Treffer 1 - 11 von 11 für Suche 'Shirke, Swarnim', Suchdauer: 0,55s Treffer weiter einschränken
  1. 1
    Constraining the Equation of State of Hybrid Stars Using Recent Information from Multidisciplinary Physics

    Constraining the Equation of State of Hybrid Stars Using Recent Information from Multidisciplinary Physics von Shirke, Swarnim, Ghosh, Suprovo, Chatterjee, Debarati

    Veröffentlicht in The Astrophysical journal

    Volltext
    Artikel

    Zu den Favoriten
    Gespeichert in:
  2. 2
    Effects of dark matter on f -mode oscillations of neutron stars

    Effects of dark matter on f -mode oscillations of neutron stars von Shirke, Swarnim, Pradhan, Bikram Keshari, Chatterjee, Debarati, Sagunski, Laura, Schaffner-Bielich, Jürgen

    Veröffentlicht in Physical review. D

    Volltext
    Artikel

    Zu den Favoriten
    Gespeichert in:
  3. 3
    R-modes as a new probe of dark matter in neutron stars

    R-modes as a new probe of dark matter in neutron stars von Shirke, Swarnim, Ghosh, Suprovo, Chatterjee, Debarati, Sagunski, Laura, Schaffner-Bielich, Jürgen


    Volltext
    Artikel

    Zu den Favoriten
    Gespeichert in:
  4. 4
    texttt{AXP4}$, a Numerical Simulator of Pulse Profiles for Binary Accreting X-ray Pulsars $-$ I: Beam Geometries

    texttt{AXP4}$, a Numerical Simulator of Pulse Profiles for Binary Accreting X-ray Pulsars $-$ I: Beam Geometries von Shirke, Parisee S, Shirke, Swarnim S

    Volltext bestellen
    Artikel

    Zu den Favoriten
    Gespeichert in:
  5. 5
    Prospects of identifying the presence of Strange Stars using Gravitational Waves from binary systems

    Prospects of identifying the presence of Strange Stars using Gravitational Waves from binary systems von Pradhan, Bikram Keshari, Shirke, Swarnim, Chatterjee, Debarati

    Volltext bestellen
    Artikel

    Zu den Favoriten
    Gespeichert in:
  6. 6
    Constraining the equation of state of hybrid stars using recent information from multidisciplinary physics

    Constraining the equation of state of hybrid stars using recent information from multidisciplinary physics von Shirke, Swarnim, Ghosh, Suprovo, Chatterjee, Debarati

    Veröffentlicht in arXiv.org

    Volltext
    Artikel

    Zu den Favoriten
    Gespeichert in:
  7. 7
    (\texttt{AXP4}\), a Numerical Simulator of Pulse Profiles for Binary Accreting X-ray Pulsars \(-\) I: Beam Geometries

    (\texttt{AXP4}\), a Numerical Simulator of Pulse Profiles for Binary Accreting X-ray Pulsars \(-\) I: Beam Geometries von Shirke, Parisee S, Shirke, Swarnim S

    Veröffentlicht in arXiv.org

    Volltext
    Artikel

    Zu den Favoriten
    Gespeichert in:
  8. 8
    Effects of Dark Matter on $f$-mode oscillations of Neutron Stars

    Effects of Dark Matter on $f$-mode oscillations of Neutron Stars von Shirke, Swarnim, Pradhan, Bikram Keshari, Chatterjee, Debarati, Sagunski, Laura, Schaffner-Bielich, Jürgen

    Volltext bestellen
    Artikel

    Zu den Favoriten
    Gespeichert in:
  9. 9
    R-modes as a New Probe of Dark Matter in Neutron Stars

    R-modes as a New Probe of Dark Matter in Neutron Stars von Shirke, Swarnim, Ghosh, Suprovo, Chatterjee, Debarati, Sagunski, Laura, Schaffner-Bielich, Jürgen

    Veröffentlicht in arXiv.org

    Volltext
    Artikel

    Zu den Favoriten
    Gespeichert in:
  10. 10
    Prospects of identifying the presence of Strange Stars using Gravitational Waves from binary systems

    Prospects of identifying the presence of Strange Stars using Gravitational Waves from binary systems von Bikram Keshari Pradhan, Shirke, Swarnim, Chatterjee, Debarati

    Veröffentlicht in arXiv.org

    Volltext
    Artikel

    Zu den Favoriten
    Gespeichert in:
  11. 11
    Effects of Dark Matter on \(f\)-mode oscillations of Neutron Stars

    Effects of Dark Matter on \(f\)-mode oscillations of Neutron Stars von Shirke, Swarnim, Bikram Keshari Pradhan, Chatterjee, Debarati, Sagunski, Laura, Schaffner-Bielich, Jürgen

    Veröffentlicht in arXiv.org

    Volltext
    Artikel

    Zu den Favoriten
    Gespeichert in:

Suchwerkzeuge: