The Physics of Accretion Onto Highly Magnetized Neutron Stars

Wolff, Michael T ; Becker, Peter A ; Fürst, Felix ; Guillot, Sebastien ; Harding, Alice K ; Pottschmidt, Katja ; Hemphill, Paul B ; Jaisawal, Gaurava K ; Bissinger né Kühnel, Matthias ; Malacaria, Christian(National Space Science and Technology Center, Huntsville, AL, United States)

关键词: NEUTRON STARS;    HIGH TEMPERATURE PLASMAS;    BINARY STARS;    MAGNETIC PROPERTIES;    MAGNETIC FIELDS;    MAGNETIC MEASUREMENT;    LUMINOSITY;    CYCLOTRON RESONANCE;    SCATTERING FUNCTIONS;   

RP-ID  :  GSFC-E-DAA-TN66958

学科分类：天体物理学

美国|英语

来源: NASA Technical Reports Server

【 摘 要 】

Studying the physical processes occurring in the region just above the magnetic polesof strongly magnetized, accreting binary neutron stars is essential to our understanding of stellarand binary system evolution. Perhaps more importantly, it provides us with a natural laboratoryfor studying the physics of high temperature and density plasmas exposed to extreme radiation,gravitational, and magnetic fields. Observations over the past decade have shed new light on themanner in which plasma falling at near the speed of light onto a neutron star surface is halted. Recentadvances in modeling these processes have resulted in direct measurement of the magnetic fieldsand plasma properties. On the other hand, numerous physical processes have been identified thatchallenge our current picture of how the accretion process onto neutron stars works. Observationand theory are our essential tools in this regime because the extreme conditions cannot be duplicatedon Earth. This white paper gives an overview of the current theory, the outstanding theoreticaland observational challenges, and the importance of addressing them in contemporary astrophysicsresearch.