Effective-one-body multipolar waveform for tidally interacting binary neutron stars up to merger

Article, Preprint English OPEN
Akcay, Sarp; Bernuzzi, Sebastiano; Messina, Francesco; Nagar, Alessandro; Ortiz, Néstor; Rettegno, Piero;
(2018)
  • Publisher: HAL CCSD
  • Related identifiers: doi: 10.1103/PhysRevD.99.044051
  • Subject: General Relativity and Quantum Cosmology | gravitational radiation: emission | numerical methods | equation of state | numerical calculations | [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] | mass ratio | gravitational radiation: magnetic | General relativity | gravitational radiation | alternative theories of gravity | relativity theory | neutron star: binary | conservation law | neutron star: binary: coalescence | gravitation: self-force | Gravitational waves, waveform modeling, binary neutron stars | higher-order: 0

International audience; Gravitational-wave astronomy with coalescing binary neutron star (NS) sources requires the availability of gravitational waveforms with tidal effects accurate up to merger. This article presents an improved version of TEOBResum, a nonspinning eff... View more
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