Future of Neutron Star Studies with Fast Radio Bursts

被引：2

作者：

Popov, Sergei B. ^{[1
,2
]}

Pshirkov, Maxim S. ^{[2
,3
]}

机构：

[1] ICTP Int Ctr Theoret Phys, Str Costiera 11, I-34151 Trieste, Italy

[2] Sternberg Astron Inst, Univ Pr 13, Moscow 119234, Russia

[3] Russian Acad Sci, PN Lebedev Phys Inst, Pushchino Radio Astron Observ, Pushchino 142290, Russia

来源：

PARTICLES | 2023年 / 6卷 / 01期

基金：

英国科研创新办公室;

关键词：

neutron stars; fast radio bursts; magnetic field; radio astronomy; POPULATION SYNTHESIS; WHITE-DWARFS; FRB; ACCRETION; EVOLUTION; ORIGIN;

D O I：

10.3390/particles6010025

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Fast radio bursts (FRBs) were discovered only in 2007. However, the number of known events and sources of repeating bursts grows very rapidly. In the near future, the number of events will be greater than or similar to 10(4) and the number of repeaters greater than or similar to 100. Presently, there is a consensus that most of the sources of FRBs might be neutron stars (NSs) with large magnetic fields. These objects might have different origin as suggested by studies of their host galaxies which represent a very diverse sample: from regions of very active star formation to old globular clusters. Thus, in the following decade we expect to have a very large sample of events directly related to extragalactic magnetars of different origin. This might open new possibilities to probe various aspects of NS physics. In the review we briefly discuss the main directions of such future studies and summarize our present knowledge about FRBs and their sources.

引用

页码：451 / 469

页数：19

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