1. Gravity Flashcards

1
Q

What does Newton’s law of gravity predict about planet orbits?

A

That they orbit the sun in elliptical trajectories

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2
Q

What is Kepler’s first law?

A

That all planet orbits are ellipses

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3
Q

What is Kepler’s second law?

A

Planets sweep out equal areas in equal times
This is due to the conservation of angular momentum

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4
Q

What is Kepler’s third law?

A

The square of the orbital period, P is equal to the cube of the semi major axis, R_a

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5
Q

What is the perihelion of a planet?

A

The point at which it is closest to the sun

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6
Q

What does Newton’s law of gravity fail to predict?

A

The precession of the perihelion of planets due to gravitational interaction

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7
Q

How is the observation of the precession of the perihelion accounted for?

A
  • Most of it due to gravitational pull from different planets e.g. Jupiter
  • Einstein’s GR says the planets move along geodesics in space-time geometry
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8
Q

What is a “prograde” perihelion?

A

A precession in which the direction of the perihelion is in the direction of orbital motion

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9
Q

State Einstein’s equivalence principle

A

Intertial and gravitational masses are the same thing

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10
Q

Describe how the equivalence principle can be applied to the motion of light in frame K and K’ for horizontal motion

A

Frame K (at rest): Light moves along a horizontal line
Frame K’ (Accel. upwards): Light has some deflection below the horizontal line

Equiv. principle: K’ frame is the same as a new frame at rest which is in a gravitational field

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11
Q

What does an observer notice about light that travels vertically upwards in frame K vs K’?

A

Frame K (rest): No change in freq.
Frame K’ (Const accel): Observed freq has changed due to gravitational redshift

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12
Q

How is Newton’s field equation obtained?

A
  • Take the gradient of the potential -GM/r, and F = M grad V.
  • Use Laplace on Green function
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13
Q

Explain how you translaste between Newton’s field equation and Einstein’s equations

A

Laplace = curvature
Potential = space time metric
Mass density = Energy density

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14
Q

What are the two principles of special relativity

A
  • Laws of nature are the same in all intertial frames
  • Speed of light is the same in all inertial frames
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15
Q

Briefly explain the concept of time dilation for a clock in Frame K

A

Clocks that are moving run slowly
- Clock in K measures cT = cT
- Clock in K’ measures cT’ = γcT
- Time elapsed in K’ is longer

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16
Q

What do measurements of the time or distance depend on ?

A

The observer

17
Q

What are invariants and why are they useful

A

Things that are the same in all frames of reference

18
Q

What is the metric of special relativity?

A

Minkowski invariant
(x’-ct’)(x-ct)

19
Q

Explain why the phase of a wave is an invariant quantity

A

The phase counts the number of waves in any wave train and all observers must agree on this

20
Q

Describe the Minkowski s-t geometry

A

Inside cone is time like
Along the cone is light like
Outside cone is space like
Future is above the past

21
Q

State the values of the velocity invariant for space, light and time like trajectories

A

> 0 is space like
=0 is light like
<0 is time like

22
Q

When is a set “space like”?

A

If at every point, every vector tangent to it is space like

23
Q

When is a set “time like”?

A

If there is at least 1 vector tangent to it that is time like

24
Q

Give examples of space and time like sets

A

Space: A plane - ct = ct’ = 0 and sphere -c^2 t^2 + x^2 + y^2 = -R^2
Time: A plane - x= x’ = 0 and sphere -c^2 t^2 + x^2 + y^2 = +R^2

25
Q

What is the Minkowski metric?

A

The covariant η_(μν) type (0,2) tensor. 00=1, 11=22=33 = 1q

26
Q

What is the name of the sign convention for the covariant tensors

A

The signature and we use (-, +, +, +)

27
Q

Explain the similarities and differences between a vector and a tensor

A
  • They both have a magnitude
  • A tensor hcan have several directions whereas a vector just has one
28
Q

What is the proper time?

A

The time measured by an observer who is moving along the trajectory

29
Q

How do free particles travel?

A

In straight lines at constant speeds (N1)

30
Q

Describe how massive and massless particles move in Minkowski space

A

Massive particles move along time like trajectories
Massless particles move along null (light) like

31
Q

What is the stress-energy-momentum tensor

A

The source of the gravitational field in general relativity which replaces the mass of Newton’s theory

32
Q

In the continuity equation, what do the values of mu represent

A

mu = 0 is the conservation of mass
mu = i are the N-S equations

33
Q

State the similarities and differences between the stress energy momentum tensor and the electromagnetic field tensor

A

Both symmetric, type (0,2) and conserved
- EM field is also traceless