Occurrence of Gravitational Collapse in the Accreting Neutron Stars of Binary-driven Hypernovae

Becerra, Laura M.; Cipolletta, F.; Fryer, C. L.; Menezes, Débora P.; Providência, Constança; Rueda, J. A.; Ruffini, R.

doi:10.3847/1538-4357/ad82ea

Title: Occurrence of Gravitational Collapse in the Accreting Neutron Stars of Binary-driven Hypernovae

Journal Article · 14 November 2024 · The Astrophysical Journal

DOI: https://doi.org/10.3847/1538-4357/ad82ea · OSTI ID:2481568

Becerra, Laura M. ^[1];

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^[5];

^[6];

^[7]

Universidad Mayor, Santiago (Chile); IICRANet, Pescara (Italy)
Barcelona Supercomputing Center (BSC) (Spain)
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Universidade Federal de Santa Catarina (UFSC), Florianopolis, SC (Brazil)
University of Coimbra (Portugal)
IICRANet, Pescara (Italy); Sapienza Università di Roma (Italy); Univ. degli Studi di Ferrara (Italy); Istituto Nazionale di Astrofisica (INAF), Roma (Italy)
IICRANet, Pescara (Italy); Sapienza Università di Roma (Italy); Istituto Nazionale di Astrofisica (INAF), Roma (Italy)

The binary-driven hypernova (BdHN) model proposes long gamma-ray bursts (GRBs) originate in binaries composed of a carbon–oxygen (CO) star and a neutron star (NS) companion. The CO core collapse generates a newborn NS and a supernova that triggers the GRB by accreting onto the NSs, rapidly transferring mass and angular momentum to them. This article aims to determine the conditions under which a black hole (BH) forms from NS collapse induced by the accretion and the impact on the GRB's observational properties and taxonomy. We perform three-dimensional, smoothed particle hydrodynamics simulations of BdHNe using up-to-date NS nuclear equations of state, with and without hyperons, and calculate the structure evolution in full general relativity. We assess the binary parameters leading either NS in the binary to the critical mass for gravitational collapse into a BH and its occurrence time, t_col. We include a nonzero angular momentum of the NSs and find that t_col ranges from a few tens of seconds to hours for decreasing NS initial angular momentum values. BdHNe I are the most compact (about 5 minute orbital period), promptly form a BH, and release ≳10⁵² erg of energy. They form NS–BH binaries with tens of kiloyears merger timescales by gravitational-wave emission. BdHNe II and III do not form BHs, and release ~10⁵⁰–10⁵² erg and ≲10⁵⁰ erg of energy, respectively. They form NS–NS binaries with a range of merger timescales larger than for NS–BH binaries. In some compact BdHNe II, either NS can become supramassive, i.e., above the critical mass of a nonrotating NS. Magnetic braking by a 10¹³ G field can delay BH formation, leading to BH–BH or NS–BH with tens of kiloyears merger timescales.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE Laboratory Directed Research and Development (LDRD) Program; USDOE National Nuclear Security Administration (NNSA); National Council for Scientific and Technological Development (CNPq)

Grant/Contract Number:: 89233218CNA000001

OSTI ID:: 2481568

Report Number(s):: LA-UR--23-33421

Journal Information:: The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 1 Vol. 976; ISSN 0004-637X

Publisher:: IOP PublishingCopyright Statement

Country of Publication:: United States

Language:: English

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ON THE CLASSIFICATION OF GRBs AND THEIR OCCURRENCE RATES Ruffini, R.; Rueda, J. A.; Muccino, M. The Astrophysical Journal, Vol. 832, Issue 2 https://doi.org/10.3847/0004-637X/832/2/136	journal	November 2016
On the Induced Gravitational Collapse Scenario of Gamma-Ray Bursts Associated with Supernovae Becerra, L.; Bianco, C. L.; Fryer, C. L. The Astrophysical Journal, Vol. 833, Issue 1 https://doi.org/10.3847/1538-4357/833/1/107	journal	December 2016
Neutrino Oscillations within the Induced Gravitational Collapse Paradigm of Long Gamma-Ray Bursts Becerra, L.; Guzzo, M. M.; Rossi-Torres, F. The Astrophysical Journal, Vol. 852, Issue 2 https://doi.org/10.3847/1538-4357/aaa296	journal	January 2018
Parameterizing the Supernova Engine and Its Effect on Remnants and Basic Yields Fryer, Chris L.; Andrews, Sydney; Even, Wesley The Astrophysical Journal, Vol. 856, Issue 1 https://doi.org/10.3847/1538-4357/aaaf6f	journal	March 2018
Effects of Fallback Accretion on Protomagnetar Outflows in Gamma-Ray Bursts and Superluminous Supernovae Metzger, Brian D.; Beniamini, Paz; Giannios, Dimitrios The Astrophysical Journal, Vol. 857, Issue 2 https://doi.org/10.3847/1538-4357/aab70c	journal	April 2018
On the Rate and on the Gravitational Wave Emission of Short and Long GRBs Ruffini, R.; Rodriguez, J.; Muccino, M. The Astrophysical Journal, Vol. 859, Issue 1 https://doi.org/10.3847/1538-4357/aabee4	journal	May 2018
SPH Simulations of the Induced Gravitational Collapse Scenario of Long Gamma-Ray Bursts Associated with Supernovae Becerra, L.; Ellinger, C. L.; Fryer, C. L. The Astrophysical Journal, Vol. 871, Issue 1 https://doi.org/10.3847/1538-4357/aaf6b3	journal	January 2019
On the GeV Emission of the Type I BdHN GRB 130427A Ruffini, R.; Moradi, R.; Rueda, J. A. The Astrophysical Journal, Vol. 886, Issue 2 https://doi.org/10.3847/1538-4357/ab4ce6	journal	November 2019
Bayesian Inference of Dense Matter Equation of State within Relativistic Mean Field Models Using Astrophysical Measurements Traversi, Silvia; Char, Prasanta; Pagliara, Giuseppe The Astrophysical Journal, Vol. 897, Issue 2 https://doi.org/10.3847/1538-4357/ab99c1	journal	July 2020
The Red Supergiant Binary Fraction of the Large Magellanic Cloud Neugent, Kathryn F.; Levesque, Emily M.; Massey, Philip The Astrophysical Journal, Vol. 900, Issue 2 https://doi.org/10.3847/1538-4357/ababaa	journal	September 2020
Relativistic Description of Dense Matter Equation of State and Compatibility with Neutron Star Observables: A Bayesian Approach Malik, Tuhin; Ferreira, Márcio; Agrawal, B. K. The Astrophysical Journal, Vol. 930, Issue 1 https://doi.org/10.3847/1538-4357/ac5d3c	journal	April 2022
GRB 190829A—A Showcase of Binary Late Evolution Wang, Yu; Rueda, J. A.; Ruffini, R. The Astrophysical Journal, Vol. 936, Issue 2 https://doi.org/10.3847/1538-4357/ac7da3	journal	September 2022
On the Nature of the Mass-gap Object in the GW190814 Event Lopes, Luiz L.; Menezes, Debora P. The Astrophysical Journal, Vol. 936, Issue 1 https://doi.org/10.3847/1538-4357/ac81c4	journal	August 2022
The Quest for New Correlations in the Realm of the Gamma-Ray Burst—Supernova Connection Dainotti, M. G.; Simone, B. De; Islam, K. M. The Astrophysical Journal, Vol. 938, Issue 1 https://doi.org/10.3847/1538-4357/ac8b77	journal	October 2022
On the Mass Function of GWTC-2 Binary Black Hole Systems and Their Progenitors Park, Hye-Jin; Kim, Shin-Jeong; Kim, Shinna The Astrophysical Journal, Vol. 938, Issue 1 https://doi.org/10.3847/1538-4357/ac9300	journal	October 2022
On the X-Ray, Optical, and Radio Afterglows of the BdHN I GRB 180720B Generated by Synchrotron Emission Rueda, J. A.; Li, Liang; Moradi, R. The Astrophysical Journal, Vol. 939, Issue 2 https://doi.org/10.3847/1538-4357/ac94c9	journal	November 2022
Astrophysical Implications on Hyperon Couplings and Hyperon Star Properties with Relativistic Equations of States Sun, Xiangdong; Miao, Zhiqiang; Sun, Baoyuan The Astrophysical Journal, Vol. 942, Issue 1 https://doi.org/10.3847/1538-4357/ac9d9a	journal	January 2023
GRB 171205A: Hypernova and Newborn Neutron Star Wang, Yu; Becerra, L. M.; Fryer, C. L. The Astrophysical Journal, Vol. 945, Issue 2 https://doi.org/10.3847/1538-4357/acb771	journal	March 2023
Exploring the Observability of Surviving Companions of Stripped-envelope Supernovae: A Case Study of Type Ic SN 2020oi Chen 陳, Hsin-Pei 昕霈; Rau 饒, Shiau-Jie 孝節; Pan 潘, Kuo-Chuan 國全 The Astrophysical Journal, Vol. 949, Issue 2 https://doi.org/10.3847/1538-4357/acc9af	journal	June 2023
Long-duration Gamma-Ray Burst Progenitors and Magnetar Formation Song, Cui-Ying; Liu, Tong The Astrophysical Journal, Vol. 952, Issue 2 https://doi.org/10.3847/1538-4357/acd6ee	journal	July 2023
GRB-SN Association within the Binary-driven Hypernova Model Aimuratov, Y.; Becerra, L. M.; Bianco, C. L. The Astrophysical Journal, Vol. 955, Issue 2 https://doi.org/10.3847/1538-4357/ace721	journal	September 2023
Probing Electromagnetic Gravitational-wave Emission Coincidence in a Type I Binary-driven Hypernova Family of Long Gamma-Ray Bursts at Very High Redshift Bianco, C. L.; Mirtorabi, M. T.; Moradi, R. The Astrophysical Journal, Vol. 966, Issue 2 https://doi.org/10.3847/1538-4357/ad2fa9	journal	May 2024
A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation Riley, T. E.; Watts, A. L.; Bogdanov, S. The Astrophysical Journal, Vol. 887, Issue 1 https://doi.org/10.3847/2041-8213/ab481c	journal	December 2019
PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter Miller, M. C.; Lamb, F. K.; Dittmann, A. J. The Astrophysical Journal, Vol. 887, Issue 1 https://doi.org/10.3847/2041-8213/ab50c5	journal	December 2019
GW190814: Gravitational Waves from the Coalescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object Abbott, R.; Abbott, T. D.; Abraham, S. The Astrophysical Journal, Vol. 896, Issue 2 https://doi.org/10.3847/2041-8213/ab960f	journal	June 2020
Refined Mass and Geometric Measurements of the High-mass PSR J0740+6620 Fonseca, E.; Cromartie, H. T.; Pennucci, T. T. The Astrophysical Journal Letters, Vol. 915, Issue 1 https://doi.org/10.3847/2041-8213/ac03b8	journal	July 2021
The Radius of PSR J0740+6620 from NICER and XMM-Newton Data Miller, M. C.; Lamb, F. K.; Dittmann, A. J. The Astrophysical Journal Letters, Vol. 918, Issue 2 https://doi.org/10.3847/2041-8213/ac089b	journal	September 2021
A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy Riley, Thomas E.; Watts, Anna L.; Ray, Paul S. The Astrophysical Journal Letters, Vol. 918, Issue 2 https://doi.org/10.3847/2041-8213/ac0a81	journal	September 2021
The Candidate Progenitor Companion Star of the Type Ib/c SN 2013ge Fox, Ori D.; Van Dyk, Schuyler D.; Williams, Benjamin F. The Astrophysical Journal Letters, Vol. 929, Issue 1 https://doi.org/10.3847/2041-8213/ac5890	journal	April 2022
PSR J0952−0607: The Fastest and Heaviest Known Galactic Neutron Star Romani, Roger W.; Kandel, D.; Filippenko, Alexei V. The Astrophysical Journal Letters, Vol. 934, Issue 2 https://doi.org/10.3847/2041-8213/ac8007	journal	July 2022
Magnetar Central Engines in Gamma-Ray Bursts Follow the Universal Relation of Accreting Magnetic Stars Dall’Osso, Simone; Stratta, Giulia; Perna, Rosalba The Astrophysical Journal Letters, Vol. 949, Issue 2 https://doi.org/10.3847/2041-8213/acccec	journal	June 2023
SN 2022jli: A Type Ic Supernova with Periodic Modulation of Its Light Curve and an Unusually Long Rise Moore, T.; Smartt, S. J.; Nicholl, M. The Astrophysical Journal Letters, Vol. 956, Issue 1 https://doi.org/10.3847/2041-8213/acfc25	journal	October 2023

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