Geodesics Flashcards

(39 cards)

1
Q

What is a geodesic?

A

The path that extremizes the interval (ds) between two points in spacetime.

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2
Q

What equation defines a geodesic?

A

d²x^μ/dλ² + Γ^μ_{νρ} dx^ν/dλ dx^ρ/dλ = 0.

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3
Q

What is the affine parameter?

A

A parameter λ that varies linearly with proper time or arc length.

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4
Q

What is the geodesic equation for null paths?

A

Same as for timelike, but ds² = 0.

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5
Q

What is the physical significance of a geodesic?

A

It is the trajectory of a freely falling particle or light ray.

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6
Q

What happens to a particle in free fall in GR?

A

It follows a geodesic of the spacetime.

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7
Q

What is the difference between geodesics and straight lines?

A

In curved spacetime, geodesics generalize straight lines from flat space.

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8
Q

What is the Euler-Lagrange equation applied to geodesics?

A

It yields the geodesic equation when extremizing the action S = ∫ds.

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9
Q

What is the Lagrangian for a geodesic?

A

L = g_{μν} dx^μ/dλ dx^ν/dλ.

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10
Q

How is the geodesic equation derived?

A

From the Euler-Lagrange equations applied to the line element or action.

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11
Q

What does parallel transport along a geodesic mean?

A

A vector remains constant in direction along the geodesic.

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12
Q

What is a timelike geodesic?

A

A geodesic where ds² < 0; represents a massive particle’s path.

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13
Q

What is a spacelike geodesic?

A

A geodesic where ds² > 0; not traversable by particles.

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14
Q

What is a null geodesic?

A

A path with ds² = 0; followed by light or massless particles.

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15
Q

What quantity is conserved along a geodesic with a Killing vector?

A

ξ^μ u_μ = constant (projection of velocity onto symmetry direction).

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16
Q

What does the geodesic equation simplify to in flat space?

A

d²x^μ/dλ² = 0 — straight line motion.

17
Q

What is the conserved quantity in static spacetimes?

A

Energy: E = -g_{tt} dt/dλ (if g_{tt} is time-independent).

18
Q

What is the geodesic deviation equation?

A

Describes how nearby geodesics diverge: D²ξ^μ/Dλ² = R^μ_{νρσ} u^ν ξ^ρ u^σ.

19
Q

What is the meaning of geodesic deviation?

A

Tells how tidal forces act — nearby free-fall paths change due to curvature.

20
Q

What is a proper parameterization of a timelike geodesic?

A

Proper time τ, such that u^μ = dx^μ/dτ and u^μ u_μ = -1.

21
Q

What is u^μ?

A

The four-velocity: u^μ = dx^μ/dτ for a particle moving along a timelike path.

22
Q

What does ‘affinely parameterized’ mean?

A

The parameter λ is such that the geodesic equation takes its standard form.

23
Q

What is the geodesic Lagrangian for null paths?

A

L = g_{μν} dx^μ/dλ dx^ν/dλ = 0.

24
Q

What is a ‘first integral’ of the geodesic equation?

A

A conserved quantity derived from a symmetry, like energy or angular momentum.

25
How is a circular orbit condition derived from geodesics?
Set radial velocity and radial acceleration to zero in the effective potential.
26
What is the variational principle for geodesics?
δ∫ds = 0 for the geodesic path between two events.
27
Why are geodesics important in GR?
They describe the motion of test particles and light in curved spacetime.
28
What role do Christoffel symbols play in geodesics?
They appear in the geodesic equation and encode the effects of curvature.
29
What is a radial geodesic?
A geodesic with no angular motion — purely in r and t coordinates.
30
How do geodesics differ for massless and massive particles?
Massive: timelike geodesics (ds² < 0); massless: null geodesics (ds² = 0).
31
What is a coordinate singularity in geodesics?
An apparent singularity due to bad coordinates, not real curvature.
32
What is the effective potential in geodesic motion?
A potential V_eff(r) derived from conserved quantities and the metric.
33
What is the condition for light deflection in GR?
Light follows null geodesics which are curved by spacetime curvature.
34
What is the turning point of a geodesic?
Where dr/dλ = 0 — occurs at extrema of effective potential.
35
What is the angular momentum of a geodesic?
A conserved quantity if the spacetime is spherically symmetric: L = r² dφ/dλ.
36
What is the relation between geodesics and gravity?
Gravity in GR is the curvature that causes geodesics to deviate from straight lines.
37
Can we always find geodesics numerically?
Yes, by solving the system of second-order ODEs given by the geodesic equation.
38
What are initial conditions for geodesic motion?
Initial position and velocity vector (u^μ), satisfying normalization constraints.
39
What is the norm of the four-velocity u^μ?
u^μ u_μ = -1 for timelike, 0 for null, +1 for spacelike.