Yo ts is not done yet please edit and stuff
Lorentz transformations
Section titled “Lorentz transformations”Special relativity rests on two postulates. The price is that space and time become entangled.
Lorentz transformation. Let frame move to the right with velocity relative to . The coordinates relate by
Three famous consequences follow directly:
- Length contraction. A moving object of proper length is measured to be along the direction of motion.
- Time dilation. A moving clock runs slow by a factor of .
- Loss of simultaneity. If two clocks are synchronized and separated by in , then in the rear clock is ahead by .
The loss of simultaneity is the one beginners forget, and it resolves nearly every “paradox.” Time dilation can be symmetric — each observer sees the other’s clock running slow — precisely because they disagree about which events are simultaneous.
Appearance vs. measurement
Section titled “Appearance vs. measurement”A reference frame is an abstract grid of rulers and synchronized clocks. What an object measures in a frame is not the same as how it looks to an eye in that frame, because light from different parts of the object takes different times to arrive.
For example, a train of rest length moving at speed , viewed by someone off to its right, appears to have length
which is larger than — even though the measured frame length is smaller. (Viewed from the left, the factor inverts.) Once light-travel time is properly accounted for, moving objects actually appear rotated rather than contracted.
Velocity addition
Section titled “Velocity addition”Velocity addition. If an object has velocity in , which moves at relative to , then in
The transverse velocity picks up a factor even though , because of time dilation in the denominator. No combination of sub-light speeds ever exceeds .
Doppler shift and aberration
Section titled “Doppler shift and aberration”Relativistic Doppler effect
Section titled “Relativistic Doppler effect”For a source of proper frequency moving directly toward you at speed , the nonrelativistic shift is modified by the source’s time dilation:
For a source receding, flip the sign of . This second-order correction was first confirmed by Ives and Stilwell.
Aberration and beaming
Section titled “Aberration and beaming”Light emitted at angle to the -axis in comes out at angle in , where
For an ultrarelativistic source (), almost all the radiation is squeezed into a forward cone of half-angle . This relativistic beaming is why decay products at the LHC come out in narrow “jets,” and the same angle change produces stellar aberration — the apparent circular wobble of stars as the Earth orbits.
Paradoxes
Section titled “Paradoxes”Relativistic “paradoxes” almost always smuggle in a nonrelativistic assumption through clever wording. A few classics:
- Twin paradox. Bob rockets away and returns; Alice stays home. Alice ages more. The asymmetry is real: Bob switches inertial frames at turnaround, so his notion of “now on Earth” jumps forward. Working it out with the Doppler effect (counting wave crests each twin receives) gives the aging difference cleanly, and unlike the frame-jump argument, it tracks what each twin actually sees.
- Why lengths contract but times dilate. The Lorentz transformation treats and symmetrically, but the questions we ask are not symmetric: length contraction compares two ends at one time, while time dilation compares one clock at two times. The minus sign in the spacetime interval does the rest.
- Ladder/pole-in-barn, drill-through-wood, etc. All resolved by the relativity of simultaneity: events that are simultaneous in one frame are not in another.
The real lesson of the long, sad history of people (even accomplished scientists) who rejected relativity over the twin paradox: the ability to write fluent prose is not the ability to think. Physicists learn to reason by solving well-defined problems mathematically.
Four-vectors
Section titled “Four-vectors”The cleanest formalism. A four-vector transforms like . The key tool is the inner product, which has minus signs:
This is invariant under Lorentz transformations. The squared interval is the same in every frame.
Four-velocity and four-momentum. Dividing displacement by proper time gives a four-vector (since is invariant). With ,
where and . Their norms are pure invariants:
The relation (restoring : ) is the workhorse of relativistic dynamics — to find an unknown final mass, compute one total four-momentum and take its norm.
Other useful four-vector facts:
- For a photon, so , and where .
- An observer with four-velocity measures a particle’s energy as .
- The inner product of two momenta, , depends only on their relative speed .
- A system’s center-of-mass frame is where total ; it moves at .
Rapidity and acceleration
Section titled “Rapidity and acceleration”A Lorentz boost is a “rotation” mixing space and time. The generalized angle is the rapidity :
The payoff: rapidities simply add when you compose collinear boosts, (compare the messy velocity-addition formula). This makes acceleration problems tractable.
For a rocket with constant proper acceleration (felt onboard), the lab-frame acceleration is , and the rapidity grows linearly with proper time: , so . The clean linear growth is exactly the rapidity-addition property at work.
Energy and momentum
Section titled “Energy and momentum”Relativistic energy and momentum.
Both are conserved. The rest mass is not conserved in inelastic processes (it can grow), while always is — the opposite of the Newtonian situation. automatically includes rest energy and all internal energy.
In dynamics problems, work with and , not velocities. Don’t even mention unless asked.
Worked example (mass from photons). Two photons of energy collide at angle and make a particle. Total four-momentum is , so
Compton scattering
Section titled “Compton scattering”A photon scattering off a stationary electron by angle shifts wavelength by
The shift (the Compton wavelength) is fixed, so it matters most for short-wavelength X-rays and -rays, where it’s a large fractional change.
Optimal collisions
Section titled “Optimal collisions”Threshold principle. For fixed total momentum, the minimum-energy configuration has all particles moving together at a common velocity. Equivalently: at threshold, the products are all at rest in the center-of-mass frame.
Worked example (pion photoproduction). For with a stationary proton, the lab four-momentum is with invariant norm. At threshold the products are at rest in the CM frame, with norm. Equating,
A little above the pion rest energy, because the products carry off kinetic energy.
To make a proton–antiproton pair via on a stationary target, the required kinetic energy of the beam scales much worse than the rest energy produced — which is exactly why colliders use two opposing beams rather than a fixed target.
Mass–energy and relativistic systems
Section titled “Mass–energy and relativistic systems”The deep content of is that internal energy is mass. Heat up a box of gas and it has more mass in every sense: more inertia, more weight, more gravitational pull. A box of photons bouncing inside reflective walls has rest mass even though each photon is massless.
In relativity the center of mass is not well-defined (a massless photon has no location to weight). Instead there’s a center of energy, and the general result is
reducing to nonrelativistically. A related and very general fact: momentum density equals energy-flux density (in EM, the momentum density is the Poynting vector, in units ).
Forces in relativity
Section titled “Forces in relativity”There are two notions of force, and you must keep them straight.
Three-force
Section titled “Three-force”Define (not — the two differ relativistically). For a particle moving along ,
so force is generally not parallel to acceleration. Transforming from the particle’s momentary rest frame to the lab,
longitudinal force is unchanged, transverse force is reduced by . This holds for any force.
Four-force
Section titled “Four-force”A “pure” force keeps the rest mass fixed, which requires . (Putting a system on a stove changes its mass without changing momentum — a valid four-force, but not a “pure” one.)
The Lorentz force and circular motion
Section titled “The Lorentz force and circular motion”The Lorentz force is a pure three-force.
Worked example (collider field). For protons of energy in a ring of radius , the centripetal force is with and . The magnetic force supplies it, so
For the LHC ( TeV, km) this gives T, and since at fixed , reaching 20 TeV needs a 12 km ring.
The slick way to express the Lorentz force as a four-force is via the antisymmetric field-strength tensor (built from and ), with . Its antisymmetry automatically guarantees , i.e. fixed rest mass.
Electromagnetic field transformations
Section titled “Electromagnetic field transformations”The biggest payoff of relativity for E&M: and are two faces of one object, and a boost mixes them.
Field transformations. Boosting with velocity , the components parallel to are unchanged,
while the perpendicular components transform as
These keep Maxwell’s equations valid in every inertial frame, and total charge stays invariant under boosts. A clean way to remember the piece: boosting a capacitor length-contracts its plates, raising the charge density and thus the field.
Field of a moving charge
Section titled “Field of a moving charge”A charge moving at constant velocity has a field that is still exactly radial, but squashed:
where is measured from . The field lines pile up perpendicular to the motion (contracted by along ) — this is literally what inspired Lorentz and FitzGerald to propose length contraction. The accompanying magnetic field is exactly
If the charge suddenly changes velocity, the “news” propagates outward at : outside an expanding sphere the field still points to where the charge would have been, and the kink between old and new fields is the radiated pulse.
Invariants
Section titled “Invariants”Out of and you can build two Lorentz invariants:
Consequences: if and in one frame (a light wave), that holds in all frames. If but somewhere, no boost can make vanish there (since is invariant).
Covariant form
Section titled “Covariant form”The charge and current densities form a four-vector , charge conservation is , and all of Maxwell’s equations compress to (with ). Elegant notation is a tool, not a religion — index notation wins because it works whenever indices contract in pairs.
Charges in fields: potentials and canonical momentum
Section titled “Charges in fields: potentials and canonical momentum”The fields come from a scalar potential and vector potential :
Canonical momentum. By Noether’s theorem, a symmetry gives a conserved quantity. For a charge in static fields, time-translation symmetry conserves energy , and (partial) space-translation symmetry conserves the canonical momentum
The term is a kind of “potential momentum,” analogous to potential energy . The power of this: even when fields and motion are complicated, if and are independent of , then is conserved. For rotational symmetry about , is conserved (using the canonical ). The relativistic versions hold with .
This is the right tool for adiabatic-invariant problems in magnetic fields (e.g. the betatron, slow changes of on an orbiting charge), and it’s the hidden conserved quantity behind several “magic” Olympiad solutions.
Gravitation and the equivalence principle
Section titled “Gravitation and the equivalence principle”Equivalence principle. A uniform gravitational field is locally indistinguishable from a uniformly accelerating frame, in all contexts. This was the seed of general relativity.
Gravitational redshift
Section titled “Gravitational redshift”Send a photon of frequency upward a height in field . Thinking of mass–energy conservation (photons “lose mass-energy” climbing) gives a fractional frequency drop
Since photon frequency is a clock, this means clocks deeper in a potential run slow by a factor . The same result follows from the equivalence principle (two accelerating observers see a Doppler shift) and was confirmed in the 1959 Pound–Rebka experiment using -rays sent down a 22.5 m tower.
Clocks, GPS, and combined effects
Section titled “Clocks, GPS, and combined effects”A real clock (e.g. on a satellite) feels two competing effects:
- Special-relativistic time dilation from its orbital speed (makes it run slow).
- Gravitational time dilation from sitting higher in the potential (makes it run fast).
For GPS satellites the gravitational effect dominates, and both must be corrected for the system to work. On the Earth’s surface, gravitational redshift also implies a vertical system in thermal equilibrium has a tiny temperature gradient (the Tolman gradient) — usually negligible.
A note on visualizing GR
Section titled “A note on visualizing GR”In general relativity gravity is spacetime curvature: freely falling objects move in straight lines (geodesics), and what we call “gravity” is the constant upward acceleration of the ground pushing us off those geodesics. The rubber-sheet picture is a poor analogy (it secretly assumes gravity to make things roll downhill); the “river model” — space flowing inward, with the event horizon where it flows faster than light — captures more, but no simple analogy is the theory. The equations are the theory; analogies are stories we tell our animal-descended minds.
Problem-solving strategy
Section titled “Problem-solving strategy”Match the question to the cleanest invariant or transformation before grinding through algebra: