![]() |
|
|
|
Thread Tools | Display Modes |
|
#1
|
|||
|
|||
![]()
Andrew Usher wrote:
On Jan 25, 3:24 am, " wrote: What will they look like toward the end of their lives? At some point the "apple-sized region" will get too small or too cold to sustain "electroweak burning", but the object could then be too small to remain a neutron star. Will it "reinflate" to a white dwarf of some sort? Can someone tell me what the heck 'electroweak burning' is? I haven't seen a good explanation here. Andrew Usher Word Salad, sprinkled with kooked opinions. |
#2
|
|||
|
|||
![]()
On 23 Jan, 09:41, Yousuf Khan wrote:
This is presumably one stage higher than a black hole, but two stages lower than a neutron star, and one stage lower than a quark star. I'm not sure, it's not mentioned in the article if it's lower or higher than a quark star. Also not mentioned in the article is what happens to this star after about 10 million years, when the electroweak burning phase finishes? Does it turn into a black hole, or does it turn into a neutron star or quark star? And how does a quark turn into a lepton? Is that in the Standard Model? Or is this coming from an interpretation of one of the Superstring or some other theories? The only thing I know about the Weak force is how it causes atomic fission. * * * * Yousuf Khan *** SPACE.com -- New Type of Exotic Star Proposed "An electroweak star could come into being toward the end of a massive star's life, after nuclear fusion has stopped in its core, but before the star collapses into a black hole, the researchers found. At this point, the temperature and density inside a star could be so high, subatomic particles called quarks (which are the building blocks of protons and neutrons) could be converted into lighter particles called leptons, which include electrons and neutrinos. "In this process, which we call electroweak burning, huge amounts of energy can be released," the researchers wrote in the scientific paper. Unfortunately for observers, much of that energy would be in the form of neutrinos, which are very light neutral particles that can pass through ordinary matter without interacting, making them very difficult to detect.."http://www.space.com/scienceastronomy/exotic-star-type-proposed-10012... Kahn Last phase for a Sun like star is a White Dwarf. It has about the size of Earth,but now has a mass density of 100,000 times greater than it was Sun size. I read it can shine for a trillion years ??? TreBert |
#3
|
|||
|
|||
![]()
bert wrote:
Kahn Last phase for a Sun like star is a White Dwarf. It has about the size of Earth,but now has a mass density of 100,000 times greater than it was Sun size. I read it can shine for a trillion years ??? TreBert A white dwarf is basically just radiating leftover heat away, it's not producing any new energy like with nuclear fusion; that's how it keeps "shining". It's now a battery rather than a generator. As the degenerate matter inside it enters into lower energy states, they radiate the energy away in the form of photons. It can take trillions of years for all of the degenerate matter from the deep interior of the white dwarf all of the way upto the surface to all enter their lowest energy states. The same goes for neutron stars and quark stars. As all of that type of degenerate matter shift around inside it, until they all eventually enter their lowest energy states, it can take trillions of years. In the case of this electroweak star, they are suggesting that the conversion of quarks into leptons is what carries away their energy, rather than through photons. They suggest that this is a phase that can last only 10 million years before it stops. I assume that means only a small percentage of quarks can be converted into leptons, probably only the stuff at the core which is at greatest pressure. When all of this is finished, I presume that the star is now much lighter as the leptons carry away not only energy but also mass. At that point the star probably just becomes a normal neutron or quark star. Yousuf Khan |
#4
|
|||
|
|||
![]()
On Jan 23, 8:41*am, Yousuf Khan wrote:
This is presumably one stage higher than a black hole, but two stages lower than a neutron star, and one stage lower than a quark star. I'm not sure, it's not mentioned in the article if it's lower or higher than a quark star. Also not mentioned in the article is what happens to this star after about 10 million years, when the electroweak burning phase finishes? Does it turn into a black hole, or does it turn into a neutron star or quark star? And how does a quark turn into a lepton? Is that in the Standard Model? It comes from one of several *extensions* to the Standard Model. Examples include the now defunct SU(5) supergroup, technicolor, and some supersymmetry variants. Or is this coming from an interpretation of one of the Superstring or some other theories? The only thing I know about the Weak force is how it causes atomic fission. * * * * Yousuf Khan *** SPACE.com -- New Type of Exotic Star Proposed "An electroweak star could come into being toward the end of a massive star's life, after nuclear fusion has stopped in its core, but before the star collapses into a black hole, the researchers found. At this point, the temperature and density inside a star could be so high, subatomic particles called quarks (which are the building blocks of protons and neutrons) could be converted into lighter particles called leptons, which include electrons and neutrinos. "In this process, which we call electroweak burning, huge amounts of energy can be released," the researchers wrote in the scientific paper. Unfortunately for observers, much of that energy would be in the form of neutrinos, which are very light neutral particles that can pass through ordinary matter without interacting, making them very difficult to detect.."http://www.space.com/scienceastronomy/exotic-star-type-proposed-10012... |
#5
|
|||
|
|||
![]()
On Jan 27, 11:53*am, PD wrote:
And how does a quark turn into a lepton? Is that in the Standard Model? It comes from one of several *extensions* to the Standard Model. Examples include the now defunct SU(5) supergroup, technicolor, and some supersymmetry variants. Please read the preceding posts. It _is_ Standard Model, albeit many people (including me, until now) have never heard of it. Andrew Usher |
#6
|
|||
|
|||
![]()
Andrew Usher wrote:
On Jan 27, 11:53 am, PD wrote: And how does a quark turn into a lepton? Is that in the Standard Model? It comes from one of several *extensions* to the Standard Model. Examples include the now defunct SU(5) supergroup, technicolor, and some supersymmetry variants. Please read the preceding posts. It _is_ Standard Model, albeit many people (including me, until now) have never heard of it. Andrew Usher It seems the majority of us in this newsgroup have a conventional understanding of nuclear physics circa the 1950's, but there are groups of scientists who have a deeper understanding about it than us. Perhaps equipped with 1970's knowledge. ![]() It may not be as profound a divide as we see between the people equipped with Newtonian knowledge, trying to come to terms with Einstein. However, it shows us how difficult it is for the Newtonians to upgrade from the 17th century to the early 20th century. Yousuf Khan |
#7
|
|||
|
|||
![]() "Yousuf Khan" wrote in message ... Andrew Usher wrote: On Jan 27, 11:53 am, PD wrote: And how does a quark turn into a lepton? Is that in the Standard Model? It comes from one of several *extensions* to the Standard Model. Examples include the now defunct SU(5) supergroup, technicolor, and some supersymmetry variants. Please read the preceding posts. It _is_ Standard Model, albeit many people (including me, until now) have never heard of it. Andrew Usher It seems the majority of us in this newsgroup have a conventional understanding of nuclear physics circa the 1950's, but there are groups of scientists who have a deeper understanding about it than us. Perhaps equipped with 1970's knowledge. ![]() It may not be as profound a divide as we see between the people equipped with Newtonian knowledge, trying to come to terms with Einstein. However, it shows us how difficult it is for the Newtonians to upgrade from the 17th century to the early 20th century. Yousuf Khan Should a sane mathematician come to terms with an incompetent egomaniac? Oh wait... a bigot like you is not qualified to answer that. Take your head out of your arse and learn something, grinagog: http://androcles01.pwp.blueyonder.co...r_children.htm |
#8
|
|||
|
|||
![]()
On Jan 28, 9:24*am, Yousuf Khan wrote:
It seems the majority of us in this newsgroup have a conventional understanding of nuclear physics circa the 1950's, but there are groups of scientists who have a deeper understanding about it than us. Perhaps equipped with 1970's knowledge. ![]() Yeah, it's strange that this is just being investigated now. I wonder if we'll ever detect one of these stars. The trouble is, the energy of electroweak burning will be virtually all emitted as neutrinos, and thus undetectable. The photon luminosity should be hardly greater than a normal neutron star. So I guess the sign of an electroweak star will be an object that clearly can't be a black hole but is above the normal neutron-star limit, which is probably around 2.2 Msun. Andrew Usher |
|
Thread Tools | |
Display Modes | |
|
|
![]() |
||||
Thread | Thread Starter | Forum | Replies | Last Post |
M-47, Open Star Cluster in Puppis; plus star clusters NGC 2423 and NGC 2425 | George Normandin[_1_] | Astro Pictures | 3 | March 4th 08 06:25 PM |
Utiyama's 1954 unfied gauge theory of gravity and electroweak-strongfields | Jack Sarfatti | Astronomy Misc | 1 | June 3rd 07 11:27 PM |
Cluster and Double Star see star crack during massive 'starquake'(Forwarded) | Andrew Yee | Astronomy Misc | 0 | September 22nd 05 04:37 PM |
Online star map / star chart / star atlas | Excalibur | Astronomy Misc | 3 | September 12th 03 07:25 PM |
Online star map / star chart / star atlas | Excalibur | Amateur Astronomy | 3 | September 12th 03 07:25 PM |