Jump to content

Genady

Senior Members
  • Posts

    5373
  • Joined

  • Days Won

    52

Everything posted by Genady

  1. Some years ago while diving around the island where I live I've noticed that this coral always makes a right-handed helix. I wonder if it might be an adaptive feature or, more generally, what could cause it. I mean, I saw dozens of them and never one turning left...
  2. I hope you will enjoy this video as well. Susskind presents an example of dark matter mass calculation starting at about 31st minute. (Only stuff inside an orbit has gravitational effect on the orbit.)
  3. R in this calculation stands for distance from origin. Which of course is arbitrary. As Susskind has shown in his derivation, the final result does not depend on R. No, that calculation doesn't have such flexibility. The observable effects of dark matter lead to calculation of not only it's mass - positive - but also of its amount and distribution. The only observable effect of dark energy is acceleration of the universe expansion.
  4. Correct again. All effect for the smaller R's add up. All effect s for the larger R's cancel.
  5. Right, it doesn't have an effect inside the sphere, it does have the effect outside it.
  6. Dark matter and dark energy are separable in a variety of ways. Dark matter attracts, dark energy repulses. Dark matter density falls off with a cube of expansion, dark energy density doesn't change with expansion. Dark matter non-uniformities accelerate clamping of regular matter, dark energy doesn't have such effect. ...
  7. By the Newton's theorem, a particle inside an empty massive sphere doesn't feel any gravity from the sphere. It holds the same for positive and for negative gravity. Neither positive nor negative mass homogeneously distributed outside galaxy have any gravitational effect on the galaxy.
  8. Sorry for the misunderstanding. I was kidding. Such headlines, I guess, are just click baits. Thought about it because the thread topic mentions impressing scientists. I don't enjoy claiming that scientists are easily shocked but rather enjoy making fun of popular science reports.
  9. Evidently, scientists are easily shocked: Scientists Shocked by Discovery of Enormous, Healthy Coral (futurism.com) Climate scientists shocked by scale of floods in Germany | Flooding | The Guardian Scientists 'shocked' by high levels of microplastic pollution in London's Thames (nbcnews.com) Scientists shocked by Arctic permafrost thawing 70 years sooner than predicted | Climate crisis | The Guardian Scientists shocked by mysterious deaths of ancient trees - BBC News Scientists shocked to discover how much lightning may clean the atmosphere | CBC Radio Scientists Shocked By Rare, Giant Sunfish Washed Up On California Beach : NPR Italian scientists shocked by earthquake devastation | Nature Scientists ‘shocked’ to find life in extreme depths under Antarctic ice - National | Globalnews.ca Scientists 'shocked' after second coral bleaching at Great Barrier Reef in two years - CNN ... the list goes on and on.
  10. A friend has sent this question to me. I have it solved with linear algebra (and some hand waving). Can you find a shorter way to the answer? (It's not a homework, not mine anyway. My homework times long gone.) A gardener collected 17 apples. He finds that each time he removes an apple from his harvest, he can share the remaining fruit in two piles of equal weight, each containing 8 apples. Show that all apples are the same weight.
  11. No, position and time are described by real numbers in QM.
  12. It is true. For observer 1, a particle P is at rest and a particle Q accelerates toward it. For observer 2, Q is at rest and P accelerates toward it. Susskind answers exactly this question in the lecture that I've linked in the post above yours.
  13. An easy derivation, with answers to the audience's questions relevant to the above discussion, can be found here, starting about 30 minutes into the lecture:
  14. The center is just an origin of coordinates. Of course, the premise is homogeneity and isotropy of the entire space. For any coordinate system, a particle in its origin does not move anywhere, but all other particles accelerate toward it. The same as in the Hubble expansion.
  15. Each particle is attracted equally from all directions, and these will cancel indeed. But, each particle attracts all other particles and they will all accelerate toward it. This is so for all particles and thus all particles accelerate toward each other. So, the entire thing homogenously and isotropically contracts, or slows its expansion. For a bit more precise treatment, take any particle as a center and consider particles on a sphere of radius R around it. Each particle on the sphere, according to the old Newton's theorem that holds in GR as well, is attracted to the center as if the mass of the entire ball of radius R is in the center, and effect of each larger sphere on it is 0. This holds for any point picked as a center. The fully precise result in GR follows from increasing mass density in Friedman equation.
  16. Yes, it would cause a net gravitational attraction and that would cause slowing of the universe expansion.
  17. Not proved, according to this: "In discussions of the cosmological constant, the Casimir effect is often invoked as decisive evidence that the zero-point energies of quantum fields are “real.” On the contrary, Casimir effects can be formulated and Casimir forces can be computed without reference to zero-point energies. They are relativistic, quantum forces between charges and currents. … I have presented an argument that the experimental confirmation of the Casimir effect does not establish the reality of zero-point fluctuations. Casimir forces can be calculated without reference to the vacuum ... . The vacuum-to-vacuum graphs (See Fig. 1) that define the zero-point energy do not enter the calculation of the Casimir force, which instead only involves graphs with external lines. So the concept of zero-point fluctuations is a heuristic and calculational aid in the description of the Casimir effect, but not a necessity." Casimir effect and the quantum vacuum R. L. Jaffe Phys. Rev. D 72, 021301(R) – Published 12 July 2005
  18. If there were much more of it around, it would affect the cosmological expansion. Perhaps it could be detected this way.
  19. The distribution of the DM in space now is very much non-uniform. Since it doesn't clump, was its distribution as non-uniform soon after the BB?
  20. Is it necessarily so? If it could interact electromagnetically by completely reflecting an EM radiation it wouldn't emit a thermal EM radiation, would it?
  21. Many think that it interacts not only via gravity but also weakly, i.e. made of WIMPs.
  22. I don't know why it's called dark, but not interacting electromagnetically makes it rather transparent than dark.
  23. We also know that it was there by the time of "recombination", about 380 000 years after the Big Bang.
  24. We know where it is and how much of it is there. We don't know what it is.
  25. Nice. Except the very last statement. That is a kind of "wishful thinking" fallacy.
×
×
  • Create New...

Important Information

We have placed cookies on your device to help make this website better. You can adjust your cookie settings, otherwise we'll assume you're okay to continue.