2018
DOI: 10.1007/s12036-017-9499-9
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Collapsing supra-massive magnetars: FRBs, the repeating FRB121102 and GRBs

Abstract: Fast radio bursts (FRBs) last for ∼ few milli-seconds and, hence, are likely to arise from the gravitational collapse of supra-massive, spinning neutron stars after they lose the centrifugal support (Falcke & Rezzolla 2014). In this paper, we provide arguments to show that the repeating burst, FRB 121102, can also be modeled in the collapse framework provided the supra-massive object implodes either into a Kerr black hole surrounded by highly magnetized plasma or into a strange quark star. Since the estimated … Show more

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Cited by 20 publications
(16 citation statements)
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“…A repeating FRB could be produced when a KBH surrounded by highly magnetized plasma interacts with an AGN (Das Gupta and Saini, 2017). Episodic winds from the AGN may prompt the KBH to intermittently accrete matter.…”
Section: Kerr Black Hole Interacting With Agnmentioning
confidence: 99%
“…A repeating FRB could be produced when a KBH surrounded by highly magnetized plasma interacts with an AGN (Das Gupta and Saini, 2017). Episodic winds from the AGN may prompt the KBH to intermittently accrete matter.…”
Section: Kerr Black Hole Interacting With Agnmentioning
confidence: 99%
“…with = 0. The deceleration parameter 0 has been analytically determined on the premise that expansion of the universe and the tired light phenomena are jointly responsible for the observed redshift, especially in the limit of very low redshift [36]. One could see it as if the tired light effect is superimposed on the Einstein de Sitter's matter only universe rather than the cosmological constant [37].…”
Section: Evolutionary Constants Modelmentioning
confidence: 99%
“…It seems to be a low-luminosity AGN or other kind of unknown peculiar source [89]. An AGN scenario thus remains possible [57,58,59,60], but it could also be due to other mechanisms such as a young neutron star with pulsar wind nebula [49,50,51,52], or a neutron star interacting with small bodies [63,64,65].…”
Section: Introductionmentioning
confidence: 99%
“…Popular mechanisms include: mergers of binary NS [31,32,33], or binary WD [34], or NS-WD binary [35,36], or NS/WD-BH binary [37,38,39], the interactions of pulsar-BH systems [40] or Kerr-Newman BH-BH [41,42], collapse of compact objects (e.g., collapse of NS [43,44,45,46,47], collapse of strange star crust [48]), giant pulses/flares from magnetars or young pulsars [49,50,51,52], and other supernovae interrelated theories [22,53,54,55,56]). A few other models include: mechanisms related to active galactic nuclei(AGN) and Kerr-BH or Strange Star interactions [57,58,59,60,61], collisions between NSs and small bodies [62,63,64,65], Axion star collides with a NS/BH [66,67,68], interactions between Axions and compact bodies [69,70,71], explosions such as starquakes [72], primordial BHs/Planck stars collapse to form white holes [73,…”
Section: Introductionmentioning
confidence: 99%