General Relativity Definitions Flashcards

1
Q

Covariant derivation?

A

Differentiation that accounts for the changing basis vectors as you move across a Reimannian manifold.

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2
Q

Local inertial frame?

A

A frame that is Minkowskian in the local region. In general relativity we can always transform into this frame.

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3
Q

Gravitational Lensing

A

Light moves along geodesics that curve around massive objects, distorting the image into a ring.

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4
Q

Weak equivalence principle?

A

No experiment can distinguish between free-falling in a gravitational field and uniform motion in free-space.

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5
Q

Strong equivalence principle?

A

No experiment can distinguish between acceleration in free-space and being held in a gravitational field.

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6
Q

Gravitational redshift?

A

From the WEP, the local inertial frame of light aquires motion towards the gravitating body, stretching the wavelength of light as it clmibs out of the gravitational potential.

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7
Q

Deflection of light by the sun?

A

Spacetime curvature causes null geodesics to be bent at twice the angle expected by naive application of the WEP.

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8
Q

Perihelion precession?

A

An elliptical orbit close to a massive object is distorted: the exterior focal point precesses about the interior.

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9
Q

Shapiro light delay?

A

An observer will see light moving along null geodesics in a curved manifold take longer than predicted by the Minkowski metric.

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10
Q

Parallel transport?

A

A vector is transported along a manifold such that its angles with the local basis vectors are preserved.

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11
Q

Reimann tensor?

A

Describes the curvature over smooth manifolds.

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12
Q

Line elements for Reimannian surface?

A

Describes the infintesimal distance bewteen points on a smooth manifold, as a sum of products of basis vectors.

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13
Q

Metric tensor?

A

A rank 2 tensor that describes the changes in basis vectors of a manifold as a function of its coordinates. It is used to derive the line element.

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14
Q

Affine geodesic?

A

A curve which follows the tangent vector to the curve at every point as it’s parallel transported along itself. In torsion-free manifolds this is equal to metric geodesics.

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15
Q

Confomally flat metric?

A

A metric that can be trnasformed into a flat metric via a conformal transformation (a transformation which preserves internal angles).

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16
Q

Reimannian manifold?

A

A smooth manifold described by a metric tensor. The set of all tangent vectors at all points form a vector space.

17
Q

Birkhoff’s theorem.

A

Any spherically symmetric mass distribution must be static & described by the Schwarzchild metric.

18
Q

Metric geodesic?

A

A spacetime path which minimises spacetime separation between two points.

19
Q

Event horizon.

A

Constant acceleration defines spacetime regions where light cannot reach you, and you become causually disconnected from these region.

20
Q

Black holes.

A

An object (dead star) that has shrunk below it’s Schwarzchild radius, which becomes an event horizon. The region below the horizon is causually disconnected to the rest of the universe.

21
Q

Coordinate transform?

A

A relation between coordinate systems described by a Jacobian matrix, which details the relations between old & new basis vectors.

22
Q

Torsion.

A

The spacetime twisting of coordinate systems, not present in classical GR. Its nonclusion allows for affine & metric geodesics to be equated, and for certain symmetries in the curvature tensors.

23
Q

Geodesic deviation?

A

The divergence/conbpvergence of geodesics through negative/positive curved spacetimes.

24
Q

Isometry?

A

An isometric tensor is equal in all frames-of-reference. In coordiante transformations it preserves distances (equivalent to how confromal transformations preserves angles).