What Makes Gamma Ray Bursts a Fascinating Field of Study?

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SUMMARY

Gamma Ray Bursts (GRBs) are a significant area of study in astrophysics, categorized into long GRBs, caused by the supernova collapse of massive stars (around 30 solar masses), and short GRBs, likely resulting from neutron star mergers. The Fermi Space Telescope has identified nearly 500 gamma-ray sources since its launch in 2008, a substantial increase from the four known sources prior. Research indicates that over half of these sources are active galaxies, with pulsars and supernova remnants making up about 5 percent each. Despite these discoveries, many gamma-ray sources remain unidentified, highlighting the ongoing mysteries in this field.

PREREQUISITES
  • Understanding of gamma-ray astrophysics
  • Familiarity with supernova mechanics and classifications, particularly Type Ic
  • Knowledge of neutron star physics and mergers
  • Experience with data from the Fermi Space Telescope
NEXT STEPS
  • Research the mechanisms behind supernova explosions and their role in long GRBs
  • Explore the latest findings on neutron star mergers and their implications for short GRBs
  • Investigate the data and discoveries made by the Fermi Space Telescope
  • Study the relationship between cosmic rays and gamma-ray bursts, particularly in the context of recent research
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Astrophysicists, researchers in high-energy astrophysics, and students interested in the dynamics of gamma-ray bursts and their implications for cosmic phenomena.

SHISHKABOB
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I've been reading about gamma ray bursts (GRBs) lately and have found them to be pretty interesting. As far as I have read, it appears that we still don't know much about what actually causes them, or rather, how the "internal engine" works.

The most popular idea for longer lasting GRBs is a very massive star, 30 solar masses I think, going supernova, right?

Is there a lot of interest in GRBs today? Is it a good field of study to look into?
 
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GRBs are a very active field in astrophysics today. There appear to be two types - long GRBs (which last longer than ~ 1 second) and short GRBs (typically shorter than 1 seond). The long GRBs are pretty firmly established to be caused by supernova collapse of massive stars, as you said. In a few cases an optical supernova (of Type Ic if you're familiar with the nomenclature) has been seen that correspond to the long GRB. The best model for the short GRBs is that the represent the merger of two neutron stars, but this is much less firmly established.
 
..and here's some up to date research, video included, from NASA: http://www.space.com/15119-mysterious-gamma-ray-space-objects.html

The Fermi space telescope has spotted nearly 500 powerful gamma-ray sources in deep space over the last three years. Before its launch in 2008, scientists only knew of four such objects.

"We're not looking for the ordinary things," Thompson said. "We're looking for the extraordinary; powerful things that might produce gamma rays."

Of the newly discovered bodies, more than half are active galaxies. Pulsars and supernova remnants each make up about 5 percent of the sources, with high-mass binary stars and other galaxies contributing just a smidge more, the researchers said.

Yet a large collection of objects remains unidentified, they added.
Edit: I found this interesting story,
http://www.newscientist.com/article/dn20436-strange-cosmic-ray-hotspots-stalk-southern-skies.htmlRespectfully submitted,
Steve
 
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Dotini said:
..and here's some up to date research, video included, from NASA: http://www.space.com/15119-mysterious-gamma-ray-space-objects.html

The Fermi space telescope has spotted nearly 500 powerful gamma-ray sources in deep space over the last three years. Before its launch in 2008, scientists only knew of four such objects.

"We're not looking for the ordinary things," Thompson said. "We're looking for the extraordinary; powerful things that might produce gamma rays."

Of the newly discovered bodies, more than half are active galaxies. Pulsars and supernova remnants each make up about 5 percent of the sources, with high-mass binary stars and other galaxies contributing just a smidge more, the researchers said.

Yet a large collection of objects remains unidentified, they added.



Edit: I found this interesting story,
http://www.newscientist.com/article/dn20436-strange-cosmic-ray-hotspots-stalk-southern-skies.html


Respectfully submitted,
Steve

Isn't there a difference between gamma ray sources and gamma ray bursts? Like I know the Fermi Bubbles are thought to perhaps be large outflows of supernova wind material reacting with the intergalactic medium (I think).

however, it is still a very interesting article. Pretty nifty that they've found so many things in the sky that are complete mysteries.
 
SHISHKABOB, these may help in your quest:

"New results out of Antarctica support the idea that the most energetic of the superspeedy space particles raining down on Earth are not from gamma-ray bursts. The conclusion, reported in the April 19 Nature, has upped the ante on a long-standing mystery in astrophysics."
http://www.skyandtelescope.com/news/Cosmic-Ray-Origin-Still-Mysterious--148267685.html[/URL]

Nature | Letter
“An absence of neutrinos associated with cosmic-ray acceleration in γ-ray bursts
IceCube Collaboration”

“Very energetic astrophysical events are required to accelerate cosmic rays to above 1018 electronvolts (Etavolts). GRBs (γ-ray bursts) have been proposed as possible candidate sources. In the GRB ‘fireball’ model, cosmic-ray acceleration should be accompanied by neutrinos produced in the decay of charged pions created in interactions between the high-energy cosmic-ray protons and γ-rays. Previous searches for such neutrinos found none, but the constraints were weak because the sensitivity was at best approximately equal to the predicted flux. Here we report an upper limit on the flux of energetic neutrinos associated with GRBs that is at least a factor of 3.7 below the predictions. This implies either that GRBs are not the only sources of cosmic rays with energies exceeding 1018 electronvolts or that the efficiency of neutrino production is much lower than has been predicted.”
[URL]http://www.nature.com/nature/journal/v484/n7394/full/nature11068.html[/URL]
 
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