George Pappas

8 ta ish

Aristotle University of Thessaloniki

1. A New Method to Constrain Neutron Star Structure from Quasi-periodic Oscillations

   Andrea Maselli, George Pappas, Paolo Pani +4

   MaqolaOAOchiq kirish202021 iqtibos

   ABIABI:AkademIndex/2026.other.055292

2. Black hole mass and spin measurements through the relativistic precession model: XTE J1859+226

   S. Motta, T. Belloni, L. Stella +5

   MaqolaOAOchiq kirish202213 iqtibos

   ABIABI:AkademIndex/2026.other.127572

3. Can supermassive black hole shadows test the Kerr metric?

   Kostas Glampedakis, George Pappas

   MaqolaOAOchiq kirish20216 iqtibos

   ABIABI:AkademIndex/2026.other.194326

4. Post-Kerr black hole spectroscopy

   Kostas Glampedakis, George Pappas, Hector O. Silva +1

   MaqolaOAOchiq kirish20173 iqtibos

   ABIABI:AkademIndex/2026.other.107911

5. Is a black hole shadow a reliable test of the no-hair theorem?

   Kostas Glampedakis, George Pappas

   MaqolaOAOchiq kirish20233 iqtibos

   ABIABI:AkademIndex/2026.other.136469

6. Effectively Universal Behavior of Rotating Neutron Stars in General Relativity Makes Them Even Simpler than Their Newtonian Counterparts

   George Pappas, Theocharis A. Apostolatos

   MaqolaOAOchiq kirish20142 iqtibos

   ABIABI:AkademIndex/2026.other.012939

7. Revising the Multipole Moments of Numerical Spacetimes and its Consequences

   George Pappas, Theocharis A. Apostolatos

   MaqolaOAOchiq kirish20122 iqtibos

   ABIABI:AkademIndex/2026.other.012963

8. Effective no-hair relations for neutron stars and quark stars: Relativistic results

   Kent Yagi, Koutarou Kyutoku, George Pappas +2

   MaqolaOAOchiq kirish20142 iqtibos

   ABIABI:AkademIndex/2026.other.013150