Is Dark Matter a Dead End in Physics?

[BillKet]

A new experiment (it's true a small scale one with the possibility of being brought to a much larger scale) has failed to find any sign of Dark Matter (DM), like all the other experiments before (at least the ground based one). AMS seems to have found some important extra anti-protons and positrons, that might be consistent with DM annihilation, but even so, it could be alternative explanations (and this wouldn't count as a direct detection, anyway). I was wondering what the Physics Forums community thinks about this lack of evidence for DM despite numerous and different approaches to find it (DAMA/LIBRA experiment claims to have found it, but no one was able to reproduce their results). Do we need a fundamentally new detection method (after all, even colliders won't be able to go too much higher in energy, for sure nowhere close to Plank scale anytime soon, so we do need a new approach for high energies)? Do we need some totally new theoretical ideas to describe Dark Matter, in a complete opposite direction from the current models? Do we need to give up on DM completely and find a new explanation for the observed gravitational behavior of the galaxies (MOND?)? What do you think?

 

[Dale]

MOND is not a viable alternative, regardless of any perceived problems with DM.

I wouldn’t rush to get rid of DM. It has been observed gravitationally and looks like it doesn’t interact much otherwise. So it will be inherently difficult to detect.

Science isn’t room service where you can order a result to your liking to be delivered by the end of the sitcom you are watching. It is a difficult enterprise and honest science always has a real risk of null results.

 

[BillKet]

MOND is not a viable alternative, regardless of any perceived problems with DM.

I wouldn’t rush to get rid of DM. It has been observed gravitationally and looks like it doesn’t interact much otherwise. So it will be inherently difficult to detect.

Science isn’t room service where you can order a result to your liking to be delivered by the end of the sitcom you are watching. It is a difficult enterprise and honest science always has a real risk of null results.

I totally agree, but if so many experiments failed to detect it, why don't we try a new approach? We know that we have something that interacts gravitationally, but why would interact otherwise with the visible matter? Maybe this is the only way, so we would need to build a detector able to detect that (which goes back to my point that we are nowhere near close to do that with the type of detectors we have so far, so maybe we need a totally new type of detector). Honestly, I feel the same goes for SUSY. It is a beautiful mathematical framework, but if so many experiments failed to detect any SUSY particle (and basically the hierarchy problem for which it was mostly invented it's hard to be solved anymore with the current boundary on SUSY), why do people keep working so hard on it (both theoretically and experimentally) instead of trying something new? And I am aware that there are many other models, but what I mean why is the scientific community so focused on something specific, when we can try many other things?

 

[Arman777]

I totally agree, but if so many experiments failed to detect it, why don't we try a new approach? We know that we have something that interacts gravitationally, but why would interact otherwise with the visible matter? Maybe this is the only way, so we would need to build a detector able to detect that (which goes back to my point that we are nowhere near close to do that with the type of detectors we have so far, so maybe we need a totally new type of detector). Honestly, I feel the same goes for SUSY. It is a beautiful mathematical framework, but if so many experiments failed to detect any SUSY particle (and basically the hierarchy problem for which it was mostly invented it's hard to be solved anymore with the current boundary on SUSY), why do people keep working so hard on it (both theoretically and experimentally) instead of trying something new? And I am aware that there are many other models, but what I mean why is the scientific community so focused on something specific, when we can try many other things?

Like what kind of other things ?

 

[BillKet]

Like what kind of other things ?

Oh i don't know, that's my point. People are focusing so much on SUSY, that other approaches barely exist or if they exist they are not given enough importance such that experiments can get funding to test them. My point is, how long do you stick to a theory (which gave absolutely no experimental evidence of being right) before you try testing other theories or start coming up with new theories? I am not an expert so I don't really know if and what other models exist out there, I am just wondering when one decides that a model doesn't describe the actual reality and tries building a new model? For example string theory makes predictions mostly at energy scale we can't test yet. So there is no solid reason to claim that String theory doesn't describe nature. But SUSY should have given experimental evidence, but it didn't. So probably it's not the right thing.

 

[Orodruin]

People are focusing so much on SUSY, that other approaches barely exist or if they exist they are not given enough importance such that experiments can get funding to test them.

This is simply untrue. While SUSY may get a lot of attention and SUSY searches are relatively well funded, this does not mean that no other approaches exist. The most prominent type of such searches probably being axion searches, but there are others too.

Also, generic WIMP models tend to be the models that are relatively easy to test.

So there is no solid reason to claim that String theory doesn't describe nature.

More importantly, there is also no reason to claim that it does.

But SUSY should have given experimental evidence, but it didn't.

This is also untrue. What has been tested are very particular SUSY models that were constructed to be easily detectable. Of course you could question the practice of engineering models that are easily testable, but that is another question.

What has been tested (to some extent) is low scale SUSY. In superstring theory models, the natural SUSY scale is the string scale ...

 

[Arman777]

Oh i don't know, that's my point. People are focusing so much on SUSY, that other approaches barely exist or if they exist they are not given enough importance such that experiments can get funding to test them.

I find 2 sites that explains other dark matter candidates.This one is a bit overview
http://web.mit.edu/redingtn/www/netadv/specr/345/node1.html
This one seems better
http://www.slac.stanford.edu/econf/C040802/papers/L002.PDF

 

[Dale]

I totally agree, but if so many experiments failed to detect it, why don't we try a new approach?

We do. Each new experiment is a new approach. And each research lab has a different strategy.

I mean why is the scientific community so focused on something specific, when we can try many other things?

If you read the literature you will see that this is already happening. The scientific community is always approaching a problem multiple ways, and in stiff competition with each other.

 

[bbbl67]

Okay, so I understand that MOND-type solutions are out-of-favour at the moment, so we won't go there. Another out-of-favour solution is MACHO-based DM. Some experiments have come to the conclusion that it can't be billions of black holes, but how do they come up with that conclusion? They come to this conclusion based on our current understanding of how black holes form, so we assume that they must all come from stellar-mass sources. What if much smaller mass black holes were produced in the aftermath of the Big Bang? It's not a mechanism for forming black holes that we're familiar with. These would have the mass of asteroids or planets, rather than stars, and they'd be so small that we couldn't possibly look for them through gravitational lensing experiments. They'd be wandering around the universe widely dispersed, barely ever encountering another such micro-black hole, ever. But in the aggregate, they'd be so common within the multi-peta cubic light-years of a galactic halo, that they'd make up the majority of the mass of these galaxies?

 

[Arman777]

Okay, so I understand that MOND-type solutions are out-of-favour at the moment, so we won't go there. Another out-of-favour solution is MACHO-based DM. Some experiments have come to the conclusion that it can't be billions of black holes, but how do they come up with that conclusion? They come to this conclusion based on our current understanding of how black holes form, so we assume that they must all come from stellar-mass sources. What if much smaller mass black holes were produced in the aftermath of the Big Bang? It's not a mechanism for forming black holes that we're familiar with. These would have the mass of asteroids or planets, rather than stars, and they'd be so small that we couldn't possibly look for them through gravitational lensing experiments. They'd be wandering around the universe widely dispersed, barely ever encountering another such micro-black hole, ever. But in the aggregate, they'd be so common within the multi-peta cubic light-years of a galactic halo, that they'd make up the majority of the mass of these galaxies?

I don't think that would be possible. First we need a lot of black holes. We need 5 times mass of the visible mass, and that much of black holes in the size of asteroids...?

Also small black holes will evaporate faster.

Another thing is Actually DM created the galaxy structures that we see. So can these tiny black holes can create the galacy structures that we see ??

So visible matter is just affected by DM. DM also must be created in the early universe to keep expansion at critical level.

 

[Orodruin]

They come to this conclusion based on our current understanding of how black holes form, so we assume that they must all come from stellar-mass sources.

You really need to stop making unsubstantiated and false claims without any proper references. It is a really bad way of discussing.

What if much smaller mass black holes were produced in the aftermath of the Big Bang? It's not a mechanism for forming black holes that we're familiar with.

Yes it is. Primordial black holes are actively discussed in the dark matter community and mostly ruled out by different experiments depending on the mass range. Some people in the community argue for and against certain bounds so there may still be some windows, but overall the situation looks rather grim for PBHs.

 

[Dale]

These would have the mass of asteroids or planets, rather than stars,

Asteroids, yes, but not planets. Ongoing efforts to detect them are in progress, and the current lower threshold for detecting them is about 1/3 of the mass of the moon. So if they exist then they are smaller than that.

All of these possibilities are being pursued in the scientific community. Each group is in competition with the others to find evidence supporting a plausible mechanism.

 

[Arman777]

Asteroids, yes, but not planets. Ongoing efforts to detect them are in progress, and the current lower threshold for detecting them is about 1/3 of the mass of the moon. So if they exist then they are smaller than that.

All of these possibilities are being pursued in the scientific community. Each group is in competition with the others to find evidence supporting a plausible mechanism.

I want to ask something. If these are the cases then should we see a lot of black holes around us ? I didnt understand the theory here.

 

[Dale]

I want to ask something. If these are the cases then should we see a lot of black holes around us ? I didnt understand the theory here.

More likely just plain asteroids, IMO. Why suppose an asteroid sized black hole when you can just as easily suppose an asteroid.

 

[Arman777]

More likely just plain asteroids, IMO. Why suppose an asteroid sized black hole when you can just as easily suppose an asteroid.

And I am asking where are the "astroids" ? I understand that we are trying to observe them but isn't it absurd ? I mean I don't understand why they are DM candidates.

"The visible disk of the Milky Way galaxy is embedded in a much larger, roughly spherical halo of dark matter. The dark matter density drops off with distance from the galactic center. It is now believed that about 95% of the Galaxy is composed of dark matter, a type of matter that does not seem to interact with the rest of the Galaxy's matter and energy in any way except through gravity. The luminous matter makes up approximately $9 x 10^10$ solar masses. The dark matter halo is likely to include around $6 x 10^11$ to $3 x 10^12$ solar masses of dark matter."

Small astroid size black holes how can there be formed, without evaporation and they can still contribute ? Since our galaxy still in one piece, then how it can be possible ?

I can understand that in the early universe they might have been formed. But I don't give any chance that they exist now or contribute to the DM that we see around.

"General relativity predicts the smallest primordial black holes would have evaporated by now, but if there were a fourth spatial dimension – as predicted by string theory – it would affect how gravity acts on small scales and "slow down the evaporation quite substantially"

"Depending on the model, primordial black holes could have initial masses ranging from $10^{−8}$ kg (the so-called Planck relics) to more than thousands of solar masses. However, primordial black holes with a mass lower than $10^{11}$ kg would have evaporated due to Hawking radiation in a time much shorter than the age of the Universe, so they cannot have survived until the present Universe.A noticeable exception is the case of Planck relics that could eventually be stable"

However this part might be true

" Primordial black holes are also good candidates for being the seeds of the supermassive black holes at the center of massive galaxies, as well as of intermediate-mass black holes"

btw, I am not trying argue here. Just with all these stuff why they think it can be the DM candidate

Yes it is. Primordial black holes are actively discussed in the dark matter community and mostly ruled out by different experiments depending on the mass range. Some people in the community argue for and against certain bounds so there may still be some windows, but overall the situation looks rather grim for PBHs.

I agree. I guess they don't see as a candidate now. Thats nice

 

[Orodruin]

Just with all these stuff why they think it can be the DM candidate

Why not? It is a perfectly fine dark matter candidate. You look at how they would behave and compare that to what you can observe about dark matter. Depending on who you ask, you might get the answer that they are ruled out by observations or that there are still some windows open that allow PBH dark matter.

 

[Dale]

And I am asking where are the "astroids" ?

That is what the MACHO studies are trying to find out.

I mean I don't understand why they are DM candidates.

I don’t think they are likely either, but they are also not completely ruled out.

 

[Arman777]

Well okay then what can I say

 

[Bandersnatch]

More likely just plain asteroids, IMO. Why suppose an asteroid sized black hole when you can just as easily suppose an asteroid.

I suppose it's because asteroids couldn't contribute to the peaks in CMB power spectrum.

 

[bbbl67]

I don't think that would be possible. First we need a lot of black holes. We need 5 times mass of the visible mass, and that much of black holes in the size of asteroids...?

Also small black holes will evaporate faster.

Another thing is Actually DM created the galaxy structures that we see. So can these tiny black holes can create the galacy structures that we see ??

So visible matter is just affected by DM. DM also must be created in the early universe to keep expansion at critical level.

I'm not talking about BH's the size (implying volume) of asteroids, but rather the mass of asteroids. For example a black hole approximately the mass of the asteroid Vesta would have a Schwarzschild radius of only 400 nm! You'll never be able to spot such a tiny object from any telescopic distance.

Yes, smaller BH's evaporate faster, but they will still last billions of years. In fact, the currently accepted limit for BH stability is about 60% the mass of the Moon. A BH with 0.6 Moon masses will have a Hawking Radiation temperature of about 2.7 K, which the same temperature as the Cosmic Background Radiation, so such a black hole would be feeding energy off of the CMBR at the same rate as it is losing to Hawking Radiation. Things much smaller than that would still be quite stable for billions or trillions of years.

As for creating the structure of the Universe, that structure was probably already created in the quantum fluctuations at the time of the Big Bang, and these primordial BH's were probably also created and placed within those fluctuations, so they are just following the pre-existing quantum structure. Dark Matter is probably just maintaining the original quantum structure, rather than having created that structure at the cosmological scale.

Asteroids, yes, but not planets. Ongoing efforts to detect them are in progress, and the current lower threshold for detecting them is about 1/3 of the mass of the moon. So if they exist then they are smaller than that.

All of these possibilities are being pursued in the scientific community. Each group is in competition with the others to find evidence supporting a plausible mechanism.

How would they be able to detect black holes at 1/3 Moon mass? Can they already detect BH's larger than that? Well, obviously they can detect stellar mass BH's, but even those are pretty elusive if they're not orbiting and feeding on another star.

 

[Orodruin]

As for creating the structure of the Universe, that structure was probably already created in the quantum fluctuations at the time of the Big Bang, and these primordial BH's were probably also created and placed within those fluctuations, so they are just following the pre-existing quantum structure. Dark Matter is probably just maintaining the original quantum structure, rather than having created that structure at the cosmological scale.

Please stop speculating! The research on how PBH dark matter would work is out there. Also, you cannot just refer to "original quantum fluctuations". The post Big Bang structure formation is rather well understood and requires dark matter that has certain properties. Your dark matter needs to have those properties.

Here is a few years old constraint plot on PBHs (from http://inspirehep.net/record/1630595).

There have been some updates and further discussions on each of these constraints, but generally this is how the situation looks. Your "asteroid Vesta sized" black holes are ruled out by gravitational microlensing in this paper https://arxiv.org/abs/1701.02151 to be less than 0.01 of the total dark matter content.

 

[mfb]

For example a black hole approximately the mass of the asteroid Vesta would have a Schwarzschild radius of only 400 nm! You'll never be able to spot such a tiny object from any telescopic distance.

Not that it would be necessary. You can calculate how often such a black hole would get trapped in a star and swallow it, for example. Is the expected rate observable? If yes, does it match observations?

This is just one out of many approaches.

 

[Dale]

How would they be able to detect black holes at 1/3 Moon mass? Can they already detect BH's larger than that?

Yes, 1/3 lunar mass is currently the lower limit for the MACHO project. Unfortunately, I cannot tell you how they are detected at that level. It is not my area of expertise.

 

[bbbl67]

Not that it would be necessary. You can calculate how often such a black hole would get trapped in a star and swallow it, for example. Is the expected rate observable? If yes, does it match observations?

This is just one out of many approaches.

Well, first of all, what reason would there be for such a BH to get trapped inside a star? There's so much space between stars, there's no reason to get trapped by a star.

Second, a micro-BH would be nearly frictionless when entering the atmosphere of a star, because it would have such a small cross-sectional area, for example a Vesta-mass BH has a Schwarzschild Radius of only 400nm. But an actual Vesta-sized asteroid entering the atmosphere of a star would have lots of drag coefficient due to its large volume, 7.8×10^16 m^3 vs. 2.681×10^-19 m^3 for a BH of the same mass, i.e. 35 orders of magnitude larger. Even if a micro-BH entered a star (e.g. the Sun), it would emerge right out of it again, its momentum hardly changed, it would feel a drag force of only 145 mN (https://is.gd/gdHaET). Whereas an actual Vesta-sized asteroid would feel a drag force of 6.293×10^22 N. If the same micro-BH entered into the Earth it would feel a slightly larger of drag force of 561 mN. It's only if it entered into a neutron star that it would feel any sort significant drag force, 2.036×10^14 N (https://is.gd/NytkBo).

On the other hand, a Vesta-mass BH would be radiating Hawking Radiation at a temperature of 459.5 K. That would be well within the infrared range.

 

[bbbl67]

Please stop speculating! The research on how PBH dark matter would work is out there. Also, you cannot just refer to "original quantum fluctuations". The post Big Bang structure formation is rather well understood and requires dark matter that has certain properties. Your dark matter needs to have those properties.

Here is a few years old constraint plot on PBHs (from http://inspirehep.net/record/1630595).
View attachment 233456
There have been some updates and further discussions on each of these constraints, but generally this is how the situation looks. Your "asteroid Vesta sized" black holes are ruled out by gravitational microlensing in this paper https://arxiv.org/abs/1701.02151 to be less than 0.01 of the total dark matter content.

These studies are making their own assumptions, and each study has its own set of assumptions. We won't know anything for certain until we have actual examples of micro-BH's. They can plot as many graphs as they like, but they are barely above the level of hypothesis.

 

[Orodruin]

These studies are making their own assumptions, and each study has its own set of assumptions. We won't know anything for certain until we have actual examples of micro-BH's. They can plot as many graphs as they like, but they are barely above the level of hypothesis.

Sorry, but this comes across as highly unscientific. You cannot discredit a study just because you do not like the conclusions. As far as I understand, the assumptions made in those particular studies are fairly general. If you have specific criticism, you should say so and not wave your hands in the air and referring to "their assumptions are probably wrong".

 

[Arman777]

@bbbl67 Why you are thinking that PBH are such a good DM candidates ? I mean why you think its better then WIMP's or some other theory since it seems you are trying to defend the idea of it highly (Unlike me )

 

[bbbl67]

@bbbl67 Why you are thinking that PBH are such a good DM candidates ? I mean why you think its better then WIMP's or some other theory since it seems you are trying to defend the idea of it highly (Unlike me )

Because it seems to be more scientifically plausible than WIMPs. With black holes, we already know they exist. With WIMPs, it's never been proven that they exist. Granted, the examples of BH's that are known to exist are several orders of magnitude heavier than the types we're talking about here, but that's still a whole lot more plausible than WIMPs.

For example, the mass of Dark Matter in the Milky Way is estimated to be about 3E+12 solar masses, while the mass of luminous matter is only about 9E+10 solar masses. Within a spherical volume with a diameter the same as the Milky Way, that's a volume of 4.434×10^62 m^3. That means that the density of Dark Matter only has to be 1.345×10^-20 kg/m^3. Given that density, and sticking with my Vesta-mass PBH example (but take your own pick, Ceres-mass, Pluto-mass, etc.), that means that you only need one Vesta PBH every 1.985×10^40 m^3, or 1 Vesta every 5.929×10^6 au^3. A 400 nm black hole every 6 million cubic AU is pretty much completely undetectable.

 

[Arman777]

Because it seems to be more scientifically plausible than WIMPs. With black holes, we already know they exist. With WIMPs, it's never been proven that they exist. Granted, the examples of BH's that are known to exist are several orders of magnitude heavier than the types we're talking about here, but that's still a whole lot more plausible than WIMPs.

For example, the mass of Dark Matter in the Milky Way is estimated to be about 3E+12 solar masses, while the mass of luminous matter is only about 9E+10 solar masses. Within a spherical volume with a diameter the same as the Milky Way, that's a volume of 4.434×10^62 m^3. That means that the density of Dark Matter only has to be 1.345×10^-20 kg/m^3. Given that density, and sticking with my Vesta-mass PBH example (but take your own pick, Ceres-mass, Pluto-mass, etc.), that means that you only need one Vesta PBH every 1.985×10^40 m^3, or 1 Vesta every 5.929×10^6 au^3. A 400 nm black hole every 6 million cubic AU is pretty much completely undetectable.

I see well thanks for sharing your opinion

 

[Bandersnatch]

With WIMPs, it's never been proven that they exist. Granted, the examples of BH's that are known to exist are several orders of magnitude heavier than the types we're talking about here

Neutrinos exist. Granted, the examples that are known to exist are lighter than the types we're talking about...

 

[Justin Hunt]

@bbbl67 PBH are just as farfetched as WIMPS. We have no proof that PBH exist, are stable, or can even be formed. Assuming hawking radiation is correct, there has not been enough time for stellar BHs to have shrunken to that size nor would micro BH been able to grow to that size.

 

[bbbl67]

Neutrinos exist. Granted, the examples that are known to exist are lighter than the types we're talking about...

Sterile neutrinos are pretty much the last harrah of WIMPs, most early WIMP theories were looking at SuSy particles, and those hopes started fading away after the LHC started reducing the places where SuSy can hide. Sterile neutrinos weren't even expected to produce enough mass to account for all of Dark Matter, originally they only expected enough sterile neutrinos to fill out a bit of the DM picture, mostly filled by SuSy. Now they're going to have to not only discover sterile neutrinos, but also to find enough of it to fill out the entire DM universe.

 

[bbbl67]

@bbbl67 PBH are just as farfetched as WIMPS. We have no proof that PBH exist, are stable, or can even be formed. Assuming hawking radiation is correct, there has not been enough time for stellar BHs to have shrunken to that size nor would micro BH been able to grow to that size.

Being primordial BH's, they wouldn't be born from stars like stellar mass BH's are. They would've been born in the high pressures and temperatures of the Big Bang itself. So no, they wouldn't be stellar mass BH's just shrunk down due to Hawking Radiation (that would take multi-trillions of years). The PBH's would have been born immediately after the Big Bang, as mass and energy densities within the plasma would've been high enough to create instantaneous BH regions. It is also expected that these PBH's would've been formed at widely-varied scales, not just the stellar mass kind. They could've been created at ranges as low as asteroid-mass all of the way upto supermassive-class BH's. In fact, I would say the most likely origin of galactic supermassive BH's is primordial rather than the merger of millions of stellar BH's.

So to answer your question about whether we've found evidence of PBH's? I think it's nearly irrefutable that all supermassive BH's are PBH's. But we haven't found evidence for sub-stellar mass PBH's yet though.

 

[Dale]

I think it's nearly irrefutable that all supermassive BH's are PBH's.

Unfalsifiable statements usually are irrefutable.

That said, I don’t definitively rule out any candidates until a good one is ruled in.

 

[Justin Hunt]

@bbbl67 White dwarfs and neutron stars do not become black holes if left alone. An article I read said that scientists believed this was due to the Pauli exclusion property of the subatomic particles. Whatever the reason is, I would imagine this is what would also prevent PBH from actually forming below stellar masses and even if they did, it is quite possible they would simply expand back out again similar to what happens when you release a stress ball. Matter resists being compressed.

As far as dark matter goes, the main theory, WIMPS and many variations believe our model is correct and we just need to account for the undetected mass somehow while MOND takes the assumption that there is an error with our model, namely gravity, and tries to modify that rather than account for the missing mass. My question is couldn't the rotation curves not matching expectation be a symptom rather than the issue? For instance, almost everything we do in Cosmology hings on one assumption or another. For example, the most accurate way to judge distances is using parallax, but Scientists can only use this to measure the distance to relatively close stars. However, they did use this method and a type of supernova to create the standard candle method for determining the distance of stars that are much further away. The problem is when you start going out to very long distance, you begin to have to take other considerations such as the expansion of the universe. My point is that almost every one of these quantities has a degree of uncertainty to it. So, couldn't part of the issue be compounded issues of uncertainty when we look at galactic distances? In order to determine the rotation curves, we had to determine the mass of the visible matter, we had to determine the velocities stars etc, none of which can be directly observed. There are way more uncontrollable variables in Cosmology than any other science and I am very impressed with everything they have been able to do. AI algorithms, however, could really come in use in sorting it all out. I have read articles here and there where AI algorithms were used in Cosmology, but for something really specific. But, it would be very useful for one to be used to take all the variables and a large collection of data and determine which combinations are the most fitting of actual data. Maybe there are WIMPS, maybe there are PBH, maybe our understanding of gravity is complete etc. or maybe it is a combination of more than one of those things. At the very least, an AI algorithm could be used to determine the most likely candidates.

 

[mfb]

@bbbl67: Please consider your discussion style and the situation here.

You dismiss entire peer-reviewed publications because they make assumptions. Well stated assumptions, discussed among experts, tested or at least checked with simulations and so on. You dismiss them without giving any reason, without even specifying what exactly you disagree with.
On the other hand your own posts here are full of assumptions, usually not even stated explicitly, many of them are demonstrably wrong - some so wrong that everyone with introductory astronomy classes knows better. Many of them have been pointed out. Yet you continue to argue along that line, as if it wouldn't matter that it is all based on wrong assumptions.

Do you really think this is a healthy discussion style?

 

[Orodruin]

Whatever the reason is, I would imagine this is what would also prevent PBH from actually forming below stellar masses and even if they did, it is quite possible they would simply expand back out again similar to what happens when you release a stress ball.

This is not correct and does not describe PBH formation in an accurate way. Very simplified, PBHs may form when density perturbations reenter the horizon such that the Schwarzschild radius of the mass contained within one Hubble radius exceeds the Hubble radius itself. This would happen in the very early universe and there would not be any question of compressing mass.

 

[Ian J Miller]

Suppose dark matter was a fermion, and further, suppose being electrically neutral it is its own antiparticle. When matter and antimatter self-annihilated but for an asymmetry that left us with an excess of matter, these fermions would not do that. The Stanford link above argues the mass must be >25 eV, but that is not exactly a huge barrier, so if dark matter did comprise such fermions, how would you detect them given they do not interact electromagnetically, they do not clump and they do not decay to anything? In my opinion, not easily, and not with detectors looking for much more massive particles.

 

[Orodruin]

When matter and antimatter self-annihilated but for an asymmetry that left us with an excess of matter, these fermions would not do that.

You seem to here be implying that there would be no dark matter. This is not the case. In fact, what you are describing is the standard production of thermal dark matter where the final density is set by when the interaction rate falls below the Hubble rate. This happens sooner for particles that do not interact very strongly with each other.

how would you detect them given they do not interact electromagnetically, they do not clump and they do not decay to anything? In my opinion, not easily, and not with detectors looking for much more massive particles.

This depends very much on the mass range that you are looking in. Standard WIMP scenarios where you search using direct detection experiments go down to a few GeV, which is needed to produce an appreciable recoil in the experiment. The exact search strategy would depend on the type of interactions that the DM has - you would need to specify your model further - but in general it can indeed be very hard.

 

[Buzz Bloom]

I find the discussion in this thread a bit odd. The OP seems to question the evidence for the existence of DM.

I was wondering what the Physics Forums community thinks about this lack of evidence for DM despite numerous and different approaches to find it (DAMA/LIBRA experiment claims to have found it, but no one was able to reproduce their results).

All of the discussion has been about possible/plausible/maybe answers to the question: What might DM consist of? Examples:

I wouldn’t rush to get rid of DM. It has been observed gravitationally and looks like it doesn’t interact much otherwise. So it will be inherently difficult to detect.

Sterile neutrinos are pretty much the last harrah of WIMPs, most early WIMP theories were looking at SuSy particles, and those hopes started fading away after the LHC started reducing the places where SuSy can hide.

None of the posts have mentioned the evidence for the existence of DM as non-baryon stuff based on the abundance of deuterium created during the period of primordial Nucleosynthesis.

https://en.wikipedia.org/wiki/Nucleosynthesis
The first nuclei were formed about three minutes after the Big Bang, through the process called Big Bang nucleosynthesis. Seventeen minutes later the universe had cooled to a point at which these processes ended, so only the fastest and simplest reactions occurred, leaving our universe containing about 75% hydrogen, 24% helium, and traces of other elements such as lithium and the hydrogen isotope deuterium. The universe still has approximately the same composition today.​

The role of DM during the period is as follows. If R, the ratio of DM density to baryon density, was substantially less than the estimated current value,

R < R₀ = 14.5%/85.5% = 17.0%,

https://en.wikipedia.org/wiki/Dark_matter
"Thus, dark matter constitutes 84.5% of total mass..."​

then the universe would have expanded more rapidly, and the fusion of deuterium into helium would have been less, and there would therefore be substantially more deuterium. Similarly, if R was substantially greater than R₀, then there would be substantially less deuterium.

A second minor issue relates to the discussion of primordial black holes (PBHs). Example:

Primordial black holes are actively discussed in the dark matter community and mostly ruled out by different experiments depending on the mass range.

The discussion of this point seems to assume that PBHs (if they exist) consist entirely of DM. However, one would expect that only 85.5% of a BH's mass would be DM.

Regards,
Buzz

 

[Orodruin]

The discussion of this point seems to assume that PBHs (if they exist) consist entirely of DM. However, one would expect that only 85.5% of a BH's mass would be DM.

Huh? This is not correct. The PBHs would be the dark matter.

 

[Buzz Bloom]

Huh? This is not correct. The PBHs would be the dark matter.

Hi Orodruin:

If you are correct about this, then I must have a wrong view about quite a few topics. I would much appreciate it if you would post an explanation of how a PBH would form without any baryonic matter being captured along with the DM.

I think there is a good reason to believe that a PBH would be less than 85.5% DM, perhaps even all baryonic matter. The reason I have in mind is that baryonic particles interact with other baryonic particles in such a way that relative to a nearby random primordial region R with greater than average mass density, these particles will lose kinetic energy and tend to fall towards the center of mass of R. DM will not lose kinetic energy in this manner, and therefore will follow a trajectory less likely to accumulate with the mass that will after a while form the PBH.

ADDED
I think there might be an issue regarding the timing of the creation of PBHs. I was assuming the PBHs form after the period of nucleosynthesis. Do you know of a reason why they must form before nucleosynthesis?

MORE ADDED
My error.

https://en.wikipedia.org/wiki/Primordial_black_hole

Primordial black holes belong to the class of massive compact halo objects (MACHOs). They are naturally a good dark matter candidate: they are (nearly) collision-less and stable (if sufficiently massive), they have non-relativistic velocities, and they form very early in the history of the Universe (typically less than one second after the Big Bang).​

I still do not understand, "they are (nearly) collision-less".

Regards,
Buzz

 

[Orodruin]

If you are correct about this, then I must have a wrong view about quite a few topics. I would much appreciate it if you would post an explanation of how a PBH would form without any baryonic matter being captured along with the DM.

How they formed is completely irrelevant. The black holes are dark matter in this scenario, there is no "other" dark matter to capture.

 

[Buzz Bloom]

How they formed is completely irrelevant. The black holes are dark matter in this scenario, there is no "other" dark matter to capture.

Hi Orodruin:

I get that now. The assumption is that a PBH is formed from ordinary matter very, very early after the "big bang" (< 1 second), and subsequently during primordial nucleosynthesis does not participate in the process of combining protons and neutrons into helium, etc. which occurred about 3-20 minutes following the "big bang".

I am now wondering about my last bit of confusion.

I still do not understand, "they are (nearly) collision-less".

In what sense is a PBH collision-less or nearly so? Why does not ordinary matter constantly collide with a PBH event horizon and become additional mass of the PBH?

Regards,
Buzz

 

[Bandersnatch]

I think collision-less here means they behave like a collision-less gas. I.e., without pressure. The only interactions they participate in are gravitational in nature - similarly to WIMPs.

 

[Sanborn Chase]

Does it matter that all of our celestial observations since the beginning of time have been through a filter the substance of which we know next to nothing?

 

[mfb]

Does it matter that all of our celestial observations since the beginning of time have been through a filter the substance of which we know next to nothing?

We know it doesn't influence the light going through apart from its gravitational effect - otherwise it would be part of the regular matter.

 

[Sanborn Chase]

How would you know it doesn't affect light if you'd never seen it otherwise?

 

[weirdoguy]

Because if dark matter exists then there is plenty of it in the galaxies and if it did interact with light electromagnetically we would certainly see effects of this interaction.

 

[Sanborn Chase]

I'm extremely buoyed by your confidence.