Questions tagged [cosmology]
Questions about the origin, history, evolution and fate of the Universe.
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How sensitive are early universe abundance calculations to the neutron half-life?
Phys.org's Physicists announce the world's most precise measurement of neutron lifetime discusses the accepted for publication Phys. Rev. Letter Improved neutron lifetime measurement with UCNτ (links ...
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+50
Cosmology context plotting : Covariance matrix - Script to plot Omega_m vs Omega_Lambda diagram in Python
I have covariance matrices and Markov chains coming from the SCP (Supernova Cosmology Project) and I would like to plot all these data
in the particular diagram Omega_Lambda vs Omega_m or w vs Omega_m....
2
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1answer
33 views
What's different of power spectrum and correlation function of BAO?
(source)
There is the sentence "the harmonic sequence in the power spectrum correspond to a single peak in the correlation function and that the damping envelope corresponds to the broadening of ...
2
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0answers
106 views
Integrate the expression of error for photometric galaxy clustering and after compute its variance - factor disturbing
The error on photometric galaxy clustering under the form of covariance which is actually a standard deviation expression for a fixed multipole $\ell$ :
$$
\sigma_{C, i j}^{A B}(\ell)=\Delta C_{i j}^{...
3
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1answer
75 views
Is the sound horizon 500 thousand light years or 500 million light years?
At 06:30 in the nice video Sound Waves from the Beginning of Time
about the baryon acoustic oscillations (BAO), the speaker says the sound horizon is about $500$ ...
2
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1answer
55 views
Observability of proper distance
Hubble's law at current time is as follows.
$$v=H(t_0)r$$
But if you look at the explanation on Wikipedia:
Strictly speaking, neither $v$ nor $D$ in the formula are directly observable, because they ...
1
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1answer
48 views
The Lambda-CDM-model: when will the Age of the universe catch up with the Hubble time?
Basic assumptions:
A) Within the Lambda-CDM-model we have two separate time measures:
the Age of the universe - today roughly 13.8 GY, and
the Hubble time - today roughly 14.4 GY
B) Very roughly, ...
2
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1answer
377 views
Why would a quantity like the 'Hubble contrast' be squared, then have its square root taken?
From Sabine Hossenfelder's recent video, New Evidence AGAINST Standard Cosmology:
And her source....
I don't get why a graph would show a quantity that is squared, then immediately 'square-rooted'......
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32 views
What does lowercase 'beta' mean in this graph of radio-emitting galaxies?
Correlation between the mass of the galaxies (X-axis) and
the difference of their radio emissions at different radio frequencies (Y-axis).
Each symbol represents an individual galaxy.
The image of an ...
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0answers
22 views
What is Euclidean fluence scaling in the context of bounding constraints on FRB all-sky rates? Would non-Euclidean scaling give a different answer?
The recent Chromatic periodic activity down to 120 MHz in a Fast Radio Burst contains two paragraphs in which X's are given "assuming an Euclidean fluence scaling".
To me, a non-astronomer, ...
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46 views
Are there ideas about Multiverse in cosmology that are independent of string theory?
It is known that string theory allows for many kinds of universes within it's Landscape which give rise to the concept of the multiverse. But are the concepts/ideas about multiverse in cosmology which ...
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47 views
Why does the 'Big Bang Nucleosynthesis' theory require that neutrinos, or at least sterile neutrinos, have a LARGE mass rather than a tiny one?
From Wikipedia, Sterile neutrino
Particles that possess the quantum numbers of sterile neutrinos and masses great enough such that they do not interfere with the current theory of Big Bang ...
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0answers
64 views
Do some physicists believe that the universe is a three-dimensional space wrapped on a four-dimension doughnut?
The astrophysicists believe if this is true, the universe would be
finite. The entire cosmos may be only three or four times larger than
the limits of the observable universe, which is about 45 ...
3
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1answer
79 views
How does the hypothesis of the "inconstant Hubble constant" solve the current crisis in cosmology?
It was published in a paper more or less like two months ago. I'd like to know also if more accurate measurements are necessary to close the gap between the model of the universe and the data reported....
5
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4answers
251 views
Why do we see a cosmological redshift at all if space is not expanded in our solar system?
It is generally accepted that the large scale redshift of galaxies (as given by the Hubble law) is due to the expansion of the universe. According to this theory, the fabric of space itself stretches ...
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1answer
68 views
How can we know the density of particles in interstellar or intergalactic space and could that density form dark matter?
It is assumed that the density of particles in the empty space between stars or galaxies is extremely low. But how do we know this density? The space surrounding the Sun is contaminated by cosmic ...
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2answers
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Why do gravitational waves travel "only" at the speed of light but the gravitational scalar potential is instantaneous?
To my old Space SE question Besides retarded gravitation, anything else to worry about when calculating MU69's orbit from scratch? @DavidHammen's excellent answer replies that one should not add a ...
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1answer
125 views
Is it "nonsense to even talk about" objects outside the observable universe not having gravitational influence on us? (finite speed of gravity)
In this supplemental answer to Is the zero gravity experienced in ISS the “artificial” kind? in Space Exploration SE I said:
Gravity moves at the speed of light so nothing outside out observable ...
2
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0answers
37 views
Formula to calculate round-trip travel time based on current distance to far-away galaxy
Cross-posted from Physics Stack Exchange - original
The question was closed as HW-like there.
The Premise
You travel at a constant velocity towards a far-away galaxy. You then travel back at the same ...
2
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3answers
290 views
Could it be that Universe is rotating while expanding? [duplicate]
I have read that the measurements of the cosmic microwave background indicate that the Universe has a flat geometry on large scales.
Could one assume then that the Universe is acceleratingly rotating ...
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0answers
22 views
How to locate helpful and instructive books and resources about numerical methods in cosmology?
I am interested in the hydrodynamical and N-body simulations, and I want to use simulation results to examine the theoretical models.
Hence I am searching for some helpful and instructive books and ...
5
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3answers
2k views
How can a black hole have a charge, or be charged?
So-called 'hairless' black holes (no-hair theory, or theorem?) , which is what real black holes are, can be described by just three characteristics: Mass, spin, and charge.
It is easy enough to ...
2
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0answers
50 views
What are the one-dimensional observables that can reveal the matter clustering properties of the Universe?
As we all know, the distribution of galaxies, which depend on the spatial coordinates, can help us understand the large-scale structure of the Universe. We can measure the distribution of galaxies ...
3
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1answer
40 views
Dark Matter Density Parameter Variation
The definition of the dark energy density parameter is $$\Omega_{\Lambda} = \frac{\epsilon_{\Lambda}}{\epsilon_c}$$
where $\epsilon$ is the energy density, $\Lambda$ subscripts represents dark energy ...
5
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1answer
166 views
If we watched extremely red-shifted galaxies near the edge of the observable universe for a very long time, how would they change? Would more appear?
I have understanding sphere eversion as #1 on my bucket list (if I ever get a round tuit) but understanding metric expansion seems to be a rapidly receding possibility :-)
Question: Suppose it takes ...
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0answers
31 views
How to find the scale factor on given time in the future if initial distance between source and destination is known
Assume the received redshift $z$ of a photon is known. We then can calculate the initial distance (when the received photon was emitted), the light Travel Distance, the current Distance (proper ...
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0answers
30 views
Questions re galaxies clusters and galaxies mergers within them
An introduction (containing the info I gathered from several Wikipedia articles).
A galaxy cluster, or cluster of galaxies, is a structure that consists of anywhere from hundreds to thousands of ...
3
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1answer
51 views
Scalar field displacement from the minimum of the potential gives rise to particles/dark matter, why?
The paper Lyman-alpha Constraints on Ultralight Scalar Dark Matter by Kobayashi et al. says, at the beginning of Section 3.1:
A light scalar field stays frozen at its initial field value in the early ...
2
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1answer
32 views
What do "overdense" and "underdense" mean in cosmology?
“Overdense" and "underdense" often appear in various documents to refer to high density and low density respectively. And I know that "overdensity" is defined as
$$
\delta(x)=\...
2
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0answers
26 views
Explain as simply as possible how the Sunyaev-Zeldovich (SZ) effect is used to estimate the Hubble constant
The Sunyaev–Zeldovich effect (SZ effect) is useful in determining the Hubble constant because it is independent of the cosmic distance ladder. This effect occurs when CMB (cosmic microwave background) ...
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1answer
98 views
Energy conservation of the universe
I have tried to derive an equation for the total energy of the universe.
I have found that,
$$E(t)= \delta\dot a(t)^2a(t)\Omega(t)$$
Where $\delta$ is just a positive constant, a(t) is the scale ...
1
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1answer
92 views
Comoving Volume Calculation
Suppose I have data from an astronomical survey at redshifts in the range $z = [2,3]$. Suppose that, on average in this range, the data covers an area on the sky of $A=1$ $\mathrm{Mpc}^2$. How would I ...
5
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0answers
49 views
How did pressure evolve in the (early) universe?
I am trying to derive how the cosmological pressure $p(t)$ evolved over time in the universe, especially in the radiation and matter dominated epochs. There are some very nice explanations how $H(t)$ ...
0
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1answer
69 views
Would it be a good idea to dockerize softwares in order to conduct hands-on tutorial sessions? [closed]
I am going to organize a tutorial in which I intend to train students on semi numerical simulations for reionization. Is it a good idea to supply use Docker to supply the codes?
What do you think ...
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0answers
24 views
Looking for analytical expression of Cosmic Variance - Poisson distribution?
I have an expression of Matter Angular power spectrum which can be computed numerically by a simple rectangular integration method (see below). I make appear in this expression the spectroscopic ...
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2answers
73 views
Does black hole singularity really exists with respective to relative frame of reference? [duplicate]
How can one describe this phenomena?
What are the factors that we should consider for solving such a problem?
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0answers
97 views
Where does the energy of the decaying CMB go?
I would expect that energy of photons in the Cosmic ray Microwave Background gets less and less because their wavelengths are stretched due to the expansion of space.
How can this be possible? Does it ...
1
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3answers
184 views
How is it possible that a universe with mass does not have curvature?
I may know the answer to my question. Mass must curve the universe but the pressure due to energy density may curve the universe in the opposite direction, leading to a flat universe, if they exactly ...
2
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4answers
334 views
What are the differences between astronomy and cosmology?
Are astronomy and cosmology same? If not, what are the differences? And which one is greater in terms of subject area?
3
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1answer
52 views
In any particular space or universe, is the shape of its metric the same as the shape of its geodesic (perhaps the sum of its geodesics)?
Perhaps I mean the curvature tensor, not the metric.
I suspect it is not.
I think the metric is a 4-dimensional object whereas the sum of the geodesics is 3-dimensional (probably 3+1 but not 4).
...
2
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0answers
88 views
Poisson noise for a squared contrast of density - expression of variance equal to $1/n^2$
I manage to compute the Poisson noise of a density field like this :
If I take $N$ the density of galaxies and compute the Shot noise with a Poisson distribution, I get :
$\langle N^2\rangle - \...
1
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1answer
41 views
Why is the FLRW universe (general relativity solution(s)) sometimes called the 'FRW universe'?
Why is the letter L for Georges LeMaîtres often, or even usually, left out?
Does he, or does he not, deserve some credit for this cosmological solution to Einstein's general relativity?
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0answers
22 views
Cosmic variance - Fourier Transform - a few precisions
I have posted initially on physics exchange but none answer, so I try my chance here (I am going to delete the physics exchange one) :
I cite an original report of a colleague :
If we are interested ...
2
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1answer
77 views
Can the Hubble Sphere ever extend over the cosmic event horizon?
I am struggling to reconcile the Hubble volume with the idea of a cosmic event horizon.
As I understand, the Hubble volume is increasing over time because Hubble's constant is decreasing. This should ...
2
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0answers
48 views
How do we know or predict which particles were present before Big Bang Nucleosynthesis occurred?
I'm reading Carroll and Ostlie's "An Introduction to Modern Astrophysics". In the BBN section, they describe that the universe contains a mixture of photons, electron-positron pairs, and ...
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3answers
2k views
Why did astronomers believe most or all stellar black holes had masses no greater than 15 solar masses?
The so-called 'mass gaps' for black holes, according to theoretical models, are between 2-5 solar masses and 50 to 150 solar masses. (Actually, I have read that there is no good theoretical reason ...
5
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1answer
103 views
Understanding better the factors on $C_l$ in Angular power spectrum and Relation with Matter power spectrum
I am looking for an explanation on the angular power spectrum. I found this extract that is interesting but not fully understood for me (I will cite the step that I didn't understand)
"what is ...
6
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0answers
57 views
What is the history of the average pressure, density, and temperature of the matter in the universe over time?
This question is inspired by this more specific question where Cerelic wanted to know if conditions were suitable for liquid water to exist during an epoch when the characteristic temperature of the ...
2
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0answers
54 views
How can the CMB have a "monopole anisotropy"?
Wikipedia's Cosmic Microwave Background (CMBR) radiation monopole anisotropy (ℓ = 0) says
When ℓ = 0, the ${\displaystyle Y(\theta ,\varphi )}{\displaystyle Y(\theta ,\varphi )}$ term reduced to 1, ...
2
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0answers
91 views
I have a scientific paper on gravity, how do I publish it, and will my research benefit me? [closed]
I read a lot about gravity and discovered a hole in it, and I want to publish that hole, but I am not good at mathematics. To show that gap, what should I do? Should I use Newton's equations which are ...
