What Makes This Gamma-Ray Burst Even Brighter Than Others?

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A recent gamma-ray burst has been identified as a "giant pulse," significantly brighter than any previously recorded. This phenomenon is associated with only a few known pulsars, with the Crab pulsar being one of the few that emits such pulses regularly. The mechanism behind these giant pulses is still under investigation, with theories suggesting that they may originate from pulsars with a wobbly rotation axis, producing tightly focused emissions. The discussion also highlights the challenges in detecting these brief pulses and their potential polarization. Understanding these giant pulses could provide deeper insights into pulsar behavior and gamma-ray emissions.
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http://www.newscientist.com/news/news.jsp?id=ns99996736
This spectacular outburst was a “giant pulse”, something associated with only a few of the known pulsars
The pulse was an order of magnitude brighter than the brightest known gamma-ray burst
 
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This thing has intrigued very much, It would be horrible if suddenly a nearby pulsar started to emit giant pulses and scorched Earth, so I have made a bit of investigation.
The thing is that giant pulses were first detected in 1968 by Staelin; there are actually known only 4 pulsars emitting giant pulses, and one of them, the Crab pulsar emits on average a giant pulse every ten seconds. Any idea of what is the mechanism that produces giant pulses?
 
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I think these are otherwise 'normal' pulsars that have a wobbly axis of rotation. When you catch it at just the right angle, you get a tightly focused pulse. I would be curious as to how much polarized they are.. I would guess they are strongly polarized. The pulses are, however, so brief they are hard enough just to detect.
 
It makes sense, Chronos. This paper is interesting because it makes a distinction between giant pulses and giant micropulses
http://xxx.arxiv.cornell.edu/abs/astro-ph/0404174
 
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