I guess the title says it all: how could/would you experimentally test whether our universe is truly time reversal invariant, without relying on the CPT theorem? What experiments have been proposed to check this? Have any of them been performed?
I know that there are indirect tests of time rever...
Since removing the point you have that the polar coordinates from $\mathbb{R}_{>0}\times S^2$ cover it and there is a diffeomorphism $\mathbb{R}_{>0} \to\mathbb{R}$.
About five minutes before I posted this, a question came up in the feed asking users to come up with innovative project ideas for a highschool project with a photoresistor. The question had no research, and it was posted originally without a homework tag. While this question was deleted (maybe a ...
@Obliv :-) People take things very seriously when they're young. It's only when you get to my advanced age you decide it's much more fun to just bugger about :-)
@0celo7 leaving aside time for the moment, I can describe space with the usual polar coordinates $r$, $\theta$, $\phi$. And constant $r$ is the submanifold $S^2$. So why can't I foliate all of space as $R \times S^2$?
@0celo7 Use Poincaré duality and that the homology of spheres is $H_n(S^n) = \mathbb{Z}, H_0(S^n) = \mathbb{Z}$ and zero otherwise. Then use homotopy invariance to contract the $\mathbb{R}$ to a point.
I do not remember precisely what the equations or who the relevant mathematicians and physicists were, but I recall being told the following story. I apologise in advance if I have misunderstood anything, or just have it plain wrong. The story is as follows.
A quantum physicist created some e...
So does every other satellite have roughly same orbit ? Also does the moons of other planets have rouhly same orbit ?
user54412
5:56 PM
@ritwiksinha Roughly, but some of them are more exotic. Note the spiraling pattern everyone mentions is not what the Moon looks like. Well, Jupiter's orbital speed is 13 km/s, while its moon Io goes around at 17 km/s. Thus for part of its orbit Io is in fact going backward around the Sun.
I do not remember precisely what the equations or who the relevant mathematicians and physicists were, but I recall being told the following story. I apologise in advance if I have misunderstood anything, or just have it plain wrong. The story is as follows.
A quantum physicist created some e...
Not even light can pass through a toroidal black hole before the hole closes up, so the question is moot.
To set the stage for why toroidal black holes are interesting, I'll start with Hawking's 1972 result that "a stationary black hole must have topologically spherical boundary." That is, once ...
user54412
Unless you're including the whole thing inside the horizon too. In which case, are they supposed to be the same?
am a bit surprised you guys dont like the question/ answers, its like a big ad for physics on the math site, and youre all kneedeep in math etc, it highlights/ unifies key discoveries etc
Some of its objects - like the M2- and M5-branes - are known by finding their corresponding objects in the limiting cases and noting they are stable against smooth deformations ("BPS states")
@0celo7 That's what one calls these states that are safe against perturbative corrections and hence should still be present in the full non-perturbative theory
They usually fulfill some extremality condition
Kind of like the masslessness of a vector boson in QFT- also an extremal mass condition - inherently protects it against acquiring mass
@0celo7 I'm not sure how to answer that briefly. There is usually a significant function of mass and charge of an object associated to that object, and there's something special about when this function becomes extremal - for example, the number of the allowed fields living on it change, and this cannot be a smooth transition, so if the object is sitting there at weak coupling it must also be there at strong coupling.
@0celo7 You do not know that all massless vector bosons are gauge bosons and protected from acquiring mass by gauge symmetry? Shame on you! ;P
A single representation is a group morphism from the group to the group of automorphisms of some vector space
If you mean matrices with $M(n)$, then you have excluded all infinite-dimensional representations, in particular the entire quantum theory of the Lorentz group :P
So the Green's function in curved spacetime is $$G(x,y) = \sum_\gamma \frac{\Delta_\gamma (x,y)^{\frac{1}{2}}}{4\pi^2} [\frac{1}{\sigma_\gamma(x,y)} + v_\gamma(x,y) \ln |\sigma_\gamma(x,y)| + \varpi_\gamma (x,y)]$$