Exploring GRB Occurrence and Galaxies Across the Observable Universe

In summary: They can explode in a number of ways, the most common being a supernova. GRBs are thought to be time dependent, meaning that their frequency decreases as the universe ages. 30 Mpc is only 100 million lightyears away, which is too close for comfort. Most scientists take a wait and see attitude when a rogue observation contradicts reasonably well established theories.
  • #1
granpa
2,268
7
GRB's occur once per day. over 10 billion years that's 3650 billion bursts (in the observable universe?). I think there are said to be around 100 billion galaxies in the observable universe so does that mean that 36 bursts occur in each galaxy?

http://www.faqs.org/faqs/astronomy/faq/part8/section-4.html

I wonder how large a galaxy has to be before it has a supermassive black hole?

I wonder how many globular clusters there are and how that compares to the number 3650 billion?
 
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  • #2
GRB's are high redshift events [the nearest suspect occurred at a distance estimated at over 30 Mpc], meaning they are relics of the distant past. Scientists believe hypernova are responsible for most GRB's. They are thought to arise from enormous, pristine [little or no metallicity] Pop I stars. Such stars do not exist in the Milky Way, or other nearby galaxies [gas clouds are too heavily polluted]. The rate of occurence is thought to be time dependent [frequency steadily decreases as universe ages].
 
  • #3
30 megaparsecs is only 100 million lightyears.
 
  • #5
Indeed, 30 Mpc is z~.1 which is a little too close for comfort to support the hypernova hypothesis. It is suspected more exotic mechanisms may also exist, such as binary neutron star mergers. No one is quite sure what might happen in those cases, but, they are rare events. High redshift hypernova's, however, reasonably account for the vast majority of GRB's. Cosmology is always full of surprises and outlier observations evoke a great deal of interest. Most scientists take a wait and see attitude when a rogue observation contradicts reasonably well established theories. Many explanations are possible. Unfortunately the resources necessary to validate [or invalidate] them are precious and most researchers are unwilling to gamble their grant money on hitting a home run. It's the nature of the beast. The need to conduct daring experiments is often obviated by more mainstream studies. Clever scientists find ways to squeeze exotic information from these more 'mainstream' studies - a low risk, high reward opportunity. They are fond of referring to this as serendipity [a technobable term meaning 'lucky guess'].
 
  • #6
Hello Chronos and granpa,

A few comments.

There are two types of GRB's, long bursts and short bursts ( > few seconds and < few seconds respectively). The hypernova model only attempts to explain long GRB bursts. Hypernova are not necessarily stars formed early in the universe ( Chronos had a typo, he meant the early pristine stars are population II or III stars), they are just really massive stars (rapidly spinning Wolf-Rayet stars).
 

1. What is a GRB (Gamma Ray Burst) and how does it occur?

A GRB is a powerful burst of high-energy gamma rays that can last from milliseconds to several minutes. It is thought to occur when a massive star collapses into a black hole or when two neutron stars merge. This explosion releases an enormous amount of energy, including gamma rays.

2. How are GRBs detected and studied?

GRBs are typically detected by satellites that are specifically designed to observe gamma ray emissions. These satellites can pinpoint the location of the GRB and provide data on its intensity and duration. Other telescopes can then observe the afterglow of the GRB in other wavelengths, such as X-rays, visible light, and radio waves, which can provide valuable information about the environment in which the GRB occurred.

3. What role do galaxies play in the occurrence of GRBs?

GRBs are most often associated with the death of massive stars, which are found in galaxies. This suggests that the formation and evolution of galaxies may play a crucial role in the occurrence of GRBs. Studying the relationship between GRBs and their host galaxies can provide insights into the formation and evolution of both.

4. How does exploring GRB occurrence across the observable universe help us understand the universe?

GRBs are thought to be one of the most energetic events in the universe, and they can be observed at extremely large distances. By studying the occurrence of GRBs across the observable universe, scientists can gain a better understanding of the distribution of matter and energy in the universe, as well as the processes that drive the formation and evolution of galaxies.

5. What are some current and future research efforts in exploring GRB occurrence and galaxies?

Current research efforts include using advanced telescopes and instruments to observe and study GRBs and their host galaxies. Future efforts involve developing new technologies and techniques for detecting and studying GRBs, as well as conducting large-scale surveys of the observable universe to better understand the relationship between GRBs and galaxies. Additionally, researchers are also working on theoretical models to better explain the origins and characteristics of GRBs.

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