Simulating the magnetorotational collapse of supermassive stars: Incorporating gas pressure perturbations and different rotation profiles
| Publication Date: |
2018-11-13
|
|---|---|
| Publisher: |
American Physical Society (APS)
|
| Print ISSN: |
0556-2821
|
| Electronic ISSN: |
1089-4918
|
| Topics: |
Physics
|
| Keywords: |
Astrophysics and astroparticle physics
|
| Published by: |
| _version_ | 1836399086436089856 |
|---|---|
| autor | Lunan Sun, Milton Ruiz, and Stuart L. Shapiro |
| beschreibung | Author(s): Lunan Sun, Milton Ruiz, and Stuart L. Shapiro Collapsing supermassive stars (SMSs) with masses M ≳ 10 4 – 6 M ⊙ have long been speculated to be the seeds that can grow and become supermassive black holes (SMBHs). We previously performed general relativistic magnetohydrodynamic (GRMHD) simulations of marginally stable Γ = 4 / 3 polytropes uniformly rotatin... [Phys. Rev. D 98, 103008] Published Mon Nov 12, 2018 |
| citation_standardnr | 6356415 |
| datenlieferant | ipn_articles |
| feed_id | 52540 |
| feed_publisher | American Physical Society (APS) |
| feed_publisher_url | http://www.aps.org/ |
| insertion_date | 2018-11-13 |
| journaleissn | 1089-4918 |
| journalissn | 0556-2821 |
| publikationsjahr_anzeige | 2018 |
| publikationsjahr_facette | 2018 |
| publikationsjahr_intervall | 7984:2015-2019 |
| publikationsjahr_sort | 2018 |
| publisher | American Physical Society (APS) |
| quelle | Physical Review D |
| relation | http://link.aps.org/doi/10.1103/PhysRevD.98.103008 |
| schlagwort | Astrophysics and astroparticle physics |
| search_space | articles |
| shingle_author_1 | Lunan Sun, Milton Ruiz, and Stuart L. Shapiro |
| shingle_author_2 | Lunan Sun, Milton Ruiz, and Stuart L. Shapiro |
| shingle_author_3 | Lunan Sun, Milton Ruiz, and Stuart L. Shapiro |
| shingle_author_4 | Lunan Sun, Milton Ruiz, and Stuart L. Shapiro |
| shingle_catch_all_1 | Simulating the magnetorotational collapse of supermassive stars: Incorporating gas pressure perturbations and different rotation profiles Astrophysics and astroparticle physics Author(s): Lunan Sun, Milton Ruiz, and Stuart L. Shapiro Collapsing supermassive stars (SMSs) with masses M ≳ 10 4 – 6 M ⊙ have long been speculated to be the seeds that can grow and become supermassive black holes (SMBHs). We previously performed general relativistic magnetohydrodynamic (GRMHD) simulations of marginally stable Γ = 4 / 3 polytropes uniformly rotatin... [Phys. Rev. D 98, 103008] Published Mon Nov 12, 2018 Lunan Sun, Milton Ruiz, and Stuart L. Shapiro American Physical Society (APS) 0556-2821 05562821 1089-4918 10894918 |
| shingle_catch_all_2 | Simulating the magnetorotational collapse of supermassive stars: Incorporating gas pressure perturbations and different rotation profiles Astrophysics and astroparticle physics Author(s): Lunan Sun, Milton Ruiz, and Stuart L. Shapiro Collapsing supermassive stars (SMSs) with masses M ≳ 10 4 – 6 M ⊙ have long been speculated to be the seeds that can grow and become supermassive black holes (SMBHs). We previously performed general relativistic magnetohydrodynamic (GRMHD) simulations of marginally stable Γ = 4 / 3 polytropes uniformly rotatin... [Phys. Rev. D 98, 103008] Published Mon Nov 12, 2018 Lunan Sun, Milton Ruiz, and Stuart L. Shapiro American Physical Society (APS) 0556-2821 05562821 1089-4918 10894918 |
| shingle_catch_all_3 | Simulating the magnetorotational collapse of supermassive stars: Incorporating gas pressure perturbations and different rotation profiles Astrophysics and astroparticle physics Author(s): Lunan Sun, Milton Ruiz, and Stuart L. Shapiro Collapsing supermassive stars (SMSs) with masses M ≳ 10 4 – 6 M ⊙ have long been speculated to be the seeds that can grow and become supermassive black holes (SMBHs). We previously performed general relativistic magnetohydrodynamic (GRMHD) simulations of marginally stable Γ = 4 / 3 polytropes uniformly rotatin... [Phys. Rev. D 98, 103008] Published Mon Nov 12, 2018 Lunan Sun, Milton Ruiz, and Stuart L. Shapiro American Physical Society (APS) 0556-2821 05562821 1089-4918 10894918 |
| shingle_catch_all_4 | Simulating the magnetorotational collapse of supermassive stars: Incorporating gas pressure perturbations and different rotation profiles Astrophysics and astroparticle physics Author(s): Lunan Sun, Milton Ruiz, and Stuart L. Shapiro Collapsing supermassive stars (SMSs) with masses M ≳ 10 4 – 6 M ⊙ have long been speculated to be the seeds that can grow and become supermassive black holes (SMBHs). We previously performed general relativistic magnetohydrodynamic (GRMHD) simulations of marginally stable Γ = 4 / 3 polytropes uniformly rotatin... [Phys. Rev. D 98, 103008] Published Mon Nov 12, 2018 Lunan Sun, Milton Ruiz, and Stuart L. Shapiro American Physical Society (APS) 0556-2821 05562821 1089-4918 10894918 |
| shingle_title_1 | Simulating the magnetorotational collapse of supermassive stars: Incorporating gas pressure perturbations and different rotation profiles |
| shingle_title_2 | Simulating the magnetorotational collapse of supermassive stars: Incorporating gas pressure perturbations and different rotation profiles |
| shingle_title_3 | Simulating the magnetorotational collapse of supermassive stars: Incorporating gas pressure perturbations and different rotation profiles |
| shingle_title_4 | Simulating the magnetorotational collapse of supermassive stars: Incorporating gas pressure perturbations and different rotation profiles |
| timestamp | 2025-06-30T23:37:21.495Z |
| titel | Simulating the magnetorotational collapse of supermassive stars: Incorporating gas pressure perturbations and different rotation profiles |
| titel_suche | Simulating the magnetorotational collapse of supermassive stars: Incorporating gas pressure perturbations and different rotation profiles |
| topic | U |
| uid | ipn_articles_6356415 |