Astronomy & Astrophysics Seminar: Life of neutron stars with evolving magnetic field

Sergei B. Popov, Sternberg Astronomical Institute, Moscow State University

21 May 2025, 14:00 
Shenkar Physics Building, Holcblat Hall 007 
Astronomy & Astrophysics Seminar

Zoom: https://tau-ac-il.zoom.us/j/87185167411?pwd=FpTUyIgXaOturzOFSetA6pPVYQilen.1

 

Abstract:

In the talk, I briefly review the basics of the magnetic field evolution in neutron stars and then focus on several specific issues. At first, I discuss evidence for an episode of magnetic field decay in radio pulsars at ages ~few 10^5 yrs.  Then, I present a simple model explaining the possible existence of highly magnetized neutron stars in high-mass X-ray binaries.

 

After a brief discussion of magnetic field evolution in central compact objects, I advocate the hypothesis that the magnetic field evolution can explain anomalous braking indices of some radio pulsars and cooling neutron stars.
 

 

 

Seminar Organizer: Dr. Jonathan Stern

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