Self-gravitating oscillons and new critical behavior

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Self-gravitating oscillons and new critical behavior. / Ikeda, Taishi; Yoo, Chul-Moon; Cardoso, Vitor.

In: Physical Review D, Vol. 96, No. 6, 064047, 25.09.2017.

Research output: Contribution to journalJournal articleResearchpeer-review

Harvard

Ikeda, T, Yoo, C-M & Cardoso, V 2017, 'Self-gravitating oscillons and new critical behavior', Physical Review D, vol. 96, no. 6, 064047. https://doi.org/10.1103/PhysRevD.96.064047

APA

Ikeda, T., Yoo, C-M., & Cardoso, V. (2017). Self-gravitating oscillons and new critical behavior. Physical Review D, 96(6), [064047]. https://doi.org/10.1103/PhysRevD.96.064047

Vancouver

Ikeda T, Yoo C-M, Cardoso V. Self-gravitating oscillons and new critical behavior. Physical Review D. 2017 Sep 25;96(6). 064047. https://doi.org/10.1103/PhysRevD.96.064047

Author

Ikeda, Taishi ; Yoo, Chul-Moon ; Cardoso, Vitor. / Self-gravitating oscillons and new critical behavior. In: Physical Review D. 2017 ; Vol. 96, No. 6.

Bibtex

@article{1de1a6c25d7b470d828dbca13534da2e,
title = "Self-gravitating oscillons and new critical behavior",
abstract = "The dynamical evolution of self-interacting scalars is of paramount importance in cosmological settings and can teach us about the content of Einstein's equations. In flat space, nonlinear scalar field theories can give rise to localized, nonsingular, time-dependent, long-lived solutions called {"}oscillons.{"} Here, we discuss the effects of gravity on the properties and formation of these structures, described by a scalar field with a double well potential. We show that oscillons continue to exist even when gravity is turned on, and we conjecture that there exists a sequence of critical solutions with an infinite lifetime. Our results suggest that a new type of critical behavior appears in this theory, characterized by modulations of the lifetime of the oscillon around the scaling law and the modulations of the amplitude of the critical solutions.",
keywords = "SCALAR FIELD, NUMERICAL RELATIVITY, EVOLUTION, COLLAPSE",
author = "Taishi Ikeda and Chul-Moon Yoo and Vitor Cardoso",
year = "2017",
month = sep,
day = "25",
doi = "10.1103/PhysRevD.96.064047",
language = "English",
volume = "96",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "6",

}

RIS

TY - JOUR

T1 - Self-gravitating oscillons and new critical behavior

AU - Ikeda, Taishi

AU - Yoo, Chul-Moon

AU - Cardoso, Vitor

PY - 2017/9/25

Y1 - 2017/9/25

N2 - The dynamical evolution of self-interacting scalars is of paramount importance in cosmological settings and can teach us about the content of Einstein's equations. In flat space, nonlinear scalar field theories can give rise to localized, nonsingular, time-dependent, long-lived solutions called "oscillons." Here, we discuss the effects of gravity on the properties and formation of these structures, described by a scalar field with a double well potential. We show that oscillons continue to exist even when gravity is turned on, and we conjecture that there exists a sequence of critical solutions with an infinite lifetime. Our results suggest that a new type of critical behavior appears in this theory, characterized by modulations of the lifetime of the oscillon around the scaling law and the modulations of the amplitude of the critical solutions.

AB - The dynamical evolution of self-interacting scalars is of paramount importance in cosmological settings and can teach us about the content of Einstein's equations. In flat space, nonlinear scalar field theories can give rise to localized, nonsingular, time-dependent, long-lived solutions called "oscillons." Here, we discuss the effects of gravity on the properties and formation of these structures, described by a scalar field with a double well potential. We show that oscillons continue to exist even when gravity is turned on, and we conjecture that there exists a sequence of critical solutions with an infinite lifetime. Our results suggest that a new type of critical behavior appears in this theory, characterized by modulations of the lifetime of the oscillon around the scaling law and the modulations of the amplitude of the critical solutions.

KW - SCALAR FIELD

KW - NUMERICAL RELATIVITY

KW - EVOLUTION

KW - COLLAPSE

U2 - 10.1103/PhysRevD.96.064047

DO - 10.1103/PhysRevD.96.064047

M3 - Journal article

VL - 96

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 6

M1 - 064047

ER -

ID: 299401906