/r/cosmology

Photograph via snooOG

/r/cosmology - a community for questions, discussions, and articles about cosmology.


Welcome to r/cosmology, the subreddit for questions, discussions, and articles about cosmology. Cosmology is the study of the early universe and the universe on the largest scales. Things galactic size and smaller generally belong elsewhere.

Reddiquette is enforced. Disrespectful and irrelevant comments will be removed.

If you claim an alternative model of the universe and ignore known data or have no equations or calculations, then your post will be removed. It isn't the responsibility of experts to review your "what if the universe was...?" idea. Homework questions will be removed. Repeated infractions will result in a ban.

Rude behavior is not tolerated.

If you do not see your submission in the new queue, please message the moderators as it may have been sent to the spam filter.

Find today's cosmology preprints on arXiv:astro-ph.CO.


Check out some other great subreddits:


Common questions:

  1. The universe is not expanding faster than light. Expansion has units of inverse time.

  2. The evidence for dark matter is overwhelming and reaches far beyond rotation curves.


Anything not related to cosmology will be removed.

/r/cosmology

96,495 Subscribers

5

De Sitter space and the “what is the universe expanding into” question

I fell asleep last night listening to Leanord Suskind on Theories of Everything talk about how string theory may not be a correct description of the world. He said that the universe seems more likely to be De Sitter. I admittedly don’t know what all that means but I was wondering if what he said, which was that there is no edge to De Spitter space, means that there isn’t even an other side for the universe to expand into

10 Comments
2024/11/02
03:38 UTC

0

If black holes are the source of dark energy, would that imply that the universe is therefore cyclic?

There is a recent study strengthening support for the hypothesis that black holes are in fact the source of dark energy.

Should this be the case, then in the far future when every black hole in the universe has evaporated, dark energy would have weakened enough for gravity to begin slowing and subsequently reversing the expansion, therefore ending the universe in a Big Crunch, of which a Big Bang would emerge.

To me this seems to suggest that if black holes are indeed the source of dark energy, then it implies that the universe cyclic, is this correct?

Evidence mounts for dark energy from black holes - University of Michigan

29 Comments
2024/10/31
12:03 UTC

8

Basic cosmology questions weekly thread

Ask your cosmology related questions in this thread.

Please read the sidebar and remember to follow reddiquette.

14 Comments
2024/10/31
09:00 UTC

22

How did time begin, without time?

I understand that standard BB cosmology holds that time began with the universe from a singularity approximately 14 billion years ago.

The thing I’m trying to understand, how can time have begun? Wouldn’t a thing ‘beginning’ require time? As in - from one state to another state requires time?

This leads me to think time must have always existed..

65 Comments
2024/10/29
19:18 UTC

6

Cosmic diffraction?

Seems to me the radiation of light across cosmic distances should develop an increasingly broad wave similar to diffraction, such that it might impinge anywhere along a wavefront. I haven't been able to see a discussion of it anywhere.

2 Comments
2024/10/29
18:39 UTC

3

Non zero chemical potential

I’ve skimmed through a few books and pretty much every case (besides the basic recombination stuff) have always set the chemical potential equal to 0.

I recently skimmed over a paper that included an equation with nonzero chemical potential and realized I have no idea what I’d do to find it (the paper was on sterile neutrinos). From basic thermo I know mu=(dU/dN)_V,S but I have no idea how to actually go about computing this.

Are there any resources where I could find more about this?

2 Comments
2024/10/29
03:47 UTC

4

how do you explain conformal cyclic universe?

Conformal cyclic cosmology (CCC) is a cosmological model in the framework of general relativity and proposed by theoretical physicist Roger Penrose.^([1])^([2])^([3]) In CCC, the universe iterates through infinite cycles, with the future timelike infinity (i.e. the latest end of any possible timescale evaluated for any point in space) of each previous iteration being identified with the Big Bang singularity of the next

19 Comments
2024/10/29
02:26 UTC

9

Would the big crunch end in one big quasar?

Let's say dark energy was removed and Universe began collapsing, would we have a giant quasar at the end in which all mass fell into and if so what would this look like?

9 Comments
2024/10/28
16:26 UTC

3

Cosmological Constant

Let's assume for a moment that the Cosmological Constant isn't defined as Constant. Let's assume that it varies with Cosmological Time:

  • Q: Does anyone have a graph of what it might look like ?
5 Comments
2024/10/28
02:29 UTC

5

Was our universe the result of a vacuum decay of a prior universe?

I was just reading the Big Think article by Ethan Siegel (just love his stuff!) about cosmic inflation and the Big Bang, and this thought suddenly occurred to me: was our Universe the result of a vacuum energy state (a "false vacuum") decay in a prior universe? (after typing this, I found some older references to the same idea that I'd not seen before)

Ooh, one more crazy speculation: what if the boundary of the "observable universe", about 93 billion light years, is the boundary of the vacuum energy decay progression?

27 Comments
2024/10/27
19:46 UTC

0

can someone link me mathematical calculations behind the inability to measure time before the bigbang?

A few months back I attended a lecture which talked about "what could have happened before the big bang". Unfortunately, I don't remember most of it, so I'm usually going by keywords, they said something about the fact that due to quantum fluctuations and the heisenberg uncertainty principle, and if you do the "calculations", you would get to the conclusion that it is impossible to measure time before the big bang, because of the the error term in time, you wont ever be able to tell what "time it is". They said the math was boring, however i wanted to look at it and also possibly get to know more about it. Can someone elaborate more on it?

9 Comments
2024/10/26
21:29 UTC

0

Could dark matter and dark energy be emergent from quantum-state interactions with space-time?

Hi everyone, I’ve been thinking about an idea and would love your thoughts. I'm new to this forum and looking to better inform myself.

What if dark matter and dark energy aren't separate entities but instead arise from interactions between quantum states of matter, photons, and the underlying structure of space-time? For example, could they result from transitions between quantum and classical behaviors as space-time adjusts to different degrees of coherence or decoherence?

I’m wondering if viewing space-time as having "layers" where quantum effects gradually shift into classical ones could offer a new perspective on these phenomena. Could this help explain some of the effects we currently attribute to dark matter and dark energy? I have tried to fit this into an overall framework, but I'm not an expert by any means.

Any thoughts or critiques would be much appreciated—thanks in advance!

9 Comments
2024/10/26
00:50 UTC

0

Would Einstein be ok with the fact that the fabric of spacetime is moving faster than the speed of light?

I know it's a fact, but wondering if general relativity or other thinkings of his would be able to explain this?

14 Comments
2024/10/25
00:29 UTC

97

Is it possible that the universe is just a cycle of Heat Deaths and Big Bangs?

Im just an enthusiast trying to understand the different theories. I was just wondering if the heat death scenario allows for an infinite existence, even if most of it is spent in a "heat death" state.

74 Comments
2024/10/24
23:01 UTC

6

Basic cosmology questions weekly thread

Ask your cosmology related questions in this thread.

Please read the sidebar and remember to follow reddiquette.

18 Comments
2024/10/24
09:00 UTC

3

Book recommendations for those interested in getting up to speed on latest developments in SETI?

I'm just some dummy but my very lay understanding of the situation is this:

Statistically speaking there almost must be aliens out there somewhere. Yet despite lots of searching, we have no evidence of them anywhere. (The Fermi Paradox.)

Despite knowing this, I find the topic very fascinating and would like to learn more about, for example, the types of things we've tried (I know about the Dyson Sphere hunt, for example), the types of things that have been suggested but not yet tried, what we might have learned from our findings (even though we haven't found evidence of aliens), if we've narrowed down the most likely candidates for specific planets that might contain life, what the current best thinking of the "explanations" for the Fermi Paradox might be, that kind of stuff.

Does anyone have any recommendations?

3 Comments
2024/10/24
03:50 UTC

0

Quantum Functions and the CCC Theory

I posted here before on some spiritual bs but now with my further knowledge on the way tunneling/fluctuations works is that they are random and that (in very rare circumstances) tunneling could happen from states of low to high energy. So could it be possible that given an exponentially long time (abt (10¹⁰)⁵⁶ years we could we could see another big bang?

4 Comments
2024/10/24
03:29 UTC

25

How much of a Problem are the JWST Observations of Early Galaxies

Hello all,

I am a physicist that works in magnetism, however I am part of journal club that is looking at all branches of physics and it's mu turn to present.

I found a paper that began by saying that some JWST observations of early galaxies (z~15) appear to be about 10 Gyr old based on how much they have evolved. However, according to their redshift and the LambdaCDM theory, they should only be 0.5 Gyr old. Clearly there is something wrong with one of the models if the results are off by that much.

Is this a big problem in Cosmology/Astrophysics? By that mean:

  • Is it foundation shaking and we need to rethink all of our models?
  • Or is it just interesting and could lead some some developments?
  • Or does nobody really care?

Just trying to get a feel for the impact of these observations. Any helpful discussion or links would be appreciated.

Thank you!

15 Comments
2024/10/23
20:31 UTC

25

My list of the most important papers in cosmology

Hi everyone, I've been putting together a list of the most influential research articles for modern cosmology. What do you think? What am I missing?

AuthorDate of ResearchWhy it was impactful
Henrietta Leavitt/Edward Pickering1912Period-luminosity relationship for Cepheids
Albert Einstein1915General relativity
Vesto Slipher1915Almost all celestial objects are redshifted
K Schwarzchild1916First solution of Einstein's field equations
Alexander Friedmann1922First to propose expanding universe
Edwin Hubble1927Hubble's law
Georges Lemaitre1927Co-discoverer of expanding universe
Fritz Zwicky1933First to propose dark matter
HP Robertson1935Co-discoverer of expanding universe
Arthur Walker1936Co-discoverer of expanding universe
Alpher/Bethe/Gamow1948Big Bang Nucleosynthesis
Penzias/Wilson1965CMB discovery
James Peebles1967Cosmic structure formation theory
YB Zel'dovich1970Cosmic structure formation theory
Vera Rubin1980Confirmation of existence of dark matter
Alan Guth1981Inflation theory
COBE collaboration1992First complete CMB map
Riess/Perlmutter/Schmidt1998/99Dark energy discovery
WMAP collaboration2003Refined CMB map
Planck collaboration2013Most high res. CMB map to date

EDIT: Added Vera Rubin, Gamow et al., Leavitt et al., COBE/WMAP/Planck teams, James Peebles, YB Zel'dovich

24 Comments
2024/10/23
12:59 UTC

12

Euclid’s 208 sky survey and those three galaxies interacting

I’m a casual observer and follower when it comes to anything space. Euclid’s sky survey (208-Gigapixel) just came across my feed and I’m interested if anyone can say anything more about the galaxies that are interacting in that video. Specifically, at time ~ [1:36]. There seems to be a very small galaxy (maybe?) between the two larger ones. Are all three of these interacting or is it just a visual illusion?

It is just amazing to see images like this, where galaxies are interacting the process of colliding. Thanks in advance

2 Comments
2024/10/22
21:48 UTC

0

Another big bang?

I was just watching a documentary about the space and it said there about another big bang slowly happening (not anytime soon), just wanted to ask to see if there is gonna happen anytime in life (talking about like millions of years)

2 Comments
2024/10/21
20:59 UTC

8

Are these calculation errors in the paper "Expanding Confusion"?

There's an excellent paper that I've read a few times called "Expanding Confusion" (2004) by Davis and Lineweaver that explains the variety of cosmic horizons quite well. Link to it here.

However in section 4.2 of that paper, when they derive a special relativistic and 𝑣=𝑐𝑧 interpretation for cosmic redshift (and disprove the SR interpretation by 23 sigma), it seems there are potentially some calculation errors: I'm unable to reproduce their results for the apparent magnitude in the B-band 𝑚𝐵.

Writing their method out explicitly we have Hubble’s law:

𝐻=𝑣/𝐷,

which is added to the longitudinal relativistic Doppler shift in terms of velocity,

https://preview.redd.it/3tze4tkzf5wd1.png?width=598&format=png&auto=webp&s=3dc8a84fcd4781cfeba421d385f54747c6d8e394

like so,

https://preview.redd.it/apfvd202g5wd1.png?width=682&format=png&auto=webp&s=5601af76cfc98307c36ab7bce9a0e8e513abad56

Then this proper distance is converted to luminosity distance, 𝐷(𝑧)(1+𝑧)=𝐷𝐿(𝑧), whose value we then plug into the distance modulus they used:

https://preview.redd.it/7ue8vfg4g5wd1.png?width=886&format=png&auto=webp&s=30c81ee6354caedfc58293a2710cff52d375ff61

where absolute magnitude 𝑀𝐵 = -3.45.

In the v = cz case, they use this for luminosity distance and put it into the same distance modulus above to get their measurements:

https://preview.redd.it/ylwlyva5g5wd1.png?width=672&format=png&auto=webp&s=ffee576d347f08420cae1cb0b3314a110abee46a

The errors become clear after a quick calculation: if we input 𝑧=1 and 𝐻=70𝑘𝑚/𝑠/𝑀𝑝𝑐 for instance, we get 𝑚𝐵=24.33 for the SR interpretation and 25.44 for the 𝑣=𝑐𝑧 interpretation rather than 𝑚𝐵=22.83,23.94, respectively, as written in the paper. I've put the corrected magnitude-redshift curves into their original Figure 5.

Did I misunderstand something or was there an oversight in their paper?

https://preview.redd.it/cmg6htk2f5wd1.png?width=2228&format=png&auto=webp&s=61bf785ac78e07d0e2eb2caad900c01623e35474

8 Comments
2024/10/21
18:34 UTC

0

Questions from Origins by Neil Degarss Tyson

Here's the two parts that I don't quite get: "To understand how the curvature of space affects the angular size of the features of the cosmic background radiation, imagine the epoch of decoupling, when the radiation finally stopped interacting with matter. During that time, the largest deviations from smoothness that existed in the Universe had a size which cosmologists can calculate: it is the age of the Universe then times the speed of light – about 380,000 light years across. This represents the maximum distance at which particles could affect each other, namely particle anomalies. At larger distances the other particles would not have arrived yet, so they could not be responsible for any deviation from smoothness.

How large an angle would the maximum deviations now cover in the sky? This depends on the curvature of space, which we can determine by finding what is the sum of ΩM, and ΩΛ. The more this curvature approaches 1, the closer the curvature of space will approach 0 and the larger will be the angular size we observe for the maximum deviations from magnitude smoothness in the cosmic background radiation. The curvature of space depends only on the sum of the two Ω, because both density types make space curve in the same way. Therefore observations of the cosmic background radiation offer a direct measurement of ΩΜ + ΩΛ, in contrast with observations of supernovae which measure the difference between ΩΜ and ΩΛ"

"This approach is based on the use of the "standard ruler", as cosmologists call it, in analogy to the "standard candles" of supernovae, used for the conventional approximation of Hubble's constant. As we described in the previous chapter, during the era of decoupling, 380,000 years after the Big Bang, the homogenizing effect exerted by radiation on matter essentially stopped. Since then, the radiation has wandered freely between the particles of matter, without affecting them to any significant degree. This happened when the maximum distance within which particles of matter could affect each other reached 420,000 light years, because regions that were much more distant did not have time to communicate in any way. This distance gives cosmologists their standard ruler. We noted its existence in the previous chapter, as it constitutes the maximum magnitude of deviations from normality in the cosmic background radiation.

As space expanded, so did the standard ruler, which continued to measure the largest areas of space within which clear deviations of the density of matter from its mean value could appear. Now we can "see" the ruler - or rather, its effect - at two different times. We have already seen the first: small deviations from uniformity in the cosmic background radiation, which follow the slightly anomalous distribution of matter during the decoupling epoch. Over the next billion years, these 1 in 100,000 density deviations evolved and became tremendously larger differences between the evolution of matter within giant galaxy clusters and the regions between them. The maximum sizes of these clusters show how much the standard ruler has increased in size from the time of decoupling to the present.

The second method of determining Hubble''s constant therefore aims to create an accurate map of the Universe today, in order to compare it with the initial differences in the cosmic background radiation. (Actually, "today" means "only 2 billion years ago," which is the average look-back time for the galaxy clusters that grew from the tiny deviations built into the cosmic background radiation.) The first decades of the 21st century, in an effort that continues to achieve greater precision, a program called the Sloan Digital Sky Survey used a specially designed telescope at Apache Point, New Mexico, to map the three-dimensional distribution of galaxies in space with unprecedented precision, thus yielding the current size of the standard ruler, which turns out to be approximately 490,000,000 light-years. Comparing this distance to the ruler's 450,000 light-years at the time of decoupling leads to a value of Hubble's constant close to 67."

(Translations to by Google translate so there might be some slight discrepancies)

From what I'm getting he's using 3 different values(380000, 420000, 450000 light years) for the same thing?

3 Comments
2024/10/20
09:10 UTC

7

How will the galaxies of the Local Group + the Antlia-Sextans group have changed in 5.5 billion years aside from Andromeda and the Milky Way colliding?

Edit: i'm more specifically referring to their locations relative to eachother and which ones will merge

3 Comments
2024/10/18
04:46 UTC

6

Basic cosmology questions weekly thread

Ask your cosmology related questions in this thread.

Please read the sidebar and remember to follow reddiquette.

14 Comments
2024/10/17
09:00 UTC

22

If Dark Energy inhabits the vacuum of spacetime, does it exist outside of our observable universe?

If there was only void/vacuum before the expansion of our universe began, then wouldn’t that mean that Dark Energy was already present? If it is believed that beyond the horizon of our observable universe is just “more of the same”, and Dark Energy is an inherent property of spacetime, does this mean that the inflationary period of our universe repelled the forces of Dark Energy?

Correct me if I am wrong, but as I understand it, the expansion of our observable universe is caused by the buildup of Dark Energy that forms between matter, which pushes any bodies of mass that are not linked by mutual gravity away from each other. And so the expansion of our universe is defined by the distance between objects just growing larger, and not that anything “expands” or “grows” per say. And as more void/vacuum builds up between mass, so to does Dark Energy, accelerating that expansion between said mass.

Following this thought process, shouldn’t the Dark Energy of the already existing void before the “Big Bang” have been affecting the inflationary period of our universe?

75 Comments
2024/10/16
15:29 UTC

6

Why are Large Quasar Groups defined as large structures yet they only have a few components?

I was reading about the large scale structure of the universe and I came across LQG. Basically large scale structures composed of Quasars, numbering as few as 5 or at most like 50 or 70 but usually around a dozen or so.

I don't understand why you can consider that a structure. Even some of the Quasars are not gravitationally connected. I tried to read the attached paper to understand it but I couldn't get it. Something about overdensities in a certain region maybe but I'm not sure.

Isn't it like if you took two marbles and connected them with a string and placed them 50 miles apart and said it was a 50 mile wide structure? And in this case the string is invisible since it's just gravity.

So please explain why you can say the structure is many billions of light years wide and yet it's composed of only a dozen or two galactic nucleus Quasars.

http://arxiv.org/pdf/1211.6256v1.pdf

2 Comments
2024/10/15
22:43 UTC

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