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Jérôme Novak: Pulsar glitch dynamics in general relativity

Jérôme Novak: Pulsar glitch dynamics in general relativity

V četrtek, 29. marca ob 11. uri bo imel Jérôme Novak (French National Centre for Scientific Research, Pariz) Astrodebato o motnjah v vrtenju pulzarjev, do česar pride zaradi prenosa vrtilne količine med različnimi “tekočinami” znotraj nevtronskih zvezd. Predavanje bo v predavalnici P.05 v stavbi matematike na Jadranski 21 (učilnica zraven Mafije). Vljudno vabljeni!

Pulsar glitch dynamics in general relativity

Jérôme Novak
French National Centre for Scientific Research, Pariz

Pulsar glitches are commonly interpreted as angular momentum transfers occurring between two fluids present in the stellar interior, triggered by the rapid motion of superfluid vortex lines at large scales. We consider for the first time all general relativistic effects in a numerical model for glitches. First, we show numerical calculation of stationary configurations of neutron stars composed of a neutron superfluid and a fluid made of charged particles, spinning with different rotation rates. These general relativistic calculations are based on realistic equations of state accounting for entrainment effects between the fluids. These configurations are then used to build a numerical model for pulsar glitches in full general relativity.

In particular, we study in details the characteristic time scale associated with the spin-up stage, during which the stellar dynamics are governed by a mutual friction force arising from the interactions between the superfluid vortices and the surrounding fluids. Taking general relativity into account leads to an additional coupling between the fluids through frame-dragging effects and is shown to affect significantly the actual value of the spin-up time scale.

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