6533b853fe1ef96bd12adc41

RESEARCH PRODUCT

Science case study and scientific simulations for the enhanced X-ray Timing Polarimetry mission, eXTP

A. De RosaG. F. BurgioT. Di SalvoA. DragoR. Search By Orcid La PlacaR. SerafinelliA. GambinoL. GualtieriA. MaselliM. FerociL. Search By Orcid StellaI. BombaciL. BurderiR. CampanaF. CapitanioP. CasellaA. D'aìF. D'ammandoD. De MartinoY. EvangelistaV. FerrariE. NardiniM. Search By Orcid OrlandiniL. PaccianiG. PagliaraP. PaniA. RiggioG. RodriguezA. SannaH. J. SchulzeR. TavernaF. TombesiS. Vercellone

subject

X-raymethods and techniquesdense matterSettore FIS/05 - Astronomia E AstrofisicaaccretionNeutron starBlack HoleAstronomical instrumentation

description

The X-ray astronomy mission eXTP (enhanced X-ray Timing Polarimetry) is designed to study matter under extreme conditions of density, gravity and magnetism. Primary goals are the determination of the equation of state (EoS) of matter at supranuclear density, the physics in extremely strong magnetic fields, the study of accretion in strong-field gravity (SFG) regime. Primary targets include isolated and binary neutron stars, strong magneticfield systems like magnetars, and stellar-mass and supermassive black holes. In this paper we report about key observations and simulations with eXTP on the primary objectives involving accretion under SFG regimes and determination of NS-EoS.

http://hdl.handle.net/20.500.12386/33206