Generating tailored high frequency features in core collapse supernova gravitational wave signals applicable in LIGO interferometric studies
DOI:
https://doi.org/10.31349/RevMexFis.70.060702Keywords:
Gravitational Waves, Core-Collapse Supernovae, high frequency feature, generated waveformsAbstract
In this article, we introduce a methodology based on an analytical model of a damped harmonic oscillator subject to random forcing to generate transient gravitational wave signals. Such a model incorporates a simulated linear high-frequency component that mirrors the growing characteristic frequency over time observed in numerical simulations of core-collapse supernova gravitational wave signals. Unlike traditional numerical simulations, the method proposed in this study requires minimal computational resources, which makes it particularly advantageous for tasks such as data analysis, detection, and reconstruction of gravitational wave transients. To verify the physical accuracy of the generated signals, they are compared against the amplitude spectral of current LIGO interferometers and a 3D numerical simulation of a core-collapse supernova gravitational wave signal from the Andresen et al. 2017 model s15.nr. The results indicate that this approach is effective in generating scalable signals that align with LIGO interferometric data, offering potential utility in various gravitational wave transient investigations.
References
A. Einstein, Approximative Integration of the Field Equations of Gravitation, Sitzungsber. Preuss. Akad. Wiss. Berlin (Math. Phys.) 1916 (1916) 688
B. P. Abbott et al., GW150914: The Advanced LIGO Detectors in the Era of First Discoveries, Phys. Rev. Lett. 116 (2016) 131103, https://doi.org/10.1103/PhysRevLett.116.131103
J. Aasi et al., Advanced LIGO, Class. Quant. Grav. 32 (2015) 074001, https://doi.org/10.1088/0264-9381/32/7/074001
F. Acernese et al., Advanced Virgo: a second-generation interferometric gravitational wave detector, Class. Quant. Grav. 32 (2015) 024001, https://doi.org/10.1088/0264-9381/32/2/024001
Y. Aso et al., Interferometer design of the KAGRA grav- itational wave detector, Phys. Rev. D 88 (2013) 043007, https://doi.org/10.1103/PhysRevD.88.043007
J. Powell and B. Müller, Gravitational wave emission from 3D explosion models of core-collapse supernovae with low and normal explosion energies, Monthly Notices of the Royal Astronomical Society 487 (2019) 1178, https://doi.org/10.1093/mnras/stz1304
C. Aerts, Probing the interior physics of stars through asteroseismology, Reviews of Modern Physics 93 (2021), https://doi.org/10.1103/revmodphys.93.015001
H. Andresen et al., Gravitational wave signals from 3D neutrino hydrodynamics simulations of core-collapse supernovae, Monthly Notices of the Royal Astronomical Society 468 (2017) 2032
K. N. Yakunin et al., Gravitational wave signatures of ab initio two-dimensional core collapse supernova explosion models for 12-25 M stars, Physical Review D 92 (2015) 084040
T. Kuroda, T. Takiwaki, and K. Kotake, A new multi-energy neutrino radiation-hydrodynamics code in full general relativity and its application to the gravitational collapse of massive stars, The Astrophysical Journal Supplement Series 222 (2016) 20, https://doi.org/10.3847/0067-0049/222/2/20
J. Powell and B. Müller, Three-dimensional core-collapse supernova simulations of massive and rotating progenitors, Monthly Notices of the Royal Astronomical Society 494 (2020) 4665, https://doi.org/10.1093/mnras/staa1048
C. J. Moore, R. H. Cole, and C. P. Berry, Gravitational-wave sensitivity curves, Classical and Quantum Gravity 32 (2014) 015014
B. Müller et al., Three-dimensional simulations of neutrinodriven core-collapse supernovae from low-mass single and binary star progenitors, Monthly Notices of the Royal Astronomical Society 484 (2019) 3307, https://doi.org/10.1093/mnras/stz216
G. Handler, Asteroseismology, In Planets, Stars and Stellar Systems, pp. 207-241 (Springer Netherlands, 2013), 10. https://doi.org/10.1007%2F978-94-007-5615-1 4
T. Kuroda et al., A full general relativistic neutrino radiationhydrodynamics simulation of a collapsing very massive star and the formation of a black hole, Monthly Notices of the Royal Astronomical Society: Letters 477 (2018) L80, https://doi.org/10.1093/mnrasl/sly059
B. Müller, H.-T. Janka, and A. Marek, new multi-dimensional general relativistic neutrino hydrodynamics code for corecollapse supernovae. II. relativistic explosion models of corecollapse supernovae, The Astrophysical Journal 756 (2012) 84, https://doi.org/10.1088/0004-637x/756/1/84
B. Müller, H.-T. Janka, and A. Marek, A new multidimensional general relativistic neutrino hydrodynamics code of corecollapse supernovae. III. gravitational wave signals from supernova explosion models, The Astrophysical Journal 766 (2013) 43, https://doi.org/10.1088/0004-637x/766/1/43
B. Müller et al., Supernova simulations from a 3D progenitor model-Impact of perturbations and evolution of explosion properties, Monthly Notices of the Royal Astronomical Society 472 (2017) 491, https://doi.org/10.1093/mnras/stx1962
J. W. Murphy, C. D. Ott, and A. Burrows, A model for gravitational wave emission from neutrino-driven core-collapse supernovae, The Astrophysical Journal 707 (2009) 1173
P. Cerda-Durán et al., Gravitational wave signatures in black hole forming core collapse, The Astrophysical Journal Letters 779 (2013) L18.
B. Müller and V. Varma, A 3D simulation of a neutrino driven supernova explosion aided by convection and magnetic fields, Monthly Notices of the Royal Astronomical Society: Letters 498 (2020) L109, https://doi.org/10.1093/mnrasl/slaa137
P. Astone et al., New method to observe gravitational waves emitted by core collapse supernovae, Phys. Rev. D 98 (2018) 122002
V. Morozova et al., The gravitational wave signal from corecollapse supernovae, The Astrophysical Journal 861 (2018) 10
E. O’Connor, An open-source neutrino radiation hydrodynamics code for core-collapse supernovae, The Astrophysical Journal Supplement Series 219 (2015) 24, https://doi.org/10.1088/0067-0049/219/2/24
L. D. Landau and E. M. Lifshitz, Course of theoretical physics (Elsevier, 2013)
J. Cramer, The Origins of Logistic Regression, Working Paper 2002-119/4, Tinbergen Institute (2002)
B. P. Abbott et al., A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals, Classical and Quantum Gravity 37 (2020) 055002
A. Casallas-Lagos et al., Characterizing the temporal evolution of the high-frequency gravitational wave emission for a core collapse supernova with laser interferometric data: A neural network approach, Phys. Rev. D 108 (2023) 084027, https://doi.org/10.1103/PhysRevD.108.084027
J. V. José and E. J. Saletan, Classical Dynamics. A contemporary approach (Cambridge University Press, 1998)
K. Cannon et al., Toward early-warning detection of gravitational waves from compact binary coalescence, The Astrophysical Journal 748 (2012) 136
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Copyright (c) 2024 Claudia Moreno González, Javier M. Antelis, Cesar Tiznado, Alejandro Casallas
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