Interesting article about dark matter

In summary: DM be made from?I also wondered could DM help explain in some way where all the anti matter ended up?In summary, DM is a label for an unknown type of matter that may be accumulating in neutron stars, and could be responsible for the lack of neutron stars in the galactic core. DM may also be a possible explanation for where all the regular antimatter ended up.
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Tanelorn
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Space news on Phys.org
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In physics, something is "black" if it absorbs lots of the light that hits it - an ideal "black body" for instance absorbs all the light that hits it.
Being black, in this sense, does not stop something from also glowing,

For an object to be black in color, it need only absorb light in the visible spectrum.

Dark Matter (DM) by comparison, does not interact with light at all, light just passes right through, and it is a label to be used until we can figure out what is going on.
The article is about this sort of DM and how it may be interacting with the regular matter in Neutron stars to result in the statistical lack of neutron stars in the galactic core.
It goes on to tell you what sort of stuff this sort of DM would be consistent with. If the theory is right, and that's a big "if", then it narrows down the field of possibilities.

DM is unlikely to explain where all the regular antimatter ended up - why would anti-DM gravitating to anti-matter do anything special?
More likely a similar mechanism gave rise to the asymmetry of both types of matter.

The article is very speculative right now - it is not even clear how you'd be able to tell if a pulsar were dying due to dark matter or not and there are other possibilities for the lack of pulsars in the galactic core.
 
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Tanelorn said:
what might this kind of DM be made from?

The article doesn't propose any new type of dark matter. It only proposes that enough of it may be 'accumulating' in a neutron star to cause to to turn into a black hole.

Tanelorn said:
I also wondered could DM help explain in some way where all the anti matter ended up?

I suppose it's possible, but at this time it doesn't help us much as far as I know.
 
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Simon, I meant dark. I seem to have written black instead of dark. Very strange.

The anti matter very long shot idea was just a brainstorming suggestion to solve two mysteries with "one stone"..
 
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Tanelorn, you obviously are smart enough to realize this is a bunch of bull, so why parade it here?
 
  • #6
Or at least give references to published papers or physics ArXiv eprints.

Garth
 
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Sorry guys, it was a just spur of the moment, ASIDE QUESTION.
I only know that we have two mysteries and I just wondered if there was any connection there:

1. Where did all the anti-matter go?
2. What is dark matter made of and where did it come from? - and 5 times more DM mass than normal matter at that.

I am certainly not clever enough to know that there was DEFINATELY no connection.
 
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Tanelorn said:
Sorry guys, it was a just spur of the moment, ASIDE QUESTION.

I didn't have a problem with your post.
 
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  • #9
Tanelorn said:
Where did all the anti-matter go?

That isn't a mystery; it all got annihilated by matter as the early universe expanded and cooled. The mystery is why there was a small amount of matter left over; ordinarily we would expect matter and antimatter to be created in equal quantities at the end of the inflation era, so the annihilation process would have left only radiation behind. However, the discovery of CP violations in the weak interaction provided a mechanism that could produced a slight asymmetry between matter and antimatter; this is currently believed to be the reason why our universe today contains matter but (practically) no antimatter.
 
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  • #10
Thanks Peter, I am pretty sure I did know this, but apparently not yesterday.
 
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Is there a lack neutron stars in globular clusters as well?
 
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  • #12
As I understand the observable gravitational effects of dark matter, the speculation introduced in the referenced article ignores much about these observations. I am sorry I cannot readily cite a source reference, but a major part of the dark matter in the universe is all around and through galactic clusters, not just in the galaxies. The behavior of the motion of galaxies in clusters requires this to be so.
 
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Simon Bridge said:
The article is about this sort of DM and how it may be interacting with the regular matter in Neutron stars to result in the statistical lack of neutron stars in the galactic core.
Drakkith said:
The article doesn't propose any new type of dark matter. It only proposes that enough of it may be 'accumulating' in a neutron star to cause to to turn into a black hole.
Hi @Simon Bridge and @Drakkith:

What I find puzzling about this idea is that there is an implication that there is a much higher concentration of DM near the galaxy core than the average in the halo. From recent dialogs in other threads, I have come to understand that in order for a DM particle to change its orbit relative to a central mass from one of large geometry to smaller, it has to get rid of its energy. Also, unlike baryonic matter, this is very unlikely since DM doesn't have interactions that can create photons to radiate away the orbital energy, as happens with baryonic matter.

Regards,
Buzz
 
  • #15
Buzz Bloom said:
... in order for a DM particle to change its orbit relative to a central mass from one of large geometry to smaller, it has to get rid of its energy. ...
I think the answer to this could be that not all orbits are perfectly circular. in fact that would probably be rare.
An eliptical orbit can have the orbiting object sometimes closer and sometimes further from the COM without needing to lose energy.
It only has to travel faster when nearer to the COM, and only gravity is involved.
 
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  • #16
rootone said:
An eliptical orbit can have the orbiting object sometimes closer and sometimes further from the COM without needing to lose energy.
It only has to travel faster when nearer to the COM, and only gravity is involved.
Hi rootone:

The problem with a DM particle P in large elliptical orbit falling onto a neutron star (NS) is that P will have to hit the surface of NS, and that is a very tiny target. Also, the angle at which P hits NS may have further limiting constraints. AFAIK, no one has done any analysis about this possibility, calculating the fraction of the DM halo that might hit and be captured by the NS, that is, not just pass through a portion of the NS and continue its orbit.

Regards,
Buzz
 
  • #17
Maths for the capture of Dark Matter by Neutron stars has been done.
http://arxiv.org/abs/1201.2400
... I find many hits for this and other papers in a casual search.
 

Related to Interesting article about dark matter

1. What is dark matter?

Dark matter is a type of matter that makes up about 27% of the universe, but it does not emit or absorb light, making it invisible to telescopes. Its existence is inferred through its gravitational effects on visible matter.

2. How was dark matter discovered?

The existence of dark matter was first proposed by Swiss astronomer Fritz Zwicky in the 1930s. He noticed that the mass of galaxy clusters seemed to be much greater than the mass of visible matter, leading him to hypothesize the existence of an invisible form of matter.

3. What is the current understanding of dark matter?

While the exact nature of dark matter is still unknown, scientists believe that it is made up of particles that interact very weakly with light and other forms of matter. These particles have not yet been directly detected, but many experiments are currently underway to try and identify them.

4. How does dark matter impact the universe?

Dark matter plays a crucial role in the formation and evolution of the universe. Its gravitational pull helps to hold galaxies together and contributes to the large-scale structure of the universe. Without dark matter, the universe would look very different and many galaxies may not have formed.

5. What are some ongoing research efforts related to dark matter?

There are many ongoing research efforts to try and better understand dark matter. These include experiments such as the Large Hadron Collider, which is searching for particles that could make up dark matter, and telescopes like the Hubble Space Telescope, which is studying the effects of dark matter on the development of galaxies. Scientists are also using computer simulations and observations of the cosmic microwave background to study the distribution and properties of dark matter in the universe.

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