Kilonovas caused by black hole neutron star mergers

In summary: Most observed GRBs are believed to consist of a narrow beam of intense radiation released during a supernova as a rapidly rotating, high-mass star collapses to form a neutron star, quark star, or black hole."The narrow beam of radiation is what is observed, and it is what is believed to cause the afterglow.
  • #1
Tanelorn
888
15
I thought readers would be interested in this interesting article today on black hole and neutron star mergers and the very small possibility of instantaneous sterilization and extinction of all life on earth:http://www.space.com/22231-gamma-ray-bursts-neutron-stars.html

http://news.yahoo.com/kilonova-dead-star-crashes-may-spark-mysterious-cosmic-212239960.htmlAnother on the origin of Gold:

http://www.space.com/21995-gold-origins-neutron-star-collisions.html
 
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Space news on Phys.org
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Could anyone please confirm if the duration of the gamma ray burst, lasting 0.09 seconds, is consistent with the stretching of the gamma ray pulse as a result of the expansion of space between us and the object 4 Billion light years away? How long would we expect the gamma ray burst to have lasted at its source? Are Gamma ray burst frequencies very narrow band or even single frequency lines, or are they quite wideband and dispersed?
 
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  • #3
Are Gamma ray burst frequencies very narrow band or even single frequency lines, or are they quite wideband and dispersed?

yes:

Gamma-ray bursts (GRBs) are flashes of gamma rays associated with extremely energetic explosions that have been observed in distant galaxies. They are the brightest electromagnetic events known to occur in the universe.[1] Bursts can last from ten milliseconds to several minutes. The initial burst is usually followed by a longer-lived "afterglow" emitted at longer wavelengths (X-ray, ultraviolet, optical, infrared, microwave and radio).[2]

Most observed GRBs are believed to consist of a narrow beam of intense radiation released during a supernova as a rapidly rotating, high-mass star collapses to form a neutron star, quark star, or black hole.

http://en.wikipedia.org/wiki/Gamma-ray_burst
 
  • #4
Could anyone please confirm if the duration of the gamma ray burst, lasting 0.09 seconds, is consistent with the stretching of the gamma ray pulse as a result of the expansion of space between us and the object 4 Billion light years away?

The duration of the source radiation has nothing to do with any subsequent redshift during transit...

And there are lots of gamma ray bursts in the universe...fortunately for us it is really, really big and we are really, really small. So if somebody shoots a cannon off in Moscow or Paris or Singapore for example, I fell pretty safe here in NJ.
 
  • #5
Thanks Naty, I was just curious if there was a change in the duration of the pulse as a result of redshift and if it agreed with any expected change in duration expected by the standard model.
"Are Gamma ray burst frequencies very narrow band or even single frequency lines, or are they quite wideband and dispersed?"

The quote you provided doesn't mention how narrow band the gamma ray pulse is.
Laser light is narrowband, white light is broadband.
 
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  • #6
GRB's are not narrow band emissions. They peak in gamma frequencies, but, are also detected in visible light frequencies.
 

1. What is a kilonova?

A kilonova is a type of astronomical event that occurs when two compact objects, such as a black hole and a neutron star, merge together. This results in a powerful explosion that releases a huge amount of energy, equivalent to about 1,000 times that of a typical nova.

2. How are kilonovas caused by black hole neutron star mergers?

Kilonovas are caused by the merger of two compact objects, specifically a black hole and a neutron star. When these two objects come together, their intense gravitational forces cause them to spiral towards each other, eventually colliding and releasing a massive amount of energy in the process.

3. How are kilonovas different from other types of astronomical events?

Kilonovas are unique in that they are much more powerful than a typical nova, but not as powerful as a supernova. They also emit different types of light compared to other events, such as gamma rays and infrared radiation, which can help scientists distinguish them from other types of explosions.

4. What can scientists learn from studying kilonovas caused by black hole neutron star mergers?

Studying kilonovas can provide valuable insights into the physics of extreme events in the universe. These explosions also release heavy elements, such as gold and platinum, into the surrounding space, which can help scientists understand the origins of these elements and how they are distributed throughout the universe.

5. How often do kilonovas caused by black hole neutron star mergers occur?

Kilonovas are relatively rare events, as they require the specific conditions of a black hole and neutron star merging together. It is estimated that they occur once every 10,000 years in a galaxy the size of our Milky Way. However, with advancements in technology and the ability to detect gravitational waves, scientists are now able to observe these events more frequently.

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