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AkademIndex

Xizmatlar

Nils Andersson

19 ta ish

University of Zurich

AkademScholarda batafsil koʻrsatkichlar

  1. Neutron star asteroseismology. Axial crust oscillations in the Cowling approximation

    Lars Samuelsson, Nils Andersson

    MaqolaOchiq kirish20066 iqtibos
    ABI

  2. Towards gravitational wave asteroseismology

    Nils Andersson, Kostas D. Kokkotas

    MaqolaOchiq kirish19986 iqtibos
    ABI

  3. The Einstein Telescope: a third-generation gravitational wave observatory

    M. Punturo, M. R. Abernathy, F. Acernese +97

    Maqola20106 iqtibos
    ABI

  4. Accretion in strong field gravity with eXTP

    Alessandra De Rosa, P. Uttley, Lijun Gou +97

    MaqolaOchiq kirish20185 iqtibos
    ABI

  5. Scattering of scalar waves by rotating black holes

    Kostas Glampedakis, Nils Andersson

    MaqolaOchiq kirish20015 iqtibos
    ABI

  6. Gravitational Waves and Pulsating Stars: What Can We Learn from Future Observations?

    Nils Andersson, Kostas D. Kokkotas

    MaqolaOchiq kirish19964 iqtibos
    ABI

  7. Elastic or magnetic? A toy model for global magnetar oscillations with implications for quasi-periodic oscillations during flares

    Kostas Glampedakis, Lars Samuelsson, Nils Andersson

    MaqolaOchiq kirish20064 iqtibos
    ABI

  8. A New Class of Unstable Modes of Rotating Relativistic Stars

    Nils Andersson

    MaqolaOchiq kirish19983 iqtibos
    ABI

  9. Sensitivity studies for third-generation gravitational wave observatories

    S. Hild, M. R. Abernathy, F. Acernese +97

    MaqolaOchiq kirish20113 iqtibos
    ABI

  10. Gravitational waves from pulsating stars: Evolving the perturbation equations for a relativistic star

    Gabrielle Allen, Nils Andersson, Kostas D. Kokkotas +1

    MaqolaOchiq kirish19983 iqtibos
    ABI

  11. The inverse problem for pulsating neutron stars: a 'fingerprint analysis' for the supranuclear equation of state

    Kostas D. Kokkotas, Theocharis A. Apostolatos, Nils Andersson

    MaqolaOchiq kirish20013 iqtibos
    ABI

  12. A new numerical approach to the oscillation modes of relativistic stars

    Nils Andersson, Kostas D. Kokkotas, B. F. Schutz

    MaqolaOchiq kirish19952 iqtibos
    ABI

  13. Rotational modes of relativistic stars: Numerical results

    Keith H. Lockitch, John L. Friedman, Nils Andersson

    MaqolaOchiq kirish20032 iqtibos
    ABI

  14. Crust-core coupling in rotating neutron stars

    Kostas Glampedakis, Nils Andersson

    MaqolaOchiq kirish20062 iqtibos
    ABI

  15. The Nature of Low <i>T</i> /| <i>W</i> | Dynamical Instabilities in Differentially Rotating Stars

    Anna L. Watts, Nils Andersson, D. I. Jones

    MaqolaOchiq kirish20042 iqtibos
    ABI

  16. Gravitational waves from hot young rapidly rotating neutron stars

    B. J. Owen, Lee Lindblom, Curt Cutler +3

    MaqolaOchiq kirish19982 iqtibos
    ABI

  17. Gravitational waves from instabilities in relativistic stars

    Nils Andersson

    MaqolaOchiq kirish20032 iqtibos
    ABI

  18. Rotational modes of relativistic stars: Analytic results

    Keith H. Lockitch, Nils Andersson, John L. Friedman

    MaqolaOchiq kirish20002 iqtibos
    ABI

  19. Tests of Lepton Universality Using <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mi>B</mml:mi><mml:mn>0</mml:mn></mml:msup><mml:mo stretchy="false">→</mml:mo><mml:msubsup><mml:mi>K</mml:mi><mml:mi>S</mml:mi><mml:mn>0</mml:mn></mml:msubsup><mml:msup><mml:mo>ℓ</mml:mo><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mo>ℓ</mml:mo><mml:mo>−</mml:mo></mml:msup></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mi>B</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo stretchy="false">→</mml:mo><mml:msup><mml:mi>K</mml:mi><mml:mrow><mml:mo>*</mml:mo><mml:mo>+</mml:mo></mml:mrow></mml:msup><mml:msup><mml:mo>ℓ</mml:mo><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mo>ℓ</mml:mo><mml:mo>−</mml:mo></mml:msup></mml:math> Decays

    R. Aaij, Ahmed Sameh Wagih Abdelmotteleb, Carlos Abellán Beteta +96

    Maqola20221 iqtibos
    ABI