1. Relativistic Kinematics
1. Costituents of Matter
2. Fundamental Forces
3. Particle Detection
4. Symmetries and Conservation Laws
5. Relativistic Kinematics
6. The Quark Model
7. The Weak Interaction
8. Introduction to the Standard Model

2. Recalling Relativistic Kinematics (Special Relativity)
Basic Principles
Every experiment will give the same results whenever executed in reference frames that are in uniform rectilinear motion with respect to one another.
Physical laws are the same in every inertial frame.
Energy, total momentum and total angular momentum of a physical system are constant in time.
The speed of light in vacuum is the same in every inertial frame : c=2.9979108 m/s
(Time is not a relativistic invariant)
(Space is not a relativistic invariant)

3. Four-vector :
For example, for a particle
Minkowski pseudo-euclidean metric
Scalar product:
Lorentz transformations
Given 2 inertial frames Oxyz, Ox’y’z’ in relative motion and assuming that the origin of the axis coincide at a common t=t’=0 and also assuming that the uniform translatory motion be along the x axis:
β=vx/c with vx velocity di O’ rispetto a O e con γ=1/(1-b2)1/2
By applying a Lorentz transformation L(b) to a four-vector A in the system O, one gets A’ in the O’ system:

4. The Lorentzian four-vector :
The Special-Relativity spacetime :
The Lorentz Boost :

5. A prototype reaction
Dispersion Relations
In the LAB
4-momentum conservation
In the CM
3-momentum
Energy conservation
Center of Mass Energy
Maximal energy that can be transformed in mass

6. In a fixed-target configuration :
At high energies (masses neglected) :
In a collider situation :
Let’s assume
At high energies (masses neglected) :

7. Sum of masses in the final state Threshold of a Reaction
Example 1: production of a muon with a neutrino beam impinging on e
Muon mass
Example 2: muon production in e+e- collisoins (collider)
Two muons to conserve leptonic numbers

8. Unstable particle: two-body decay
In the M rest frame
in this section only
Possible only if
Momentum uniquely defined

9. …and the energies of the two particles
and, similarly :
Because of momentum conservation, 1 and 2 are heading in opposite directions in the M reference frame
If 1 and 2 happen to have the same mass :

10. Two body decays in flight in this slide
2-vectors
Momentum conservation in the transverse direction :
Between the CM and the laboratory :
Kinetic energy and mass energy :

11. Mandelstam variables
Let’s introduce three Lorentz scalars :
Only two of them are independent :

12. Physical meaning of s: energy available in the center-of-mass
In the case of an unstable particle decaying :
Physical meaning of t: let us see it in the CM
Θ*< 900
Momentum transfer

13. Elements of Collisions Theory for the specific case of :
Classical Collisions
Mass is conserved
3-momentum is conserved
T may or may not be conserved
T decreases (it can be transformed into heat
or chemical energy) . Extreme case: A+BC
(two particles sticking together).
T increases (internal energy is released).
Extreme case: AC+D (a particle breaks up)
Classical Elastic Collision
Because of the conservation of mass, the extreme cases need to be :

14. Relativistic Collisions
Energy is conserved
3-momentum is conserved
T may or may not be conserved
T decreases (rest energy increases) .
Heavier particles can be produced.
T increases (rest energy decreases).
Extreme case: AC+D (a particle decays)
Elastic Collision (rest energy conserved)
Mass is conserved only in elastic collisions : almost always it means that the identity of the particles does not change.

15. Types of Collisions : the Elastic case
A new definition of Elasticity !
The identity of particles does not change between the initial and the final state
How many invariants can be used to characterize the collision ?
There’s 16 of them…
…..but four of them are trivial, since
The remaining 12 are really only 6 six because of symmetry
The remaining six are just two since we have the four conditions of conservation of Energy-Momentum
We can use 3 Mandelstam variables s,t,u keeping in mind

16. Reactions in the s or in the t channel (timelike or spacelike photons)b q
Now, choosing a frame where
This is a space-like photon that enters diffusion-like graphs a b q
The final state does not have photon quantum numbers.

17. In the case where the final state does have the photon quantum numbers :
Now, choosing a frame where a
This is a time-like photon that enters annihilation graphs : q b

18. Three body decay: the Dalitz plot
Invariant mass of subsystems
Only two of the subsystem invariant masses are independent :
Let us study the limits of the kinematics variable’s space (phase space)
In the CM system:

19. To find the lower limit we use the CM system of 2 ,3 (Jackson frame) :
So that, for every s:
A parallelogram !
One can actually devise a better limit by considering the correlation between the variables (not done here).
The Dalitz plot describes the transition between an initial state and a three-body final state.
It is built up by using two independent variables.
Kinematics dictates the boundaries of the plot.

20. The Dalitz Plot contours are given by kinematics
The density of dots in the Dalitz Plot is giving information on the dynamics of the final state particles :

22. What does really a Dalitz Plot represent ?
Which admits a formal analogy with :

23. Invariant Mass
Let us consider the decay of a particle in flight.
Let us suppose it decays in three particles (with n particles would be the same)
The states 1,2,3 are observed in the spectrometer
Momenta get measured
A mass hypotesis is made, based on the information from the spectrometer
Ingredients :

24. This quantity is built up :
which can also be written as :
But this is a Lorentz scalar. Then, I can compute it (for instance), in the rest frame of the decaying particle :
Bump hunting in invariant mass distributions :
???
The Upsilon peaks
???
B0 decay

25. The production of many particles
...
And, clearly
In a fixed target laboratory frame, with 1 (projectile) impinging on 2
Which can also be calculated in the CM using the final state

26. Threshold Energy in the Center of Mass :
….and in the Lab System:
We can also use the Kinetic Energy in the Lab Frame :

27. Particle propagation in Space
For a photon one has :
So that the phase :
According to the de Broglie hypotesis, for any particle:
A real particle is a superposition of plane waves :
with the appropriate dispersion law :

28. Wave-Optical description of Hadron Scattering
Propagation of a wave packet: superposition of particle waves of a number of different frequencies:
The wavepacket impinges on a scattering (diffusion) center
Neglecting an exp(-iωt) term
Neglecting the structure of the wave-packet
Range of Nuclear Forces

29. Beam of particles propagating along z
Depicted as a time-independent inde plane wave
We wll consider a spinless collision center in the origin : z
Expansion of the incident wave in spherical harmonic functions, in the kr>>1 approximation
entering and exiting
If we now introduce the effect of the diffusion center, we will have a phase shift and a reduction of the amplitude of the out wave

30. Asymptotic form of the global wave
The diffused wave: difference between incident and total wave :
Scattering amplitude
Elastic diffusion, with k staying the same (but of general validity in the CM system)

31. Physical meaning of the scattering amplitude
What we have written is equivalent to :
We can consider an incident flux equal to the number of incident particles per cross sectional area of the collision center.
This is given by the probability density times the velocity :
And we have a diffusion flux given by :
Diffusion cross section defined as the number of particles scattered per unit flux in an area subtended by a solid angle dΩ:

32. Integrating over the solid angle :
As a general result :
Legendre polynomials orthogonality
Integrating over the solid angle :
Total elastic cross section
No absorption and diffusion only due to phase shifts

33. In a more general case (η<1) we can divide the cross section between a reaction part and an elastic part :
The total cross section :
Non-zero absorption
Phase shift part (with or without absorption)
Computed with the probability loss
Effect on the outgoing wave

34. Optical Theorem :
The scattering amplitude is a complex quantity
The scattering amplitude is not well defined for θ = 0
How can we get information on F close to (or at) θ = 0 ?
Let us consider the amplitude for forward scattering :
Relation between the total cross section and the forward amplitude

35. Limit on the cross section due to conservation of probability
Unitarity
If one starts from the fully elastic case :
The maximum cross-section for the l wave takes place when
And in any case, for a given non-zero ηl the value of
Also gives a maximum for the total cross section
The maximum absorption cross section takes place when

36. Semiclassical interpretation: angular momentum and impact parameter
Role of the various angular momentum waves : a given angular momentum is related to a given impact parameter .
Suppose a particle is impinging on a target, with impact parameter b.
The angular momentum can be expressed in units of the Planck constant : p b
A bigger impact parameter is related to a different unit of angular momentum
Particles between l and l+1 are absorbed by an annular area

37. Scattering amplitude for the l wave
Im f i
Unitarity Circle
i/2 2δ
f(η=1)
Re f
η=1: f traces a circle with radius ½, centered in i/2, with phase shift between 0 and π/2
The maximum module is reached at π/2: resonance in the scattering amplitude
η<1 : f has a raiuds smaller than the Unitarity Circle
The vector cannot exceed the Unitarity Circle  a limit to the cross section

38. Resonance and Breit –Wigner formula
Goal: to express the behaviour of the cross section near to a resonance, i.e. when the scattering amplitudes goes through π/2 (spinless particles case)
At resonance δ = π/2
Power series expansion
Resonance energy
Assuming
Breit – Wigner
formula
We obtain :

39. Using the Breit-Wigner formula, one obtains - for the case when a given l is predominant :
This is a quantum dependence on energy, that corresponds to a temporale dependence of the state of the type :
Decay law of a particle
The Fourier transform of the decay law gives the E dependence :

40. In the case of an elastic resonance, the cross section is proportional to the square modulus of this amplitude :
This holds for elastic collisions of spinless particles. In general, if we form a spin J resonance by making spin Sa and Sb particles collide, one has :

41. In the case of an elastic scattering in l-wave :
A spin factor (for the proton)