Nearly Complete Dyson Spheres
journal, July 2018

  • Zackrisson, Erik; Korn, Andreas J.; Wehrhahn, Ansgar
  • The Astrophysical Journal, Vol. 862, Issue 1
  • DOI: 10.3847/1538-4357/aac386

On the possibility of the Dyson spheres observable beyond the infrared spectrum
journal, June 2018


Possible Photometric Signatures of Moderately Advanced Civilizations: The Clarke Exobelt
journal, March 2018


Heritage of the Kepler mission: Special object KIC 8462852 and criticism of the cometary hypothesis
journal, September 2017


Some properties of the companions of KIC 8462852 (based on KEPLER data)
journal, April 2017


Life under a black sun
journal, January 2017

  • Opatrný, Tomáš; Richterek, Lukáš; Bakala, Pavel
  • American Journal of Physics, Vol. 85, Issue 1
  • DOI: 10.1119/1.4966905

Our sky now and Then: Searches for lost Stars and Impossible Effects as Probes of Advanced Extraterrestrial Civilizations
journal, September 2016

  • Villarroel, Beatriz; Imaz, Inigo; Bergstedt, Josefine
  • The Astronomical Journal, Vol. 152, Issue 3
  • DOI: 10.3847/0004-6256/152/3/76

Optical seti Observations of the Anomalous star kic 8462852
journal, June 2016


Radio seti Observations of the Anomalous star kic 8462852
journal, July 2016


On the search for artificial Dyson-like structures around pulsars
journal, August 2015


The Ĝ Search for Extraterrestrial Civilizations with Large Energy Supplies. iv. the Signatures and Information Content of Transiting Megastructures
journal, December 2015

  • Wright, Jason T.; Cartier, Kimberly M. S.; Zhao, Ming
  • The Astrophysical Journal, Vol. 816, Issue 1
  • DOI: 10.3847/0004-637X/816/1/17

Extragalactic Seti: the Tully–Fisher Relation as a Probe of Dysonian Astroengineering in disk Galaxies
journal, August 2015

  • Zackrisson, Erik; Calissendorff, Per; Asadi, Saghar
  • The Astrophysical Journal, Vol. 810, Issue 1
  • DOI: 10.1088/0004-637X/810/1/23

THE Ĝ INFRARED SEARCH FOR EXTRATERRESTRIAL CIVILIZATIONS WITH LARGE ENERGY SUPPLIES. III. THE REDDEST EXTENDED SOURCES IN WISE
journal, April 2015

  • Griffith, Roger L.; Wright, Jason T.; Maldonado, Jessica
  • The Astrophysical Journal Supplement Series, Vol. 217, Issue 2
  • DOI: 10.1088/0067-0049/217/2/25

IRAS -BASED WHOLE-SKY UPPER LIMIT ON DYSON SPHERES
journal, June 2009


A program to search for dyson spheres with the infrared space observatory
journal, May 1998


Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
journal, September 1998

  • Riess, Adam G.; Filippenko, Alexei V.; Challis, Peter
  • The Astronomical Journal, Vol. 116, Issue 3
  • DOI: 10.1086/300499

Measurements of Ω and Λ from 42 High‐Redshift Supernovae
journal, June 1999

  • Perlmutter, S.; Aldering, G.; Goldhaber, G.
  • The Astrophysical Journal, Vol. 517, Issue 2
  • DOI: 10.1086/307221

Planck 2015 results : XIII. Cosmological parameters
journal, September 2016


Life, the Universe, and Nothing: Life and Death in an Ever‐expanding Universe
journal, March 2000

  • Krauss, Lawrence M.; Starkman, Glenn D.
  • The Astrophysical Journal, Vol. 531, Issue 1
  • DOI: 10.1086/308434

Long-term future of extragalactic astronomy
journal, January 2002


Future evolution of nearby large-scale structures in a universe dominated by a cosmological constant
journal, July 2003


Future evolution of the intergalactic medium in a universe dominated by a cosmological constant
journal, October 2004


The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems
journal, January 2002


Cosmic Star-Formation History
journal, August 2014


On the mass of the Local Group
journal, September 2014

  • González, Roberto E.; Kravtsov, Andrey V.; Gnedin, Nickolay Y.
  • The Astrophysical Journal, Vol. 793, Issue 2
  • DOI: 10.1088/0004-637X/793/2/91

The Ĝ Infrared Search for Extraterrestrial Civilizations with Large Energy Supplies. ii. Framework, Strategy, and First Result
journal, August 2014


The Stellar Initial mass Function in Early-Type Galaxies from Absorption line Spectroscopy. ii. Results
journal, November 2012


Works referencing / citing this record:

Habitable Zones around Almost Extremely Spinning Black Holes (Black Sun Revisited)
journal, January 2020

  • Bakala, Pavel; Dočekal, Jan; Turoňová, Zuzana
  • The Astrophysical Journal, Vol. 889, Issue 1
  • DOI: 10.3847/1538-4357/ab5dab

Habitable zones around almost extremely spinning black holes (black sun revisited)
text, January 2020


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