Remarks on the maximum luminosity

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Remarks on the maximum luminosity. / Cardoso, Vitor; Ikeda, Taishi; Moore, Christopher J.; Yoo, Chul-Moon.

In: Physical Review D, Vol. 97, No. 8, 084013, 10.04.2018.

Research output: Contribution to journalJournal articleResearchpeer-review

Harvard

Cardoso, V, Ikeda, T, Moore, CJ & Yoo, C-M 2018, 'Remarks on the maximum luminosity', Physical Review D, vol. 97, no. 8, 084013. https://doi.org/10.1103/PhysRevD.97.084013

APA

Cardoso, V., Ikeda, T., Moore, C. J., & Yoo, C-M. (2018). Remarks on the maximum luminosity. Physical Review D, 97(8), [084013]. https://doi.org/10.1103/PhysRevD.97.084013

Vancouver

Cardoso V, Ikeda T, Moore CJ, Yoo C-M. Remarks on the maximum luminosity. Physical Review D. 2018 Apr 10;97(8). 084013. https://doi.org/10.1103/PhysRevD.97.084013

Author

Cardoso, Vitor ; Ikeda, Taishi ; Moore, Christopher J. ; Yoo, Chul-Moon. / Remarks on the maximum luminosity. In: Physical Review D. 2018 ; Vol. 97, No. 8.

Bibtex

@article{b4606e0fc7fe4a5092262b35e6508138,
title = "Remarks on the maximum luminosity",
abstract = "The quest for fundamental limitations on physical processes is old and venerable. Here, we investigate the maximum possible power, or luminosity, that any event can produce. We show, via full nonlinear simulations of Einstein's equations, that there exist initial conditions which give rise to arbitrarily large luminosities. However, the requirement that there is no past horizon in the spacetime seems to limit the luminosity to below the Planck value, L-P = c(5)/G. Numerical relativity simulations of critical collapse yield the largest luminosities observed to date, approximate to 0.2L(P). We also present an analytic solution to the Einstein equations which seems to give an unboundedly large luminosity; this will guide future numerical efforts to investigate super-Planckian luminosities.",
keywords = "EQUATIONS, EVOLUTION",
author = "Vitor Cardoso and Taishi Ikeda and Moore, {Christopher J.} and Chul-Moon Yoo",
year = "2018",
month = apr,
day = "10",
doi = "10.1103/PhysRevD.97.084013",
language = "English",
volume = "97",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "8",

}

RIS

TY - JOUR

T1 - Remarks on the maximum luminosity

AU - Cardoso, Vitor

AU - Ikeda, Taishi

AU - Moore, Christopher J.

AU - Yoo, Chul-Moon

PY - 2018/4/10

Y1 - 2018/4/10

N2 - The quest for fundamental limitations on physical processes is old and venerable. Here, we investigate the maximum possible power, or luminosity, that any event can produce. We show, via full nonlinear simulations of Einstein's equations, that there exist initial conditions which give rise to arbitrarily large luminosities. However, the requirement that there is no past horizon in the spacetime seems to limit the luminosity to below the Planck value, L-P = c(5)/G. Numerical relativity simulations of critical collapse yield the largest luminosities observed to date, approximate to 0.2L(P). We also present an analytic solution to the Einstein equations which seems to give an unboundedly large luminosity; this will guide future numerical efforts to investigate super-Planckian luminosities.

AB - The quest for fundamental limitations on physical processes is old and venerable. Here, we investigate the maximum possible power, or luminosity, that any event can produce. We show, via full nonlinear simulations of Einstein's equations, that there exist initial conditions which give rise to arbitrarily large luminosities. However, the requirement that there is no past horizon in the spacetime seems to limit the luminosity to below the Planck value, L-P = c(5)/G. Numerical relativity simulations of critical collapse yield the largest luminosities observed to date, approximate to 0.2L(P). We also present an analytic solution to the Einstein equations which seems to give an unboundedly large luminosity; this will guide future numerical efforts to investigate super-Planckian luminosities.

KW - EQUATIONS

KW - EVOLUTION

U2 - 10.1103/PhysRevD.97.084013

DO - 10.1103/PhysRevD.97.084013

M3 - Journal article

VL - 97

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 8

M1 - 084013

ER -

ID: 299202815