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The anthropic principle and its implications for biological evolution
Abstract
In the form in which it was originally expounded, the anthropic principle was presented as a warning to astrophysical and cosmological theorists of the risk of error in the interpretation of astronomical and cosmological information unless due account is taken of the biological restraints under which the information was acquired. However, the converse message is also valid: biological theorists also run the risk of error in the interpretation of the evolutionary record unless they take due heed of the astrophysical restraints under which evolution took place. After an introductory discussion of the ordinary (‘weak’) anthropic principle and of its more contestable (‘strong’) analogue, a new application of the former to the problem of the evolution of terrestrial life is presented. It is shown that the evidence suggests that the evolutionary chain included at least one but probably not more than two links that were highly improbable (a priori) in the available time interval.
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“Since there are more centers in glorious-future worlds than doomsday worlds by a factor of billions, the posterior probability of the doomsday hypothesis is boosted from one in a million to close to one.”
From Multiple Universes and Self-Locating Evidence (2022) · cites this paper as Carter 1983
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Items 101–200 of 291
Ćirković, M. (2013) · doi:10.1016/j.actaastro.2013.03.012 · Cited by 16
“Carter's argument, the latest of the “Big Three,” is based on our ignorance about the characteristic temporal scales of biological evolution leading to emergence of intelligent observers [13,14].”
BackgroundTheological Implications of Possible Extraterrestrial Life
Bonting, S. J. (2003) · doi:10.1111/1467-9744.00523 · Cited by 16
Civilization's Wake: Ecology, Economics and the Roots of Environmental Destruction and Neglect
Smith, J., & Sauer-Thompson, G. (1998) · Population and Environment · doi:10.1023/a:1024616725080 · Cited by 16
Eta-Earth Revisited II: Deriving a Maximum Number of Earth-Like Habitats in the Galactic Disk
Scherf, M., Lammer, H., & Sproß, L. (2024) · Astrobiology · doi:10.1089/ast.2023.0076 · Cited by 19
False Positives and the Challenge of Testing the Alien Hypothesis
Foote, S., Sinhadc, P., Mathis, C., & Walker, S. I. (2023) · Astrobiology · doi:10.1089/ast.2023.0005 · Cited by 18
Viewing the technosphere in an interplanetary light
Szerszynski, B. (2016) · The Anthropocene Review · doi:10.1177/2053019616670676 · Cited by 17
“Carter (1983) and Watson (2008) both argue that the strictly necessary steps for intelligent observerhood are probably very few, which implies that all the other evolutionary steps that have de facto shaped the character of the Earth, of human beings and of the Earth’s technosphere (for example the…”
BackgroundToo early? on the apparent conflict of astrobiology and cosmology
Ćirković, M. (2005) · Biology & Philosophy · doi:10.1007/s10539-005-8305-2 · Cited by 15
Gaia and observer self-selection
Watson, A. (2004) · The MIT Press eBooks · doi:10.7551/mitpress/6100.003.0024 · Cited by 15
ON THE DETECTABILITY OF INTELLIGENT CIVILIZATIONS IN THE GALAXY
Djurić, N., & Field, L. (2003) · doi:10.2298/saj0367001d · Cited by 15
“Finally, an argument made by Carter (1983) is based on the similarity between the biological evolutionary time scale here on Earth and the Sun’s evolutionary time scale.”
BackgroundFriederich, S. (2021) · Cambridge University Press eBooks · doi:10.1017/9781108765947 · Cited by 35
Multiverse Predictions for Habitability: Fraction of Planets that Develop Life
Sandora, M. (2019) · Universe · doi:10.3390/universe5070171 · Cited by 11
“], we include this discussion here anyway. 3.1. Would We Live in This Universe if the Hard Step Model Is True? The first hypothesis we consider is the hard step model, originally proposed in Reference [46]. Its tenet is that the emergence of intelligence requires a small number of very hard evolutionary innovations, ea…”
BackgroundMethodInfluentialA Minimal Active Inference AgentPreprint
McGregor, S., Baltieri, M., & Buckley, C. L. (2015) · arXiv (Cornell University) · doi:10.48550/arxiv.1503.04187 · Cited by 12
Carter on Anthropic Principle Predictions
Wilson, P. (1994) · British Journal for the Philosophy of Science · doi:10.1093/bjps/45.1.241 · Cited by 14
Crawford, I., & Schulze‐Makuch, D. (2023) · Nature Astronomy · doi:10.1038/s41550-023-02134-2 · Cited by 17
Valuing Life-Detection Missions
Kite, E. S., Gaidos, E. J., & Onstott, T. C. (2018) · Astrobiology · doi:10.1089/ast.2017.1813 · Cited by 15
“It is rather unlikely that (say) * 50% are inhabited, because there is no reason for the scale of the environment needed for origin of life to be equal to the scale of a planet, even to order of magnitude (Carter, 1983; Lacki, 2016).”
Testing Anthropic Selection: A Climate Change Example
Waltham, D. (2011) · Astrobiology · doi:10.1089/ast.2010.0475 · Cited by 13
“Bayes’ theorem gives an elegant way to express the concept of anthropic selection (Carter,1983; Waltham, 2007).”
Intelligence's likelihood and evolutionary time frame
Bogonovich, M. (2011) · International Journal of Astrobiology · doi:10.1017/s147355041000042x · Cited by 13
“The step hypothesis has received attention from astrobiologists (Carter 1983; McKay 1996; Watson 2008).”
BackgroundA reassessment of the “hard-steps” model for the evolution of intelligent life
Mills, D. B., Macalady, J. L., Frank, A., & Wright, J. T. (2025) · Science Advances · doi:10.1126/sciadv.ads5698 · Cited by 14
“Like the anthropic principle itself, the hard-steps model is applicable to humans and nonhuman entities alike—notably, extraterrestrial organisms ( 1 ), as well as any organism that has existed or will exist on Earth.”
InfluentialBiosignature surveys to exoplanet yields and beyond
Sandora, M., & Silk, J. I. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa1284 · Cited by 12
“We focus here on what we expect to be a nested sequence of biosignatures, corresponding to the major evolutionary transitions that occur on Earth, as outlined in Carter (1983); Szathmáry & Smith (1995).”
BackgroundDirac's large number hypothesis: A journey from concept to implication
Ray, S., Mukhopadhyay, U., Ray, S., & Bhattacharjee, A. (2019) · International Journal of Modern Physics D · doi:10.1142/s0218271819300143 · Cited by 15
Anthropic selection and the habitability of planets orbiting M and K dwarfs
Waltham, D. (2011) · Icarus · doi:10.1016/j.icarus.2011.07.023 · Cited by 11
“characteristic timescale for the emergence of intelligence is actually much greater than 4 Gyr (Carter, 1983; Watson, 2008).”
BackgroundInfluentialHominid evolution: genetics versus memetics
Carter, B. (2010) · International Journal of Astrobiology · doi:10.1017/s1473550411000279 · Cited by 11
“The idea underlying the anthropic principle (Carter 1983; Leslie 1996; Bostrom 2002) is that to interpret what one observes when one emerges in the universe, one needs some idea of what might or might not be expected as far as one’s personal identity and situation in space and time are concerned.”
BackgroundMethodInfluentialSelf-citationObservational Selection Effects in Quantum Cosmology
Page, D. (2007) · doi:10.48550/arxiv.0712.2240 · Cited by 11
“One or more correlated steps might be highly improbable on a per-planet basis [36] (say P ∼ 10−n with n ≫ 24 so that the probability would be very low for any others within the observable universe of probably not more than 1024 planets).”
BackgroundUniverses without the weak force: Astrophysical processes with stable neutrons
Grohs, E., Howe, A. R., & Adams, F. C. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.97.043003 · Cited by 11
Dark energy from the motions of neutrinos
Simpson, F., Jimenez, R., Peña-Garay, C., & Verde, L. (2016) · Physics of the Dark Universe · doi:10.1016/j.dark.2018.04.002 · Cited by 10
Anthropic decision theoryPreprint
Armstrong, S. (2011) · arXiv.org · doi:10.48550/arxiv.1110.6437 · Cited by 10
“nder the creation of agents who don’t yet know what reference class they are in. 5.3 The Doomsday argument Closely related to the Adam and Eve paradox, though discovered rst, is the Doomsday argument [CM83]. Based on SSA’s preference for ‘smaller’ universes, it implies that there is a high probability of the human rac…”
InfluentialEllis, G. F. R. (2011) · General Relativity and Gravitation · doi:10.1007/s10714-011-1257-8 · Cited by 46
“Their version of the SAP (p.21) is essentially the same as Carter’s 1974 version.”
BackgroundInfluentialAgnesi weighting for the measure problem of cosmology
Page, D. N. (2011) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2011/03/031 · Cited by 11
“The shift of the measure (say calibrated for a fixed comoving density of observers making a constant number of observations per time) from being uniform in the time to having the weighting factors of the inverse three-volume (from the spatial density averaging) and of very nearly the inverse square of the time (from t…”
Macro-Engineering in the Galactic Context
Ćirković, M. M. (2006) · Water science and technology library · doi:10.1007/1-4020-4604-9_13 · Cited by 9
“f the Galactic age (Hart, 1975; Jones, 1976; Tipler, 1980, 1981). In this light, Fermi's legendary question: Where are they? becomes disturbingly pertinent (Brin, 1983; Webb, 2002). In addition, Carter (1983) suggested an independent and powerful anthropic argument for the uniqueness of intelligent life on Earth…”
BackgroundHuemer, M. (2018) · doi:10.1007/978-3-319-90490-0_11 · Cited by 10
The Doomsday Argument without Knowledge of Birth Rank
Monton, B. (2003) · The Philosophical Quarterly · doi:10.1111/1467-9213.00297 · Cited by 10
A Statistical Case Against Empirical Human-AI AlignmentPreprint
Rodemann, J., Arias, E. G., Luther, C., Jansen, C., & Augustin, T. (2025) · arXiv (Cornell University) · doi:10.48550/arxiv.2502.14581 · Cited by 9
“Modern-day physics is aware of such anthropocentric biases and – going even further – the more general anthropic principle, also referred to as "observation selection effect" (Bostrom, 2000; 2002; Carter, 1983).”
A Bayesian Analysis of Technological Intelligence in Land and Oceans
Lingam, M., Balbi, A., & Mahajan, S. M. (2023) · The Astrophysical Journal · doi:10.3847/1538-4357/acb6fa · Cited by 11
“If the origination of TI is encapsulated by a Poisson process (e.g., Carter 1983; Spiegel & Turner 2012; Scharf & Cronin 2016), we can introduce a uniform rate parameter λL for the emergence of TI and a “habitability interval” tL, which is the time over which TI could arise; both these parameters…”
MethodThe habitability of large elliptical galaxies
Whitmire, D. P. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa957 · Cited by 10
Area Coverage of Expanding E.T. Signals in the Galaxy: SETI and Drake’s N
Grimaldi, C., Marcy, G., Tellis, N. K., & Drake, F. (2018) · Publications of the Astronomical Society of the Pacific · doi:10.1088/1538-3873/aaac6a · Cited by 9
“That such a birthrate may be defined with an associated time interval between births has been discussed by Carter (1983) and Gott (1993) in terms of convergent evolution and the coincidence of timescales between the remaining main sequence lifetime of the Sun, the age of the Earth, and the…”
BackgroundDoes God So Love the Multiverse?
Page, D. (2008) · doi:10.1002/9781118241455.ch18 · Cited by 9
“This is generally agreed upon both by those who attempt to use this fine tuning to support theism, as in the references above, and by many scientists who are usually neutral or opposed to such an attempt [22, 23, 24, 25, 26, 27, 28, 29, 30, 31, 32, 33, 34, 35].”
BackgroundEvolutionary catastrophes and the Goldilocks problem
Ćirković, M. (2007) · International Journal of Astrobiology · doi:10.1017/s1473550407003916 · Cited by 9
“Carter (1983)). The next question we should ask is : How big does the catastrophe at each point in the history of Earth need to be in order to be consistent with the existence of intelligent observers at t=t0? Notice that the observers we are asking about here need not be us, humans, in either a morphological, phyloge…”
BackgroundMacroengineering in the Galactic Context: A New Agenda for AstrobiologyPreprint
Ćirković, M. M. (2006) · arXiv (Cornell University) · doi:10.48550/arxiv.astro-ph/0606102 · Cited by 11
“Improved epistemological and methodological understanding of our properties as intelligent observers, as well as physical, chemical and other pre-conditions necessary for the existence of such observers (Carter, 1983; Livio, 1999).”
BackgroundLivio, M., & Kopelman, A. (1990) · Nature · doi:10.1038/343025a0 · Cited by 9
Are anthropic arguments, involving multiverses and beyond, legitimate?
Stoeger, W. R. (2007) · Cambridge University Press eBooks · doi:10.1017/cbo9781107050990.027 · Cited by 8
“made a distinction between the ‘weak’ and ‘strong’ forms of the AP [4].”
Göthel, J., Corsten, A., & Volkova, O. (2025) · Next Energy · doi:10.1016/j.nxener.2025.100448 · Cited by 7
Lenton, T. M. (2025) · Philosophical Transactions of the Royal Society B Biological Sciences · doi:10.1098/rstb.2024.0095 · Cited by 9
“A suitable Bayesian null model already exists: the ‘critical steps’ model [70,71] predicts there were roughly four innately rare, contingent steps on the path to observers (us) that were roughly evenly spaced , and are argued to have involved reorganizations of the biosphere [12].”
Bayesian reasoning in eternal inflation: A solution to the measure problem
Khoury, J., & Wong, S. S. C. (2023) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.108.023506 · Cited by 15
Cellular evolution of language.
Torday, J. (2021) · Progress in Biophysics and Molecular Biology · doi:10.1016/j.pbiomolbio.2021.05.009 · Cited by 8
A Bayesian Approach to the Simulation Argument
Kipping, D. (2020) · doi:10.3390/universe6080109 · Cited by 8
Bouchard‐Côté, A., Chern, K., Čubranić, D., Hosseini, S., Hume, J., Lepur, M., Ouyang, Z., & Sgarbi, G. (2022) · Journal of Statistical Software · doi:10.18637/jss.v103.i11 · Cited by 10
“Consider the simplified Doomsday Argument (Carter and McCrea 1983) for modeling the total number of humans that were ever or will ever be born.”
BackgroundInfluentialWoodpeckers and Diamonds: Some Aspects of Evolutionary Convergence in Astrobiology
Ćirković, M. M. (2018) · Astrobiology · doi:10.1089/ast.2017.1741 · Cited by 8
“Each of the ‘‘major transitions’’ (Maynard Smith and Szathmary, 1997) or ‘‘crit-ical steps’’ (Carter, 1983) in evolution opened up huge new parts of the total morphospace—parts that without the transition in question would have been not only unreachable but perhaps inconceivable as well.”
Dirac’s Large Number Hypothesis: Is it Related to 40 Hz Gamma Oscillation or Consciousness?
Roy, S., Bhattacharya, S., & Sreekantan, B. V. (2015) · NeuroQuantology · doi:10.14704/nq.2015.13.3.847 · Cited by 5
“In this context, it is relevant to mention a very important issue raised by Carter in his paper on biological evolution (Carter, 1983) that cosmologists would run a risk of error in the”
BackgroundInfluentialThe size distribution of inhabited planets
Simpson, F. (2015) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slv170 · Cited by 9
DRAKE EQUATION FOR THE MULTIVERSE: FROM THE STRING LANDSCAPE TO COMPLEX LIFE
GLEISER, M. (2010) · International Journal of Modern Physics D · doi:10.1142/s0218271810017949 · Cited by 29
Design and the Anthropic principle
Leslie, J. (1992) · Biology & Philosophy · doi:10.1007/bf00129975 · Cited by 10
How to Predict Future Duration from Present Age
Monton, B., & Kierland, B. (2006) · doi:10.1111/j.1467-9213.2005.00426.x · Cited by 8
The impact of the cosmological constant on past and future star formation
Sorini, D., Peacock, J. A., & Lombriser, L. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae2236 · Cited by 12
Multiverse Predictions for Habitability: Planetary Characteristics
Sandora, M., Airapetian, V., Barnes, L. A., & Lewis, G. F. (2022) · Universe · doi:10.3390/universe9010002 · Cited by 5
“Alternatively, they consider that the emergence of complex life should be proportional to some greater powers of each of these quantities, if given by a sequence of hard steps, as in [116].”
Natural Intelligence and Anthropic Reasoning
Slijepčević, P. (2020) · Biosemiotics · doi:10.1007/s12304-020-09388-7 · Cited by 13
“12 the term “cognition principle” (Carter 1983) may have been less problematic than the somewhat inappropriate term AP.”
BackgroundMethodInfluentialThe fine structure constant and habitable planets
Sandora, M. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/08/048 · Cited by 7
“In fact, there is reason to believe that life necessarily takes billions of years to develop intelligence: the similarity to stellar lifetimes has been taken as evidence that this may be the minimum possible time required [44] (though see [45] for the alternative interpretation that time spent is the circumstellar hab…”
BackgroundKarl Rahner and the extra-terrestrial intelligence question
Fisher, C. L., & Fergusson, D. (2006) · The Heythrop Journal · doi:10.1111/j.1468-2265.2006.00288.x · Cited by 7
SACRED ALGORITHMS: EXCHANGE THEORY OF RELIGIOUS CLAIMS
Bainbridge, W. (2003) · Religion and the social order · doi:10.1016/s1061-5210(03)10002-3 · Cited by 7
The Precambrian Evolution of Terrestrial Life
Knoll, A. (1985) · Springer eBooks · doi:10.1007/978-94-009-5462-5_29 · Cited by 7
Substantial Extension of the Lifetime of the Terrestrial Biosphere
Graham, R. J., Halevy, I., & Abbot, D. (2024) · The Planetary Science Journal · doi:10.3847/psj/ad7856 · Cited by 6
“…late in Earth’s window of habitability and to estimate the number of critical, highly improbable steps in the evolution of intelligent life on Earth (Carter 1983; Hanson 1998a,b; Flambaum 2003; Watson 2004; Carter 2008; Watson 2008; ´Cirkovi´c et al. 2009; Aldous 2012; Bostrom 2013; Lingam & Loeb…”
Nuclear processes in other universes: Varying the strength of the weak force
Howe, A., Grohs, E., & Adams, F. (2018) · Physical Review D · doi:10.1103/physrevd.98.063014 · Cited by 6
Implication of our technological species being first and early
Whitmire, D. P. (2017) · International Journal of Astrobiology · doi:10.1017/s1473550417000271 · Cited by 9
“Our Principle of Mediocrity inference based on us being technologically early is not the same logic as the so-called Doomsday Argument (Carter & McCrea 1983; Gott 1993; Leslie 1996; Bostrom 2002), which itself is an unjustified extension of the German Tank Problem.”
InfluentialOn the Habitability of Our UniversePreprint
Loeb, A. (2016) · arXiv (Cornell University) · doi:10.48550/arxiv.1606.08926 · Cited by 4
“Our results provide a new perspective on the so-called “coincidence problem”, why do we observe Ωm ∼ ΩΛ? [261] The answer comes naturally if we consider the history of Sun-like star formation, as the number of habitable planets peaks around present time for m ∼ 1M .”
ResultThe Distribution of Stars Most Likely to Harbor Intelligent Life
Whitmire, D., & Matese, J. (2009) · Astrobiology · doi:10.1089/ast.2008.0272 · Cited by 6
“The approximate equality of T i and T for the Solar System, along with the assumption that f (T) and f i T i are independent, led Carter (1983) to conclude that intelligent life is rare in the universe.”
A difficulty for Everett's many‐worlds theory
Leslie, J. (1996) · International Studies in the Philosophy of Science · doi:10.1080/02698599608573542 · Cited by 3
Lacki, B. (2024) · Astrophysical Journal · doi:10.3847/1538-4357/ad11f2 · Cited by 5
Hyde, B. (2023) · ETHICS IN PROGRESS · doi:10.14746/eip.2023.2.9 · Cited by 5
Multiverse Predictions for Habitability: Origin of Life Scenarios
Sandora, M., Airapetian, V., Barnes, L. A., Lewis, G. F., & Pérez‐Rodríguez, I. (2023) · Universe · doi:10.3390/universe9010042 · Cited by 3
“Lastly, one may regard the origin of life as a ‘hard step’ process, whereby each step in a chain of necessary innovations is proportional to disequilibrium, leading to the concatenation of all processes being proportional to some integer [14].”
BackgroundDirected Panspermia Using Interstellar Comets
McKay, C. P., Davies, P. C. W., & Worden, S. P. (2022) · Astrobiology · doi:10.1089/ast.2021.0188 · Cited by 5
“This conclusion would fly in the face of the Principle of Mediocrity (Gott, 1993; Franck et al. , 2007), but that Principle is a purely philosophical argument, not a scientific one, and opposite philosophical positions have been taken based on the Anthropic Principle of post-selection (Carter, 1983).”
Engler, J., & von Wehrden, H. (2019) · International Journal of Astrobiology · doi:10.1017/s1473550418000496 · Cited by 5
Exploring Temporal Patterns in Big History Dynamics
LePoire, D. J. (2016) · KronoScope · doi:10.1163/15685241-12341358 · Cited by 28
The longevity of habitable planets and the development of intelligent life
Simpson, F. (2016) · International Journal of Astrobiology · doi:10.1017/s1473550416000306 · Cited by 8
Wilson, A. (2015) · The British Journal for the Philosophy of Science · doi:10.1093/bjps/axv035 · Cited by 17
“Perhaps the most well-known sources are (Carter 1983), Gott (1993), and Leslie (1989)(3).”
BackgroundDoes God So Love the Multiverse
Page, D. (2010) · doi:10.1002/9781444317350.ch29 · Cited by 5
“s is generally agreed upon both by those who attempt to use this fine tuning to support theism, as in the references above, and by many scientists who are usually neutral or opposed to such an attempt [22, 23, 24, 25, 26, 27, 28, 29, 30, 31, 32, 33, 34, 35]. Of course no one knows what other forms of life might be poss…”
BackgroundScientific and Philosophical Challenges to Theism
Page, D. N. (2010) · Wiley eBooks · doi:10.1002/9781444317350.ch30 · Cited by 6
“One rather arcane challenge that has occurred to me is the application of the Carter-Leslie-Nielsen-Gott doomsday argument [5, 6, 7, 8, 9, 10] to the afterlife.”
MethodMicro-anthropic principle for quantum theory
Carter, B. (2007) · Cambridge University Press eBooks · doi:10.1017/cbo9781107050990.021 · Cited by 6
“As a prescription for ascribing a priori probability weightings to the eventuality of finding oneself in the position of particular conceivable observers, the anthropic principle was originally developed for application to problems of cosmology [1] and biology [2].”
BackgroundInfluentialSelf-citationAnthropic Reasoning in Cosmology: A Historical Perspective
Bettini, S. (2004) · doi:10.48550/arxiv.physics/0410144 · Cited by 5
Reflection on systemic aspects of consciousness
Běinová, Z. (2023) · Neural Network World · doi:10.14311/nnw.2023.33.022 · Cited by 5
“We can consider the existence of thalamo-cortical reverberation as an accompanying phenomenon, or even as a key part of the processes of human consciousness (Faber [9, 22, 31]).”
BackgroundWebb, S. (2011) · doi:10.1007/978-3-642-13196-7_17 · Cited by 5
Tunneling as a marker of quantum mechanics (Review article)
Gabovich, A., Kuznetsov, V., & Voitenko, A. I. (2024) · Low temperature physics (Woodbury, N.Y., Print) · doi:10.1063/10.0030409 · Cited by 4
A Bayesian Analysis of the Probability of the Origin of Life Per Site Conducive to Abiogenesis
Lingam, M., Nichols, R., & Balbi, A. (2024) · Astrobiology · doi:10.1089/ast.2024.0037 · Cited by 7
Alternatives to the self-indication assumption are doomed
Adelstein, M. (2024) · Synthese · doi:10.1007/s11229-024-04686-w · Cited by 4
“Such an argument has had its fair share of defenders (e.g. Bostrom, 2013; Leslie, 2002) since its formulation by Carter (1983).”
Concepts of Existential Catastrophe
Greaves, H. (2024) · The Monist · doi:10.1093/monist/onae002 · Cited by 4
Selecting continuous life-like cellular automata for halting unpredictability
Davis, Q. T., & Bongard, J. (2022) · Genetic and Evolutionary Computation Conference Companion (GECCO Companion) · doi:10.1145/3520304.3529037
“The anthropic principle has many variants in two categories: those predicated on the universe being somehow fine-tuned to support life (famously espoused by Barrow and Tipler [1]), and the incorporation of selection bias into reasoning about the universe, described originally by Carter [4].”
BackgroundCompetitive Coherence Generates Qualia in Bacteria and Other Living Systems
Norris, V. (2021) · Biology · doi:10.3390/biology10101034 · Cited by 4
“They were here first, they occupy almost every possible niche from over a kilometre deep in the crust [100] to the upper troposphere [101], and, given the likely capacity of archaea and bacteria to survive in suspension in salt crystals for geological times [102,103], they will be here long after we are extinct [104].”
BackgroundReconfiguring SETI in the microbial context: Panspermia as a solution to Fermi's paradox
Slijepčević, P., & Wickramasinghe, C. (2021) · Biosystems · doi:10.1016/j.biosystems.2021.104441 · Cited by 7
Waltham, D. A. (2019) · Earth-Science Reviews · doi:10.1016/j.earscirev.2019.02.008 · Cited by 10
Finding a Second Sample of Life on Earth
Davies, P., & Lineweaver, C. H. (2005) · Astrobiology · doi:10.1089/ast.2005.5.154 · Cited by 88
“Estimates of the time scale for life to emerge from non-life range from a few million years (Oberbeck and Fogelman, 1989; Lazcano and Miller, 1994) up to billions of years or even longer (Carter, 1983).”
Extraterrestrial Life in the Microbial Age
Gronstal, A. (2013) · Advances in astrobiology and biogeophysics · doi:10.1007/978-3-642-35983-5_11 · Cited by 2
Abiogenesis: the Carter argument reconsidered
Whitmire, D. P. (2022) · International Journal of Astrobiology · doi:10.1017/s1473550422000350 · Cited by 4
“Although Carter fi rst presented the argument in a Bayesian framework (Carter 1983), Francis Crick had previously emphasized the same concept (1981), as acknowledged by Carter.”
InfluentialCatastrophe risk can accelerate unlikely evolutionary transitions
Snyder-Beattie, A. E., & Bonsall, M. B. (2022) · Proceedings of the Royal Society B Biological Sciences · doi:10.1098/rspb.2021.2711 · Cited by 3
“However, it is evident that these evolutionary transitions may not necessarily be independent of planetary processes, as originally hypothesized (by Carter [3]).”
BackgroundThe Drake Equation at 60: Reconsidered and Abandoned
Gertz, J. (2021) · doi:10.48550/arxiv.2105.03984 · Cited by 3
Uwagi o teistycznej interpretacji zasady antropicznej
Pabjan, T. (2019) · Studia Philosophiae Christianae · doi:10.21697/2019.55.1.04 · Cited by 5
Waltham, D. A. (2019) · Astrobiology · doi:10.1089/ast.2018.1942 · Cited by 3
“This results from a model—due to Carter and McCrea (1983)—that the probability of observers increases with t n where t is time available and n is around 3; hence a red dwarf with a main sequence lifetime 100 times greater than the Sun is one million times more likelytoproduce observers.”
The Copernican principle, intelligent extraterrestrials, and arguments from evil
Ruhmkorff, S. (2019) · Religious Studies: An International Journal for the Philosophy of Religion · doi:10.1017/s0034412518000045 · Cited by 3
Anthropic Selection of Physical Constants, Quantum Entanglement, and the Multiverse Falsifiability
Da̧browski, M. P. (2019) · Universe · doi:10.3390/universe5070172 · Cited by 3
Anthropic arguments outside of cosmology and string theory
Ćirković, M. M. (2016) · Belgrade Philosophical Annual · doi:10.5937/bpa1629091c · Cited by 20
“There are 188 confirmed impact craters on Earth at the time of this writing (February 2016).15 There is, obviously, a relationship between the size of the impactor and the size of the crater created, although the relationship is non-linear and complicated, needing to account for properties such as chemical composition…”
BackgroundInfluentialWhat do we know and what can we learn about the topology of the universe?
Uzan, J. (1997) · International Journal of Theoretical Physics · doi:10.1007/bf02768933 · Cited by 3
Quantum theory of fields and origin of gravity
Gliner, E. B. (1986) · International Journal of Theoretical Physics · doi:10.1007/bf00668784 · Cited by 2
Group Report: Long-term Geosphere–Biosphere Coevolution and Astrobiology
Lenton, T. M., Caldeira, K., Franck, S., Horneck, G., Jolly, A., Rabbow, E., Schellnhuber, H. J., Szathmáry, E., Westall, F., Zavarzin, G. A., et al. (2004) · The MIT Press eBooks · doi:10.7551/mitpress/2548.003.0008 · Cited by 1
Metadata
- Authors
- Carter, B.
- Affiliations
- Observatoire de Paris (FR)
- Corresponding author
- Carter, Brandon
- ORCID
- Carter, Brandon
- Venue
- Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences
- Publisher
- The Royal Society
- Published
- 1983-12-20
- Volume
- 310
- Issue
- 1512
- Pages
- 347-363
- ISSN
- 0080-4614 (ISSN-L)
- 2054-0272
- OpenAlex
- W2122258450
- Cited by
- 375
- References
- 14
- Citations by year
- 2026: 4 · 2025: 17 · 2024: 13 · 2023: 15 · 2022: 15 · 2021: 13 · 2020: 28 · 2019: 32 · 2018: 26 · 2017: 11 · 2016: 17 · 2015: 8 · 2014: 6 · 2013: 11 · 2012: 9
- FWCI
- 4.69
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Philosophical Transactions of the Royal Society of London Series A Mathematical and Physical Sciences (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Origins and Evolution of Life
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Physical Sciences › Environmental Science › Global and Planetary Change › Earth Systems and Cosmic Evolution
- Keywords
- anthropic principle, evolution
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