Introduction Flashcards

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1
Q

elementary particles

Which are the matter particles and how do we classify them?

A

Leptons: electron, muon, tau + corresponding neutrinos

Quarks: up, down, strange, charm, bottom, top

  • first three: light quarks, second three: heavy quarks

All of them are spin-1/2 fermions and they’re further classified into families/generations.

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2
Q

elementary particles

Which are the interaction particles? Which interactions to they mediate?

A

Photon: EM-interaction, massless
W(+/–), Z bosons: weak interaction, massive
Gluon: strong interaction, massless
Higgs-boson: gives mass to elementary particles (exc. photons and gluons), massive

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3
Q

interactions as particle exchange

What does a particle interaction mean in practical terms? What’s the problem with this? What’s the solution?

A

It means the exchange of mediator particles carrying just the right amount of the various quantum numbers.

Problem: when a particle is exchanged the energy and the momentum can’t be conserved simultaniously, which leads to serious contradictions from a classical perspective

Solution: Heisenberg’s uncertainty principle. The interaction can violate energy conservation for Δt ~ ħ/ΔE span of time

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4
Q

interactions as particle exchange

What does the range of interaction of particles mean? What determines it?

A

Range of interaction: inverse of the mass of the lightest mediator particle

  • so the determining factors are Heisenberg’s uncertainty principle and therefore the lightest mediator particle
  • Compton-length: Δx = cΔt, the particle can go as far as it would in Δt time if it had c velocity
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5
Q

interactions as particle exchange

What determines the strength of interactions?

A

The likeliness of absorption or emission which is described by the coupling constant.

  • the larger the coupling, the higher the chance
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6
Q

natural units

What are the natural units?

A

ħ = c = 1, e = 1

  • e is also dimensionless
  • c —» [m] = [E] (unit of mass = unit of energy)
  • ħ —» [t] = 1/[E] (unit of time = unit of inverse energy)
  • ħc —» [l] = [t] = 1/[E] = 1/[m] (unit of length = unit of time = …)
  • ħc = 197 MeV for the conversion
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7
Q

building up matter

How do the elementary particles build up the known matter? How are mesons and baryons constructed?

A
  1. quarks —» hadrons: strong interaction
  2. hadrons —» nuclei: strong interaction
  3. nuclei + electrons —» atoms: EM interaction

Construction of hadrons: same quark content but different spin/angular momentum state means different mesons, different quark content means different hadrons

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8
Q

building up matter

What’s the lightest baryon and why is it stable?

A

It’s the proton, which ensures the stability of ordinary matter. It’s stable exactly because it’s the lightest: there’s nothing for it to decay into because of the conservation of baryon number.

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9
Q

stable and unstable particles

Which are the stable particles and what are some properties of the unstable ones?

A

Stable particles: protons, electrons, neutrinos, photons

Unstable particles: everything else

  • lifetime: typical mean time it takes a particle to decay
  • decay width: inverse of lifetime, energy dimension
  • decay channel: particles decay through different modes and each mode is a channel
  • partial width: characterization of each channel
  • branching ration/fraction: the relative probability of a decay happening in a certain channel
  • exponential decay law: insert képlet
  • energy conservation is independent of the frame of reference: the sum of the decay products cannot exceed the initial particle’s mass
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10
Q

decays and conservation laws

How can we tell which process governs which interaction?

A

By lifetime: strong —» EM —» weak (increasing lifetime from left to right)

  • also corresponds to the strength of the interaction decreasing with the increasing lifetime
  • signature particles: (anti)neutrinos (weak), photons (EM), pions (strong)

By conservations laws: all interactions conserve electric charge, baryon number and lepton number, but not all conservation laws are valid for all interactions in general

  • generally they’re related to the symmetries of the systems through Noether’s theorem
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11
Q

decays and conservation laws

What conservation laws are there and how can we categorize them? Which elementary interaction conserves them?

A

Particle-type conservation laws:

  • baryon number
  • strangeness, charm, beauty, upness, downness, topness
  • lepton number, individual lepton numbers, lepton family number
  • electric charge

Approximation of flavour symmetries: only the masses distinguish the different flavoured quarks in terms of the strong interaction, isospin can be introduced (more on a different card)

Discrete symmetries:

  • parity: spatial inversion
  • charge conjugation: exchange of particles with antiparticles
  • time reversal: inversion of the direction of time
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12
Q

decays and conservation laws

What is isospin and what does it represent?

A

It’s a type of internal symmetry (formulated analogously to spin), meaning it acts in the internal space spawned by the up and down component of the quark state.

  • different flavoured quarks can be “rotated” into each other without physical effects: rotational symmetry
  • completely different from spacial symmetries (only mathematically identical)
  • it manifests through multiplets (like the degeneracy of the energy levels): I = (I1, I2, I3), I3 = -I,…,I, I3 = (1/2)(baryon number + S)
  • only conserved by the strong interaction
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