Past exam of the relativity course of the University of Cambridge 2019 Section B B4 Solution 2026-10-18
Use signature and local inertial coordinates . Write and , where is rest mass density. The perfect fluid in general relativity has componentsHere is energy density, is energy flux, is momentum density, and is the flux of the th momentum component through a surface normal to . In the local rest frame these reduce to energy density , zero energy and momentum flow, and isotropic pressure . The equation expresses local stress-energy conservation. Its temporal and spatial components give energy and momentum balance; in flat coordinates, for example, .
For relativistic dust, . Contracting its divergence with , and using metric compatibility together with , givesConsequently . Substituting this continuity equation back into the divergence leaves . Wherever matter is present,so the individual particles follow geodesics.
The electromagnetic four-force law must preserve the particle's rest mass. Thus , and requiring this for arbitrary timelike four-velocities makes the electromagnetic field tensor antisymmetric. Its six independent components comprise the electric field and magnetic field. With the stated signature and , one consistent convention isIt gives the spatial force and energy transfer . Under a Lorentz transformation, transforms as a rank-two contravariant tensor; its electric and magnetic components consequently mix. A four-potential supplies , unchanged by . The Maxwell equations areThese combine the source equations and the homogeneous equations into covariant tensor statements; is the four-current.
For charged relativistic dust, the matter tensor exchanges four-momentum with the electromagnetic field: , while their total stress-energy tensor is conserved. Identical particles of rest mass and electric charge have . Contraction with again gives mass continuity because . Removing that term givesUsing zero divergence for the matter tensor alone in this last step would omit the electromagnetic Lorentz force.
Past exam of the relativity course of the University of Cambridge 2022 Section B 5 e Solution 2026-10-18
Measure in the orthonormal tetrad of a static observer at . This specifies the local frame needed to define an angle. If is the conserved photon energy, gravitational redshift gives . The tangential local momentum is , so the impact parameter isInside the photon sphere, an outward ray must have to cross the potential barrier. The Schwarzschild photon escape cone therefore has critical half-angleThe upper bound is strict: a critical ray only approaches the circular orbit. At , the critical half-angle is , and exactly tangential light is circular. As , the cone shrinks to zero opening. No static observer exists exactly on the Schwarzschild event horizon, and no future-directed photon emitted there escapes to exterior infinity; the zero-angle result is an exterior limit.
Compton scattering transfers energy and momentum from a photon to an electron. For an initially stationary, approximately free electron, a photon scattered through a nonzero angle generally has lower frequency and longer wavelength; the recoiling electron carries the difference. The effect demonstrates the photon momentum , beyond a purely elastic classical scattering description.
The middle panel of the figure in solution shows the incident photon along , the outgoing photon at angle above that direction, and the recoiling electron at deflection angle below it. Each arrow labels its particle and momentum; the initial electron is at rest at the interaction point. The scattered photon and electron have opposite transverse momentum components, while their forward components sum to the incident photon momentum.
An electron accelerated from negligible initial kinetic energy through gains . The largest possible single photon energy in an X-ray tube is this entire kinetic energy, so the Duane-Hunt law givesThe massive anode can absorb the required recoil momentum with negligible recoil energy; most actual events produce lower-energy bremsstrahlung photons. The acceleration energy is valid without approximating the electron speed nonrelativistically.
Work in the initial rest frame of the free electron. If it absorbed a photon of positive energy , conservation of momentum would give the final electron momentum magnitude , while conservation of energy would give . But the final electron must obey the relativistic energy–momentum relation,Combining these statements giveswhich contradicts . ThusThe initial rest frame always exists for an electron, so this excludes the process in every inertial frame. Compton scattering is allowed because an outgoing photon carries additional energy and momentum. Absorption by an electron bound in matter is also possible because the rest of the system can share recoil.
Applying the Hamiltonian operator to gives , and thereforeThe ground state has zero kinetic energy. Every positive energy level is of quantum degeneracy two, because and correspond to opposite angular momenta with equal squared magnitude.
The confinement scale suggests a tangential momentum scale and thus an excitation energy scale , consistent with the Heisenberg uncertainty principle. More precisely the de Broglie wavelength must fit an integer number of times around the circumference: , so . This explains both the dependence and the sequence.
One must not infer a nonzero ground-state energy by applying naively. Angle is periodic and is not a globally canonical position operator on the circle. The uniform wavefunction, with , is a concrete counterexample to that naive inequality. The ordinary Cartesian Heisenberg uncertainty principle is not violated by the zero-angular momentum state.
Let be radial position, the outward radiative energy flux, and the radiation pressure. A thin layer absorbs a fraction of an incident directed beam. Since a photon carries momentum , the outward force per unit volume deposited by the radiation is . Balance it against the radiation pressure gradient:Substituting yields the radiative diffusion equationThe sign expresses outward energy flux down the temperature gradient. The approximation assumes optically thick material and near local thermodynamic equilibrium, with an appropriate mean opacity.
The printed attenuation law describes the loss from an incident beam; it is not generally the radial derivative of the net luminosity, since absorption is accompanied by emission. For a concrete counterexample, in a steady envelope without local energy generation the net luminosity is constant even though and . Applying to that net luminosity would contradict energy conservation. The local momentum deposition argument supplies the physically correct derivation.