Thermal expansion is the tendency of matter to change its shape, area, volume, and density in response to a change in temperature, usually not including phase transitions.Temperature is a monotonic function of the average molecular kinetic energy of a substance. When a substance is heated, molecules begin to vibrate and move more, usually creating more distance between themselves. Substances which contract with increasing temperature are unusual, and only occur within limited temperature ranges (see examples below). The relative expansion (also called strain) divided by the change in temperature is called the material's coefficient of linear thermal expansion and generally varies with temperature. As energy in particles increases, they start moving faster and faster weakening the intermolecular forces between them, therefore expanding the substance.
I am reading Griffiths chapter 3.4.3 on origin of coordinates in multipole expansion (can be found online here https://peppyhare.github.io/r/notes/griffiths/ch3-4/) And I got stuck at this:
For the figure 3.22: the dipole moment $p = qd\hat{y}$ and has a corresponding dipole term in the...
According to Hubble's law, galaxies are moving away from Earth at a speed proportional to their distance. In other words, the further away they are, the faster they move away from the Earth. The speed of galaxies is determined by their redshift.
Based on this law, some scientists have come to...
$$\delta W_{rev}=-PdV\tag{3}$$
and so
$$(dU)_{rev}=TdS-PdV\tag{4}$$
For an irreversible, closed system we have
$$(dU)_{irrev}=\delta Q_{irrev}+\delta W_{irrev}\tag{5}$$
My question is about the following statement
Sure, internal energy is a state function. I still don't understand...
In the following expansion how to find the coefficients ##\alpha## and ##\beta##?
$$|S, S_z\rangle = \alpha |S+1/2, S_z+1/2\rangle \otimes |1/2,-1/2\rangle + \beta |S+1/2, S_z-1/2\rangle \otimes |1/2,+1/2\rangle$$
I do not know if this is the place to post this. I am not a great physicist. Actually, I was an Electronic/Electrical Technician before I retired.
I learned that the vacuum of space is filled with matter/antimatter particles popping out of nothing and destroying themselves almost instantly.
My...
The cosmological redshift is generally assumed to be due to space expansion.
But if spacetime is locally flat Minkowskian then surely photon wavelength should not change?
The first equation states that every wavefunction can be written as a sum of wavefunctions of definite momentum, with A_p being defined as the coefficients in the expansion such that when you take the |wavefunction|^2 it equals 1 - fine.
We then multiply by the wavefunction conjugate and...
I had a question today as a part of my studies which was 1) If space is ever expanding what is the pressure on the creating space (universe) upon creation and 2) at what rate might you assume the quantum field is also being created and is it being affected by this pressure of creation. This is...
Is it theoretically possible for the expansion of the universe to red-shift the energy of a photon all the way to zero? If so, what happens to the photon? Or does the photon's energy only approach zero as an asymptote?
I don't understand the discovery of "accelerating expansion" in 1998 (hence the postulate of dark energy, etc..), because Hubble's old law already described exponentially accelerating expansion in 1929, right?
Hi I'm a medical doctor, this is just a hobby my uncle got me interested in as a kid. If the universe is acceleration and galaxies are moving further apart, we assume the universe as a whole is expanding as a result. It's also projected to my understanding that eventually the universe will...
I have two concentric thick cylinders in close tolerance (currently 50 micron gap), with a thin layer of glue between them.
Internal cylinder is made from steel and external cylinder is made from ceramic (so the thermal expansion coefficient is not the same)
The assembly is headed form inside...
##(1+x)^n=1+C_1x+C_2x^2+C_3x^3...+C_nx^n##
Let ##x=1##, hence ##2^n=1+C_1+C_2+C_3...+C_n## which is equal to the sum of the coefficients.
I originally thought the sum of the coefficients would be ##2^n-1## since the very first term ##1## is just a number and has no variable. But apparently...
Orodruin said in another thread that "the spacetime of a spatially flat universe generally has curvature".
Is the expansion (or contraction) of a spatially flat universe the manifestation of the curvature of its spacetime?
If so, does the expansion correspond to a positive or negative curvature?
I am trying to find some sources about time dimension expansion during spacetime expansion.
Why do We assume that only spacial dimensions expand? I only found a lot of weird arguments.
Btw, temporal dimension expansion does not mean that second was shorter in the past. Similarly to spacial...
Sorry for my questions as an amateur interested in physics: If light changes its frequency during a long time of travel in space (vacuum?) for all observers (redshift) and therefore its energy decreases (E=hf), what "entity" absorbs this energy? I suppose the answer will be that the wavelength...
Can the expansion/creation of space in the universe affect the speed of light over long distances? (dividing the space traveled (including expanded space) by the travel time). If the Hubble constant is valid throughout the universe, it follows that from a certain Megaparsec of distance, galaxies...
Ref: Principles of Physical Cosmology by P.J.E. Peoples, Princeton Univ. Press
This question is likely fully answered somewhere, but I cant find it.
Hubble obtained (1926) the mean mass density of the Universe as 10^-31 g/c.c. The gravitational stability equation gives (McCrea, Milne (1934))...
How can space expand when space is not a physical thing? I’ve heard some say that is not expanding but rather it is getting less dense, which to me implies the same thing.
To be clear, I'm looking for the speed at which points in space were moving apart from one another in the universe as it existed 370000 years after the big bang, not the Hubble parameter (expansion rate) derived from our current distance within our current time.
Thanks in advance!
Here's as far as I've gotten in the research (please correct any errors I'm making). The stages of high density had included these periods:
• light at high energy was in a cycle of forming into matter, forming back into light, and so on
• until things cooled enough for nucleons to form
•...
$$\int \text{d}^4 q \, \frac{1}{(q^2 + m^2)\left(1+\frac{q^2}{\Lambda^2}\right)^2} =2 \pi^2\left(\frac{\Lambda^2}{2}-m^2 \log \frac{\Lambda}{m} \right) + o(\Lambda^0)$$
How to get this result? The notation ##o(\Lambda^0)## means all terms constant in Lambda, which we ignore because we are...
I read this old thread: https://www.physicsforums.com/threads/what-happens-to-time-as-space-is-expanding.1001016/
And I am confused by the responses.
When I consider time dimension expansion, I perceive it the same way as space dimension expansion.
The expansion doesn't change the unit size...
I believe in the Big Bang but I struggle with something. If the Big Bang happened and universe is expanding there has to be something (or really nothing) there for the universe to be expanding into. Any thoughts?
Hello, assuming to keep an aluminum alloy motorcycle frame not in use, still, will the daily temperature variations cause thermal fatigue due to the continuous expansions and retractions or is the force developed by a few degrees of variations not sufficient to create microstructural dislocations?
Necessary condition for a curve to provide a weak extremum.
Let ##x(t)## be the extremum curve.
Let ##x=x(t,u) = x(t) + u\eta(t)## be the curve with variation in the neighbourhood of ##(\varepsilon,\varepsilon')##.
Let $$I(u) = \int^b_aL(t,x(t,u),\dot{x}(t,u))dt = \int^b_aL(t,x(t) +...
I suspect it will help if you know about my background: I did some linear algebra in university but never used it and am now in my mid 60s. I am interested in understanding the mathematics of quantum physics. I have read a number of layman's texts on quantum mechanics, but they all gloss over...
For this problem,
The solution is,
I understand their logic for their equation, but when I was trying to solve this problem, I came up with a different expression:
##\Delta A = \Delta L_x\Delta L_y##
##\Delta L_x =\Delta L_y = \Delta L## since this is a square.
##\Delta A = \Delta L^2##...
I the lambda-CDM model, is the expansion of spacetime uniform around all of spacetime, is there a smooth transition between expanding parts of spacetime (the voids) and non-expanding parts of spacetime, or is there a sharp distinction between expanding and non-expanding parts of spacetime.
Is...
Wikipedia states the following in their article about the expansion of the universe:
If the cosmological principle was discovered to be false in our universe, i.e. our universe was discovered to be inhomogeneous or anisotropic or both on very large scales and the FLRW metric does not hold for...
What is the meaning of the expansion at first order in ##\delta_2## and ##\delta_3## at the second step in the last line? These quantities are not "small" - on the contrary, the entire point is to then take the ##\epsilon \to 0## limit and the counterterms blow up
Using the adiabatic process formula, I've calculated the change in volume for a volume of gas with an initial pressure of 10 psig expanding to 0 psig. The initial volume is 100 cubic inches and the expanded volume is 144.9. This is a difference of 44.9. The total work done ends up being about...
Can you please explain this series
f(x+\alpha)=\sum^{\infty}_{n=0}\frac{\alpha^n}{n!}\frac{d^nf}{dx^n}
I am confused. Around which point is this Taylor series?
when you do a multipole expansion of the vector potential you get a monopole, dipole, quadrupole and so on terms. The monopole term for a current loop is μI/4πr*∫dl’ which goes to 0 as the integral is over a closed loop. I am kinda confused on that as evaulating the integral gives the arc length...
Greetings everyone.
I learned that the distance between molecules in liquid increases while the temperature increases. Hence, its density is decreased. The process is thermal expansion. At the same time, the collision between molecules would be more frequent when the temperature increases...
I proceeded in the usual manner in which we take ##dU = 0## in the case of free expansion because there is no heat transfer in the box, as well as no work is done.
We can write, taking ## U ## as the function of ##V## and ##T##, $$ dU(V,T) = \left( \dfrac{\partial U}{\partial V} \right)_T ~...
For a freely expanding ideal gas(irreversible transformation), the change in entropy is the same as in a reversible transformation with the same initial and final states. I don't quite understand why this is true, since Clausius' theorm only has this corrolary when the two transformations are...
Are there any kind of observed and experimentally verified processes or mechanisms where photon emission occurs and which are directly cause by spacetime expansion in some way?
Hey all. I'm trying to understand the evolution of the velocity distribution function of a gas undergoing free expansion. I know that at t=0, the velocity distribution function is given by ##u(t=0, x)=Ax^{1/2}##, where ##A## is a known constant.
From the momentum equation, I have:
##du/dt+u...
I'm wondering what's the difference between work done on quasi-static and non quasi-static expansion.
In a quasi-static process, the gas inside the system must do a work to "extend".
However, in a non quasi-static process, where the gas inside the system doesn't move fast enough to "push" the...
I am interested in the potential for air bubbles in a plastic structure to expand with heat, and put pressure on the plastic surrounding the air bubble.
In this case the plastic structure is formed by melting a thermoplastic powder. In between the grains of powder are voids with air in them. As...
Hi, I am a new user,
This question is bothering me for a long time and now with all the Webb telescope hype I need to ask:
It sounds very logical to think that a star that is a billion light years away is seen as it was a billion years ago because the light
took 1 billion years to get here...
Considering the FLWR metric in cartesian coordinates:
##ds^2=-dt^2+a^2(t)(dx^2+dy^2+dz^2)##
With ##a(t)=t##, the trace of the extrinsic curvature tensor is ##-3t##. But why is it negative if it's describing an expanding universe, not a contracting one?
Please explain how we know that it is space itself that is expanding rather than an expansion due to an explosion such as the big bang.
In either case wouldn’t every object appear to be moving away from us?
How do we determine that space/ time is expanding?
Tex
As I understand it, the flatness problem of Bob Dicke, says a flat universe in unstable and so has to be set very precisely in the early universe to give us the flat universe we see today. Is this the same problem as saying the expansion rate had to be finely tuned and if so how are the two...