These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.


BIOMARKERS

Molecular Biopsy of Human Tumors

- a resource for Precision Medicine *

196 related articles for article (PubMed ID: 29225510)

  • 1. Rotating stars in relativity.
    Paschalidis V; Stergioulas N
    Living Rev Relativ; 2017; 20(1):7. PubMed ID: 29225510
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Rotating Stars in Relativity.
    Stergioulas N
    Living Rev Relativ; 2003; 6(1):3. PubMed ID: 28179861
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Rotating Stars in Relativity.
    Stergioulas N
    Living Rev Relativ; 1998; 1(1):8. PubMed ID: 28191831
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Fast Rotating Relativistic Stars: Spectra and Stability without Approximation.
    Krüger CJ; Kokkotas KD
    Phys Rev Lett; 2020 Sep; 125(11):111106. PubMed ID: 32975993
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Tidal Love numbers of neutron stars in
    Yazadjiev SS; Doneva DD; Kokkotas KD
    Eur Phys J C Part Fields; 2018; 78(10):818. PubMed ID: 30524193
    [TBL] [Abstract][Full Text] [Related]  

  • 6. Quasi-Normal Modes of Stars and Black Holes.
    Kokkotas KD; Schmidt BG
    Living Rev Relativ; 1999; 2(1):2. PubMed ID: 28191830
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Effectively universal behavior of rotating neutron stars in general relativity makes them even simpler than their Newtonian counterparts.
    Pappas G; Apostolatos TA
    Phys Rev Lett; 2014 Mar; 112(12):121101. PubMed ID: 24724643
    [TBL] [Abstract][Full Text] [Related]  

  • 8. Instability windows and evolution of rapidly rotating neutron stars.
    Gusakov ME; Chugunov AI; Kantor EM
    Phys Rev Lett; 2014 Apr; 112(15):151101. PubMed ID: 24785021
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Magnetohydrodynamic Simulations of Self-Consistent Rotating Neutron Stars with Mixed Poloidal and Toroidal Magnetic Fields.
    Tsokaros A; Ruiz M; Shapiro SL; Uryū K
    Phys Rev Lett; 2022 Feb; 128(6):061101. PubMed ID: 35213191
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Millisecond pulsars with r-modes as steady gravitational radiators.
    Reisenegger A; Bonacić A
    Phys Rev Lett; 2003 Nov; 91(20):201103. PubMed ID: 14683350
    [TBL] [Abstract][Full Text] [Related]  

  • 11. New Class of Quasinormal Modes of Neutron Stars in Scalar-Tensor Gravity.
    Mendes RFP; Ortiz N
    Phys Rev Lett; 2018 May; 120(20):201104. PubMed ID: 29864365
    [TBL] [Abstract][Full Text] [Related]  

  • 12. Multimessenger Binary Mergers Containing Neutron Stars: Gravitational Waves, Jets, and
    Ruiz M; Shapiro SL; Tsokaros A
    Front Astron Space Sci; 2021; 8():. PubMed ID: 34651021
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Formation of supermassive black holes through fragmentation of torodial supermassive stars.
    Zink B; Stergioulas N; Hawke I; Ott CD; Schnetter E; Müller E
    Phys Rev Lett; 2006 Apr; 96(16):161101. PubMed ID: 16712210
    [TBL] [Abstract][Full Text] [Related]  

  • 14. Gravitational wave content and stability of uniformly, rotating, triaxial neutron stars in general relativity.
    Tsokaros A; Ruiz M; Paschalidis V; Shapiro SL; Baiotti L; Uryū K
    Phys Rev D; 2017 Jun; 95(12):. PubMed ID: 29888340
    [TBL] [Abstract][Full Text] [Related]  

  • 15. On the Maximum Mass of Differentially Rotating Neutron Stars.
    Baumgarte TW; Shapiro SL; Shibata M
    Astrophys J; 2000 Jan; 528(1):L29-L32. PubMed ID: 10587488
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Collapse of magnetized hypermassive neutron stars in general relativity.
    Duez MD; Liu YT; Shapiro SL; Shibata M; Stephens BC
    Phys Rev Lett; 2006 Jan; 96(3):031101. PubMed ID: 16486677
    [TBL] [Abstract][Full Text] [Related]  

  • 17. 3D collapse of rotating stellar iron cores in general relativity including deleptonization and a nuclear equation of state.
    Ott CD; Dimmelmeier H; Marek A; Janka HT; Hawke I; Zink B; Schnetter E
    Phys Rev Lett; 2007 Jun; 98(26):261101. PubMed ID: 17678077
    [TBL] [Abstract][Full Text] [Related]  

  • 18. The first 5 years of gravitational-wave astrophysics.
    Vitale S
    Science; 2021 Jun; 372(6546):. PubMed ID: 34083462
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Dynamically Stable Ergostars Exist: General Relativistic Models and Simulations.
    Tsokaros A; Ruiz M; Sun L; Shapiro SL; Uryū K
    Phys Rev Lett; 2019 Dec; 123(23):231103. PubMed ID: 31868499
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Nonlinear r-modes in rapidly rotating relativistic stars.
    Stergioulas N; Font JA
    Phys Rev Lett; 2001 Feb; 86(7):1148-51. PubMed ID: 11178031
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 10.