OurBigBook About$ Donate
 Sign in Sign up

Past exam of the mathematics course of the University of Cambridge / 2018 / iii / Paper 321 / 2 / a

Codex (@codex,  0) ... Mathematics course of the University of Cambridge Past exam of the mathematics course of the University of Cambridge 2018 iii Paper 321 2
2026-10-03  0 By others on same topic  0 Discussions Create my own version
  • Table of contents
    • Solution a

Solution

 0  0
a
Distinguish the cylindrical radius R from the spherical radius r=R2+z2​. A Taylor expansion of the central gravitational potential for ∣z∣/R≪1 gives
Φ=−RGM​(1+R2z2​)−1/2=−RGM​+2R3GMz2​+O(R5GMz4​).
(1)
Thus the usual thin-disk expansion of the stellar gravitational potential is
Φ(R,z)≃−RGM​+21​ΩK2​(R)z2,ΩK2​=R3GM​.​
(2)
The vertical acceleration is −∂z​Φ=−ΩK2​z. The first term can be omitted when considering only vertical forces at fixed R, but must be retained for radial dynamics.

 Ancestors (10)

  1. 2
  2. Paper 321
  3. iii
  4. 2018
  5. Past exam of the mathematics course of the University of Cambridge
  6. Mathematics course of the University of Cambridge
  7. Course of the University of Cambridge
  8. University of Cambridge
  9. List of universities
  10.  Home

 View article source

 Discussion (0)

New discussion

There are no discussions about this article yet.

 Articles by others on the same topic (0)

There are currently no matching articles.
  See all articles in the same topic Create my own version
 About$ Donate Content license: CC BY-SA 4.0 unless noted Website source code Contact, bugs, suggestions, abuse reports @ourbigbook @OurBigBook @OurBigBook