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INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks elementary historical review of concepts, discover and achievements Recommended reading: D.H. Perkins, Introduction to High Energy Physics F.E. Close, The cosmic onion Luigi DiLella, Summer Student Program

INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

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Page 1: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

INTRODUCTIONTO PARTICLE PHYSICS

From atoms to quarks An elementary historical review of concepts, discoveries and achievements

Recommended reading:D.H. Perkins, Introduction to High Energy PhysicsF.E. Close, The cosmic onion

Luigi DiLella, Summer Student Program

Page 2: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

The Atoms of the 92 Elements . Hydrogen Mass MH x g 2. Helium 3. Lithium ............. ............. 92. Uranium Mass MH

increasing mass

Estimate of a typical atomic radius

Number of atoms cm:

Atomic volume: Packing fraction: f —

A

Nn A

NA x mol (Avogadro costant)

A: molar mass: density

3

3

4V R

3/1

4

3

n

fR

Example: Iron (A = g; = g cm)

R = ( — ) x cm

The “elementary particles” in the 19th century:

Page 3: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Study of “cathode rays”: electric current intubes at very low gas pressure (“glow discharge”)

Measurement of the electron mass: me MH/“Could anything at first sight seem more impractical than a body which is so small that its mass is an insignificant fraction of the mass of an atom of hydrogen?” (J.J. Thomson)

Thomson’s atomic model: Electrically charged sphere Radius ~ 10-8 cm Positive electric charge Electrons with negative electric charge embedded in the sphere

1894 – 1897: Discovery of the electron

J.J. Thomson

ATOMS ARE NOT ELEMENTARY

Page 4: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

radioactivesource

particles

target(very thin Gold foil)

fluorescent screen

Detector (human eye)

1896: Discovery of natural radioactivity(Henri Becquerel)

Henri Becquerel

: Rutherford’s scattering experiments Discovery of the atomic nucleus

Ernest Rutherford

particles: nuclei of Helium atoms spontaneously emitted by heavy radioactive isotopes

Typical – particle velocity c (c : speed of light)

Page 5: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Expectations for – atom scattering

particle

Atom: spherical distribution of electric charges

impactparameter b

– atom scattering at low energies is dominated by Coulomb interaction

– particles with impact parameter = b “see” only electric charge withinsphere of radius = b (Gauss theorem for forces proportional to r)

For Thomson’s atomic modelthe electric charge “seen” by the – particle is zero, independentof impact parameter

no significant scattering at large angles is expected

Page 6: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Nuclear radius cm x atomic radius

Mass of the nucleus mass of the atom(to a fraction of 1‰ )

Rutherford’s observation:significant scattering of – particles at large angles, consistentwith scattering expected for a sphere of radius few x cmand electric charge = Ze, with Z = (atomic number of gold)and e = |charge of the electron|

an atom consists of a positively charged nucleus surrounded by a cloud of electrons

Page 7: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Two questions: Why did Rutherford need – particles to discover the atomic nucleus? Why do we need huge accelerators to study particle physics today?

Answer to both questions from basic principles of Quantum Mechanics

Observation of very small objects using visible light

point-likelight source= m(blue light)

opaque screenwith small circular aperture

photographicplate

focusing lenses

Page 8: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Aperture diameter: D = mFocal length: cm y

(mm

)

x (mm)

Opaque disk, diam. min the centre

Presence of opaque disk is detectable

Observation of light diffraction, interpreted as evidence that light consists of waves since the end of the th centuryAngular aperture of the first circle(before focusing):

= D

Page 9: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

diameter = m diameter = m diameter = m

no opaque disk

Opaque disk of variable diameter

The presence of the opaque disk in the centreis detectable if its diameter is larger than thewavelength of the light

The RESOLVING POWER of the observationdepends on the wavelength Visible light: not enough resolution to see objectssmaller than . – . m

Page 10: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Opaque screen with two circular apertures

aperture diameter: mdistance between centres: m

x (mm)

y (m

m)

Image obtained by shutting one aperturealternatively for of the exposure time

Image obtained with both aperturesopen simultaneously

x (mm)

y (m

m)

Page 11: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Observation of a threshold effect as a function of the frequency of the lightimpinging onto the electrode at negative voltage (cathode):

Frequency < : electric current = zero, independent of luminous flux;

Frequency > : current > 0, proportional to luminous flux

glass tube under vacuum

Currentmeasurement

Photoelectric effect: evidence that light consists of particles

INTERPRETATION (A. Einstein):

Albert Einstein

E = h (Planck constant h = x J s)

Threshold energy E0 = h0: the energy needed to extract an electron from an atom (depends on the cathode material)

Light consists of particles (“photons”) Photon energy proportional to frequency:

Page 12: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Repeat the experiment with two circular aperturesusing a very weak light sourceLuminous flux = photon second (detectable using modern, commercially available photomultiplier tubes)Need very long exposure time

aperture diameter: mdistance between centres: m

Question: which aperture will photons choose?

Answer: diffraction pattern corresponds to both apertures simultaneously open, independent of luminous flux

y (m

m)

x (mm)

Photons have both particle and wave properties simultaneouslyIt is impossible to know which aperture the photon traversedThe photon can be described as a coherent superposition of two states

Page 13: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

: De Broglie’s principle

Louis de Broglie

Not only light, but also matter particles possess both the properties of waves and particles

Relation between wavelength and momentum:

hp

h: Planck constantp = m v : particle momentum

Hypothesis soon confirmed by the observation of diffractionpattern in the scattering of electrons from crystals, confirmingthe wave behaviour of electrons (Davisson and Germer, )

Wavelength of the – particles used by Rutherford in the discovery ofthe atomic nucleus:

cm 107.6m 107.6)s m105.1()kg106.6(

s J 10626.6

v1315

1-727

34

m

h

c~ resolving powerof Rutherford’s

experimentparticle

mass

Page 14: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Typical tools to study objects of very small dimensions

Optical microscopes Visible light ~ cm

Electron microscopes Low energy electrons ~ cm

Radioactive sources particles ~ cm

Accelerators High energy electrons, protons ~ cm

Resolvingpower

Page 15: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Units in particle physics

Energy1 electron-Volt (eV):the energy of a particle with electric charge = e,initially at rest, after acceleration by a differenceof electrostatic potential = Volt(e x C)

eV = x J

Multiples:

keV = eV ; MeV = eV

GeV = eV; TeV = eV

Energy of a proton in the LHC (in the year ): TeV = x J(the same energy of a body of mass = mg moving at speed = m s)

Page 16: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Energy and momentum for relativistic particles(velocity v comparable to c)

Speed of light in vacuum c = x m s

Total energy:2

202

)v(1 /c

cmmcE

...v2

1 20

20 mcmE

m: relativistic mass

m: rest mass

Expansion in powers of (vc):

energyassociated

with rest mass

“classical”kineticenergy

Momentum: 2

0

)/v(1

vv

c

mmp

cE

pc v

Page 17: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

E – pc = (mc) “relativistic invariant”(same value in all reference frames)

Special case: the photon (v = c in vacuum)

E = h = h p

E p = = c (in vacuum)

E – pc = photon rest mass m =

Momentum units: eVc (or MeVc, GeVc, ...)

Mass units: eVc(or MeVc,GeVc, ...)

Numerical example: electron with v = . c

Rest mass: me = MeV/c

089.7)/v(1

12

c(often called “Lorentz factor”)

Total energy: E = me cxMeV

Momentum: p = (v / c) x (E / c) = x = MeV/c

Page 18: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

First (wrong) ideas about nuclear structure (before 1932)Observations Mass values of light nuclei multiples of proton mass (to few %) (proton nucleus of the hydrogen atom) decay: spontaneous emission of electrons by some radioactive nuclei

Hypothesis: the atomic nucleus is a system of protons and electrons strongly bound togetherNucleus of the atom with atomic number Z and mass number A:a bound system of A protons and (A – Z) electronsTotal electric charge of the nucleus = [A – (A – Z)]e = Z e

Problem with this model: the “Nitrogen anomaly”Spin of the Nitrogen nucleus = Spin: intrinsic angular momentum of a particle (or system of particles)In Quantum Mechanics only integer or half-integer multiples of ħ (h )are possible: integer values for orbital angular momentum (e.g., for the motion of atomic electrons around the nucleus) both integer and half-integer values for spin

Page 19: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Electron, proton spin = ½ħ (measured)Nitrogen nucleus (A = , Z = ): protons + electrons = spin ½ particlesTOTAL SPIN MUST HAVE HALF-INTEGER VALUE Measured spin =

DISCOVERY OF THE NEUTRON (Chadwick, 1932)

Neutron: a particle with mass proton mass but with zero electric chargeSolution to the nuclear structure problem:Nucleus with atomic number Z and mass number A:a bound system of Z protons and (A – Z) neutrons James Chadwick

Nitrogen anomaly: no problem if neutron spin = ½ħ Nitrogen nucleus (A = , Z = ): protons, neutrons = spin ½ particles total spin has integer value

Neutron source in Chadwick’s experiments: a Po radioactive source ( MeV – particles ) mixed with Beryllium powder emission of electrically neutral radiation capable of traversing several centimetres of Pb:

He + Be C + neutron

- particle

Page 20: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Basic principles of particle detection

Passage of charged particles through matterInteraction with atomic electrons

ionization(neutral atom ion+ + free electron)

excitation of atomic energy levels(de-excitation photon emission)

Ionization + excitation of atomic energy levels energy loss

proportional to (electric charge) of incident particle

Mean energy loss rate – dE dx

for a given material, function only of incident particle velocity

typical value at minimum:

dE dx = – MeV (g cm)

NOTE: traversed thickness (dx) is givenin g cmto beindependent of materialdensity (for variable density materials,such as gases) – multiply dE dx by density (gcm) to obtain dE dx in MeVcm

Page 21: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Passage of neutral particles through matter: no interaction with atomic electrons detection possible only in case of collisions producing charged particles

Residual rangeResidual range of a charged particle with initial energy E

losing energy only by ionization and atomic excitation:

v)(/

1

0

2

0

MFdEdxdE

dxRR Mc

E

M: particle rest mass v: initial velocity

220 )/v(1/ cMcE

the measurement of R for a particle of known rest mass M is a measurement of the initial velocity

Neutron discovery:observation and measurement of nuclear recoils in an “expansion chamber”filled with Nitrogen at atmospheric pressure

incidentneutron

(not visible)

scattered neutron(not visible)

recoil nucleus(visible by ionization)

An old gaseous detector basedon an expanding vapour;ionization acts as seed for theformation of liquid drops. Tracks can be photographedas strings of droplets

Page 22: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Plate containing free hydrogen(paraffin wax)

Incident neutrondirection

proton tracks ejectedfrom paraffin wax

Recoiling Nitrogen nuclei

Assume that incident neutral radiation consistsof particles of mass m moving with velocities v < Vmax Determine max. velocity of recoil protons (Up) and Nitrogen nuclei (UN)from max. observed range

Up = Vmax

mm + mp

UN = Vmax

mm + mN

From non-relativistic energy-momentumconservationmp: proton mass; mN: Nitrogen nucleus mass

Up m + mN

UN m + mp

=From measured ratio Up UN and known values of mp, mN

determine neutron mass: m mn mp

Present mass values : mp = . MeV/c; mn = . MeV/c

Page 23: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Pauli’s exclusion principleIn Quantum Mechanics the electron orbits around the nucleus are “quantized”:only some specific orbits (characterized by integer quantum numbers) are possible.

Example: allowed orbit radii and energies for the Hydrogen atom

[m] 1053.04 210

2

220 n

me

nRn

[eV] 6.13

)4(2 22220

4

nn

meEn

m = memp/(me + mp)

n = , , ......

In atoms with Z > only two electrons are found in the innermost orbit – WHY?

ANSWER (Pauli, ): two electrons (spin = ½) can never be in the same physical state

Wolfgang Pauli

Pauli’s exclusion principle applies to all particles with half-integer spin (collectively named Fermions)

Lowestenergystate

Hydrogen (Z = ) Helium (Z = ) Lithium (Z = ) .....

Page 24: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

ANTIMATTER Discovered “theoretically” by P.A.M. Dirac ()

P.A.M. Dirac

Dirac’s equation: a relativistic wave equation for the electron

Two surprising results: Motion of an electron in an electromagnetic field: presence of a term describing (for slow electrons) the potential energy of a magnetic dipole moment in a magnetic field existence of an intrinsic electron magnetic dipole moment opposite to spin

electron spin

electronmagnetic dipolemoment e

[eV/T] 1079.52

5e

e m

e

For each solution of Dirac’s equation with electron energy E there is another solution with E What is the physical meaning of these “negative energy” solutions ?

Page 25: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Generic solutions of Dirac’s equation: complex wave functions ( r , t)In the presence of an electromagnetic field, for each negative-energy solutionthe complex conjugate wave function * is a positive-energy solution ofDirac’s equation for an electron with opposite electric charge (+e)

Dirac’s assumptions: nearly all electron negative-energy states are occupied and are not observable. electron transitions from a positive-energy to an occupied negative-energy state are forbidden by Pauli’s exclusion principle. electron transitions from a positive-energy state to an empty negative-energy state are allowed electron disappearance. To conserve electric charge, a positive electron (positron) must disappear e+e– annihilation. electron transitions from a negative-energy state to an empty positive-energy state are also allowed electron appearance. To conserve electric charge, a positron must appear creation of an e+e– pair. empty electron negative–energy states describe

positive energy states of the positron

Dirac’s perfect vacuum: a region where all positive-energy states are empty and all negative-energy states are full.

Positron magnetic dipole moment = e but oriented parallel to positron spin

Page 26: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Experimental confirmation of antimatter(C.D. Anderson, )

Carl D. Anderson

Detector: a Wilson cloud – chamber (visual detector based on a gasvolume containing vapour close to saturation) in a magnetic field,exposed to cosmic rays

Measure particle momentum and sign of electric charge frommagnetic curvature

Lorentz force Bef

v projection of the particle trajectory in a planeperpendicular to B is a circle

Circle radius for electric charge e:[T] 3

[GeV/c]10[m]

B

pR

p : momentum component perpendicular to magnetic field direction

NOTE: impossible to distinguish between positively and negatively charged particles going in opposite directions

–e

+e need an independent determination of the particle direction of motion

Page 27: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

First experimental observationof a positron

mm thick Pb plate

MeV positron

MeV positron

Production of anelectron-positron pair

by a high-energy photonin a Pb plate

direction of high-energy photon

Cosmic-ray “shower”containing several e+ e– pairs

Page 28: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

NeutrinosA puzzle in – decay: the continuous electron energy spectrum

First measurement by Chadwick ()

Radium E: Bi(a radioactive isotope produced in the decay chain of 238U)

If – decay is (A, Z) (A, Z+) + e–, then the emitted electron is mono-energetic:

electron total energy E = [M(A, Z) – M(A, Z+)]c

(neglecting the kinetic energy of the recoil nucleus ½p/M(A,Z+) << E)

Several solutions to the puzzle proposed before the ’s (all wrong), including violation of energy conservation in – decay

Page 29: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

December 1930: public letter sent by W. Pauli to a physics meeting in Tübingen

Zürich, Dec. 4, 1930Dear Radioactive Ladies and Gentlemen,...because of the “wrong” statistics of the N and 6Li nuclei and the continuous -spectrum, I have hit upon a desperate remedy to save the law of conservation of energy. Namely,the possibility that there could exist in the nuclei electrically neutral particles, that I wishto call neutrons, which have spin ½ and obey the exclusion principle ..... The mass of theneutrons should be of the same order of magnitude as the electron mass and in any eventnot larger than 0.01 proton masses. The continuous -spectrum would then becomeunderstandable by the assumption that in -decay a neutron is emitted in addition to theelectron such that the sum of the energies of the neutron and electron is constant........ For the moment, however, I do not dare to publish anything on this idea ......So, dear Radioactives, examine and judge it. Unfortunately I cannot appear in Tübingenpersonally, since I am indispensable here in Zürich because of a ball on the night of6/7 December. .... W. Pauli

NOTES Pauli’s neutron is a light particle not the neutron that will be discovered by Chadwick one year later As everybody else at that time, Pauli believed that if radioactive nuclei emit particles, these particles must exist in the nuclei before emission

Page 30: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Theory of -decay (E. Fermi, 1932-33)

Enrico Fermi

decay: n p + e + decay: p n + e + (e.g., 14O8 14N7 + e+ + )

Fermi’s theory: a point interaction among four spin ½ particles, using the mathematical formalism of creation and annihilation operators invented by Jordan particles emitted in – decay need not exist before emission – they are “created” at the instant of decay

Prediction of – decay rates and electron energy spectra as a function of only one parameter: Fermi coupling constant GF (determined from experiments)

Energy spectrum dependence on neutrino mass (from Fermi’s original article, published in German on Zeitschrift für Physik, following rejection of the English version by Nature)Measurable distortions for near the end-point(E: max. allowed electron energy)

: the particle proposed by Pauli (named “neutrino” by Fermi): its antiparticle (antineutrino)

Page 31: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Neutrino detection

Target:surface S, thickness dxcontaining n protons cm–

Incident :Flux [ cm–s–](uniform over surface S)

dx

Prediction of Fermi’s theory: + p e+ + n

– p interaction probability in thickness dx of hydrogen-rich material (e.g., HO)

p interaction rate = S n dx interactions per second

: – proton cross-section (effective proton area, as seen by the incident )

p interaction probability = n dx = dx

Interaction mean free path: = n Interaction probability for finite target thickness T = – exp(–T )

( p) – cm for MeV 150 light-years of water !

Interaction probability T very small (~– per metre HO) need very intense sources for antineutrino detection

Page 32: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Nuclear reactors: very intense antineutrino sources

Average fission: n + U (A, Z) + (A, – Z) + free neutrons + MeV

nuclei withlarge neutron excess

a chain of decays with very short lifetimes:

(A, Z) (A, Z + ) (A, Z + ) ....e– e– e–

(until a stable or long lifetime nucleus is reached)

On average, 6 per fission

/s 1087.1106.1MeV 200

6 rate production 11

13

t

t PP

Pt: reactor thermal power [W] conversion factorMeV J

For a typical reactor: Pt = x W x s (isotropic)Continuous energy spectrum – average energy ~ MeV

Page 33: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

First neutrino detection(Reines, Cowan 1953)

+ p e+ + n

detect MeV -rays from e+e– (t = )

E = MeV

neutron “thermalization” followed by capture in Cd nuclei emission of delayed -rays (average delay ~ s)

HO +

CdCl

I, II, III:Liquid scintillator

m Event rate at the Savannah River nuclear power plant: events hour(after subracting event rate measured with reactor OFF )in agreement with expectations

Page 34: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

COSMIC RAYS Discovered by V.F. Hess in the 1910’s by the observation of the increase of radioactivity with altitude during a balloon flight Until the late 1940’s, the only existing source of high-energy particles

Composition of cosmic rays at sea level – two main components Electromagnetic “showers”, consisting of many e and -rays, mainly originating from:

+ nucleus e+e– + nucleus (pair production); e + nucleus e + + nucleus (“bremsstrahlung”)

The typical mean free path for these processes (“radiation length”, x) depends on Z. For Pb (Z = 82) x = 0.56 cm Thickness of the atmosphere 27 x

Cloud chamber image of anelectromagnetic shower.Pb plates, each . cm thick

Muons ( ) capable of traversing as much as 1 m of Pb without interacting; tracks observed in cloud chambers in the 1930’s. Determination of the mass by simultaneous measurement

of momentum p = mv( – v/c)-½ (track curvature in magnetic field) and velocity v (ionization): m = MeV/c me

Page 35: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Muon decay ± e± + +

Decay electron momentum distribution

Cosmic ray muon stoppingin a cloud chamber anddecaying to an electron

decay electron track Muon lifetime at rest: = . x - s . s

Muon decay mean free path in flight:

c

cm

p

m

p

c-decay

2/v1

v

muons can reach the Earth surface after a path 10 km because the decay mean free path is stretched by the relativistic time expansion

p : muon momentum

c . km

Muon spin = ½

Page 36: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Particle interactions (as known until the mid ’s)

Gravitational interaction (all particles) Totally negligible in particle physics Example: static force between electron and proton at distance D

In order of increasing strength:

2D

mmGf pe

NG Gravitational:2

2

04

1

D

efE Electrostatic:

Ratio fG fE . x –

Weak interaction (all particles except photons) Responsible for decay and for slow nuclear fusion reactions in the star core Example: in the core of the Sun (T = . x ºK) p He + e+ + Solar neutrino emission rate ~ . x neutrinossFlux of solar neutrinos on Earth~ . x neutrinoscms –

Very small interaction radius Rint (max. distance at which two particles

interact) (Rint = in the original formulation of Fermi’s theory) Electromagnetic interaction (all charged particles) Responsible for chemical reactions, light emission from atoms, etc. Infinite interaction radius (example: the interaction between electrons in transmitting and receiving antennas)

Page 37: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Strong interaction ( neutron, proton, .... NOT THE ELECTRON ! ) Responsible for keeping protons and neutrons together in the atomic nucleus Independent of electric charge Interaction radius Rint – cm

In Relativistic Quantum Mechanics static fields of forces DO NOT EXIST ; the interaction between two particles is “transmitted” by intermediate particles acting as “interaction carriers” Example: electron – proton scattering (an effect of the electromagnetic interaction) is described as a two-step process : ) incident electron scattered electron + photon ) photon + incident proton scattered proton

The photon ( ) is the carrier of the electromagnetic interaction

incident electron ( Ee , p )

scattered electron ( Ee , p’ )

incident proton ( Ep , – p )

scattered proton ( Ep , – p’ )

In the electron – protoncentre-of-mass system

“Mass” of the intermediate photon: Q E – pc = – pc ( – cos )

The photon is in a VIRTUAL state because for real photons E – p

c = (the mass of real photons is ZERO ) – virtual photons can only travel over very short distances thanks to the “Uncertainty Principle”

Energy – momentum conservation:

E =

p = p – p ’ ( p = p ’)

Page 38: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

The Uncertainty Principle

Werner Heisenberg

CLASSICAL MECHANICSPosition and momentum of a particle can be measuredindependently and simultaneously with arbitrary precision

QUANTUM MECHANICSMeasurement perturbs the particle state position and momentummeasurements are correlated:

(also for y and z components) xpx

Numerical example:

MeV/c 100 xp cm 1097.1 13x

Page 39: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

1937: Theory of nuclear forces (H. Yukawa) Existence of a new light particle (“meson”)as the carrier of nuclear forcesRelation between interaction radius and meson mass m:

mcR

int

mc2 MeV for Rint cm

Yukawa’s meson initially identified with the muon – in this case – stoppingin matter should be immediately absorbed by nuclei nuclear breakup(not true for stopping + because of Coulomb repulsion - + never come close enough to nuclei, while – form “muonic” atoms)

Experiment of Conversi, Pancini, Piccioni (Rome, 1945): study of – stopping in matter using – magnetic selection in the cosmic rays

In light material (Z ) the – decays mainly to electron (just as +)In heavier material, the – disappears partly by decaying to electron,and partly by nuclear capture (process later understood as – + p n + ).However, the rate of nuclear captures is consistent with the weak interaction.

the muon is not Yukawa’s meson

Hideki Yukawa

Page 40: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

: Discovery of the - meson (the “real” Yukawa particle)

Observation of the + + e+ decay chain in nuclear emulsionexposed to cosmic rays at high altitudes

Four events showing the decay of a +

coming to rest in nuclear emulsion Nuclear emulsion: a detector sensitive toionization with ~ m space resolution(AgBr microcrystals suspended in gelatin)

In all events the muon has a fixed kinetic energy (. MeV, corresponding to a range of ~ m in nuclear emulsion) two-body decay

m = . MeVcspin = Dominant decay mode: + + + and– – + Mean life at rest:=xs =ns – at rest undergoes nuclear capture, as expected for the Yukawa particle

A neutral – meson (°) also exists:

m (°) = . MeV cDecay: ° + , mean life = . x s

– mesons are the most copiously produced particles in proton – proton and proton – nucleus collisions at high energies

Page 41: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

CONSERVED QUANTUM NUMBERS

Why is the free proton stable?Possible proton decay modes (allowed by all known conservation laws: energy – momentum,electric charge, angular momentum): p ° + e+

p ° + +

p + + . . . . . No proton decay ever observed – the proton is STABLE

Limit on the proton mean life: p > . x years

Invent a new quantum number : “Baryonic Number” B B = 1 for proton, neutron B = -1 for antiproton, antineutron B = 0 for e± , ± , neutrinos, mesons, photonsRequire conservation of baryonic number in all particle processes:

i f

fi BB

( i : initial state particle ; f : final state particle)

Page 42: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Strangeness Late 1940’s: discovery of a variety of heavier mesons (K – mesons) and baryons (“hyperons”) – studied in detail in the ’s at the new high-energy proton synchrotrons (the 3 GeV “cosmotron” at the Brookhaven National Lab and the 6 GeV Bevatron at Berkeley)

Mass values

Mesons (spin = 0): m(K±) = . MeV/c ; m(K°) = . MeV/c

Hyperons (spin = ½): m() = . MeV/c ; m(±) = . MeV/c

m(°) = . MeV/c;m(– ) = . MeV/c

Properties Abundant production in proton – nucleus , – nucleus collisions Production cross-section typical of strong interactions ( > - cm) Production in pairs (example: – + p K° + ; K– + p – + K+ ) Decaying to lighter particles with mean life values – – – s (as expected for a weak decay)Examples of decay modes

K± ± ;K± ± +– ;K± ± ; K° +– ; K° ; . . . p – ; n ° ; + p ° ; + n + ; + n – ; . . .

– – ; ° °

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Invention of a new, additive quantum number “Strangeness” (S)(Gell-Mann, Nakano, Nishijima, 1953) conserved in strong interaction processes:

i ffi SS

not conserved in weak decays: 1SS f

fi

S = +: K+, K° ; S = –: , ±, ° ; S = – : °, – ; S = 0 : all other particles(and opposite strangeness –S for the corresponding antiparticles)

Example of a K – stoppingin liquid hydrogen: K – + p + °(strangeness conserving)

followed by the decay

p + –

(strangeness violation)p

K–

° e+ e– (a rare decay)

is produced in A and decays in B

Page 44: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Antiproton discovery (1955)Threshold energy for antiproton ( p ) production in proton – proton collisionsBaryon number conservation simultaneous production of p and p (or p and n)

p p p p p p Example: Threshold energy ~ 6 GeV

“Bevatron”: GeV proton synchrotron in Berkeley build a beam line for . GeV/c momentum

select negatively charged particles (mostly – ) reject fast – by Čerenkov effect: light emission in transparent medium if particle velocity v > c n (n: refraction index) – antiprotons have v < c n no Čerenkov light measure time of flight between counters S and S ( m path): ns for – , ns for antiprotons

For fixed momentum,time of flight gives particle velocity, henceparticle mass

Page 45: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Example of antiproton annihilation at rest in a liquid hydrogen bubble chamber

Page 46: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Another neutrinoA puzzle of the late ’s: the absence of e decays

Experimental limit: in + e+ decaysA possible solution: existence of a new, conserved “muonic” quantum number distinguishing muons from electronsTo allow + e+ decays, must have “muonic” quantum number

but not in + decay the is not the antiparticle of

two distinct neutrinos (e , ) in the decay + e+ e Consequence for – meson decays: + + ;

- – to conserve the “muonic” quantum numberHigh energy proton accelerators: intense sources of – mesons ,

Experimental method ,

protonbeam

target

decay region

Shieldingto stop all other particles,including from decay

Neutrino detector

If e , interactions produce – and not e– (example: + n – + p)

Page 47: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

: discovery at the Brookhaven AGS(a 30 GeV proton synchrotron running at GeV for the neutrino experiment)

. m iron shielding(enough to stop GeV muons)

Neutrino detector

Spark chambereach with Al plates(x x . cm)mass Ton

Muon – electron separationMuon: long trackElectron: short, multi-spark event from electromagnetic shower

Neutrino energy spectrumknown from productionand , K decay kinematics

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64 “events” from a 300 hour run: single track events, consistent with track events consistent with electron shower (from small, calculable e contamination in beam)

Clear demonstration that e

Three typical single-track eventsin the BNL neutrino experiment

Page 49: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

THE “STATIC” QUARK MODELLate ’s – early ’s: discovery of many strongly interacting particlesat the high energy proton accelerators (Berkeley Bevatron, BNL AGS, CERN PS),

all with very short mean life times (– – – s, typical of strong decays) catalog of strongly interacting particles (collectively named “hadrons”)

ARE HADRONS ELEMENTARY PARTICLES?

1964 (Gell-Mann, Zweig): Hadron classification into “families”;observation that all hadrons could be built from three spin ½ “building blocks” (named “quarks” by Gell-Mann):

u d sElectric charge( units e)Baryonic number

Strangeness

and three antiquarks ( u , d , s ) with opposite electric chargeand opposite baryonic number and strangeness

Page 50: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Mesons: quark – antiquark pairs

2/)( ; ; 0 uudddudu Examples of non-strange mesons:

Examples of strange mesons:

dsKusKdsKusK 00 ; ; ;

Baryons: three quarks bound together Antibaryons: three antiquarks bound together Examples of non-strange baryons:

udduud neutron ; proton Examples of strangeness – baryons:

; ; 0 sddsudsuu

Examples of strangeness – baryons:

; 0 ssdssu

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Prediction and discovery of the – particle A success of the static quark model The “decuplet” of spin baryons

Strangeness Mass (MeVc )

N*++ N*+ N*° N*– uuu uud udd ddd

– *+ *° *– suu sud sdd

– *° *– ssu ssd

– – (predicted) sss–: the bound state of three s – quarks with the lowest mass

with total angular momentum =

Pauli’s exclusion principle requires that the three quarkscannot be identical

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The first – event (observed in the m liquid hydrogen bubble chamber at BNL

using a GeV/c K– beam from the GeV AGS)

Chain of events in the picture: K– + p – + K+ + K° (strangeness conserving)

– ° + – (S = weak decay)

° ° + (S = weak decay)

– + p (S = weak decay)

° + (electromagnetic decay) with both – rays converting to an e+e – in liquid hydrogen(very lucky event, because the mean free path for e+e – in liquid hydrogen is ~ m)

– mass measured from this event = 1686 ± 12 MeVc2

Page 53: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

“DYNAMIC” EVIDENCE FOR QUARKSElectron – proton scattering using a GeV electron beam from theStanford two – mile Linear Accelerator ( – ).The modern version of Rutherford’s original experiment:

resolving power wavelength associated with GeV electron cm

Three magnetic spectrometers to detect the scattered electron: GeV spectrometer (to study elastic scattering e– + p e– + p) GeV spectrometer (to study inelastic scattering e– + p e– + hadrons) . GeV spectrometer (to study extremely inelastic collisions)

Page 54: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

The Stanford two-mile electron linear accelerator (SLAC)

Page 55: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Electron elastic scattering from a point-like charge eat high energies:differential cross-section in the collision centre-of-mass (Mott’s formula)

ME

c

d

d

)2/(sin

)2/(cos

8

)(4

2

2

22 137

12

c

e

Scattering from an extended charge distribution: multiply M by a “form factor”:

MFd

d

)Q( 2Q = ħ / D : mass of the exchanged virtual photon D: linear size of target region contributing to scattering Increasing Qdecreasing target electric charge

Q (GeV)

F(Q)

F (Q) = for a point-like particle the proton is not a point-like particle

Page 56: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

F(Q)

Q (GeV)

Inelastic electron – proton collisionsincident electron ( Ee , p )

scattered electron ( Ee’ , p’ )

incident proton ( Ep , – p )

Hadrons(mesons, baryons)

2

22

2 cpEWi

ii

i

Total hadronic energy :

For deeply inelastic collisions,the cross-section depends only weaklyon Qsuggesting a collisionwith a POINT-LIKE object

Page 57: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Interpretation of deep inelastic e - p collisionsDeep inelastic electron – proton collisions are elastic collisions with point-like,electrically charged, spin ½ constituents of the proton carrying a fraction x of theincident proton momentum

Each constituent type is described by its electric charge ei (units of e )

and by its x distribution (dNi dx) (“structure function”)If these constituents are the u and d quarks, then deep inelastic e – p collisionsprovide information on a particular combination of structure functions:

dx

dNe

dx

dNe

dx

dN dd

uu

22

pe

Comparison with – p and – p deep inelastic collisions at high energies

under the assumption that these collisions are also elastic scatterings on quarks + p – + hadrons : + d – + u (depends on dNd dx )

+ p + + hadrons : + u + + d (depends on dNu dx ) (Neutrino interactions do not depend on electric charge)

All experimental results on deep inelastic e – p , – p, – p

collisions are consistent with eu = and ed

= the proton constituents are the quarks

Page 58: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

PHYSICS WITH e+e– COLLIDERSTwo beams circulating in opposite directions in the same magnetic ringand colliding head-on

e+ e–

E , p E , – p

A two-step process: e+ + e– virtual photon f + f f : any electrically charged elementary spin ½ particle (, quark)

(excluding e+e– elastic scattering)Virtual photon energy – momentum : E = E , p = Q = E – p

c = E

Cross - section for e+e– f f : )3(3

2 22

222

feQ

c = e(ħc) ef : electric charge of particle f (units e ) = vc of outgoing particle f (formula precisely verified for e+e– +– )

Assumption: e+e– quark ( q ) + antiquark ( q ) hadrons

at energies E mqc(for q = u , d , s) :

3

2

9

1

9

1

9

4

)ee(

hadrons)e(e 222

sdu-eeeR

Page 59: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Experimental results from the Stanford e+e– collider SPEAR ( –):

R

Q = E (GeV) For Q . GeV R . If each quark exists in three different states, R is consistent with x ( ). This would solve the – problem.

Between and .GeV, the peaks and structures are due to the production of quark-antiquark bound states and resonances of a fourth quark (“charm”, c) of electric charge +

Above . GeV R .. Expect R (from u, d, s) + x () = . from the addition of the c quark alone. So the data suggest pair production of an additional elementary spin ½ particle with electric charge = (later identified as the – lepton (no strong interaction) with mass MeV/c).

Page 60: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Q = E (GeV)

ee

e

Final state : an electron – muon pair + missing energy

Evidence for production of pairs of heavy leptons ±

Page 61: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

THE MODERN THEORY OF STRONG INTERACTIONS: the interactions between quarks based on “Colour Symmetry”Quantum ChromoDynamics (QCD) formulated in the early ’s Each quark exists in three states of a new quantum number named “colour”

Particles with colour interact strongly through the exchange of spin 1 particles named “gluons”, in analogy with electrically charged particles interacting electromagnetically through the exchange of spin 1 photons

A MAJOR DIFFERENCE WITH THE ELECTROMAGNETIC INTERACTIONElectric charge: positive or negativePhotons have no electric charge and there is no direct photon-photon interaction

Colour: three varietiesMathematical consequence of colour symmetry: the existence of eight gluons witheight variety of colours, with direct gluon – gluon interaction

The observed hadrons (baryons, mesons ) are colourless combinations of coloured quarks and gluons

The strong interactions between baryons, mesons is an “apparent” interaction between colourless objects, in analogy with the apparent electromagnetic interaction between electrically neutral atoms

Page 62: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Free quarks, gluons have never been observed experimentally;only indirect evidence from the study of hadrons – WHY?

CONFINEMENT: coloured particles are confined withincolourless hadrons because of the behaviour of the colour forcesat large distances

The attractive force between coloured particles increases withdistance increase of potential energy production of quark – antiquark pairs which neutralize colour formationof colourless hadrons (hadronization)

CONFINEMENT, HADRONIZATION: properties deducedfrom observation. So far, the properties of colour forces atlarge distance have no precise mathematical formulation in QCD.

At high energies (e.g., in e+e– q + q ) expect the hadrons tobe produced along the initial direction of the q – q pair production of hadronic “jets”

Page 63: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

e+ + e– hadronsA typical event atQ = E = GeV:reconstructedcharged particle tracks

A typical proton-antiproton collisionat the CERN p p collider ( GeV )producing high-energy hadrons atlarge angles to the beam axis(UA experiment, )

Energy depositionsin calorimeters

Page 64: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

1962-66: Formulation of a Unified Electroweak Theory(Glashow, Salam, Weinberg)

intermediate spin interaction carriers (“bosons”): the photon () responsible for all electromagnetic processes

Examples: n p e– : n p + W– followed by W– e– + e+ e :

+ + W+ followed by W+ e+ e

Z responsible for weak processes with no electric charge transfer (Neutral Current processes) PROCESSES NEVER OBSERVED BEFORE Require neutrino beams to search for these processes, to remove the much larger electromagnetic effects expected with charged particle beams

three weak, heavy bosons W+ W– Z W± responsible for processes with electric charge transfer = ±(Charged Current processes)

Page 65: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

First observation of Neutral Current processes in the heavy liquidbubble chamber Gargamelle at the CERN PS ()

Example of + e– + e–

(elastic scattering)Recoil electron energy = MeV

( beam from – decay

in flight)

Example of + p (n) + hadrons

(inelastic interaction)( beam from + decay

in flight)

Page 66: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

Measured rates of Neutral Current events estimate of the W and Z masses(not very accurately, because of the small number of events):

MW 70 – 90 GeV/c ; MZ 80 – 100 GeV/c too high to be produced at any accelerator in operation in the ’s1975: Proposal to transform the new 450 GeV CERN protonsynchrotron (SPS) into a proton – antiproton collider (C. Rubbia)

p p

Beam energy = GeV total energy in the centre-of-mass = GeV

Beam energy necessary to achieve the same collision energy on a proton at rest :

22222 GeV) 630()( cpcmE p E = TeV

Production of W and Z by quark – antiquark annihilation:

Wdu Wdu

Zuu Zdd

Page 67: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

UA1 and UA2 experiments (1981 – 1990)

Search for W± e± + (UA1, UA2) ; W± ± + (UA1)

Z e+e– (UA1, UA2) ; Z + – (UA1)

UA: magnetic volume with trackers, surrounded by “hermetic” calorimeter

and muon detectors

UA: non-magnetic, calorimetric detector

with inner tracker

Page 68: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

One of the first W e + events in UA1

48 GeV electronidentified by

surrounding calorimeters

Page 69: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

UA final results

Events containing two high-energy electrons:Distributions of the “invariant mass” Mee

2221

221

22 )()()( cppEEcM ee

(for Z e+e– Mee = MZ)

Events containing a single electron with largetransverse momentum (momentum componentperpendicular to the beam axis) and large missingtransverse momentum (apparent violation ofmomentum conservation due to the escaping neutrinofrom W e decay) mT (“transverse mass”): invariant mass of the electron – neutrinopair calculated from the transverse components onlyMW is determined from a fit to the mT distribution: MW = . ± . GeVc

Page 70: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

GeV 200 and 0.3between )ee(

hadrons)e(e

-

R

R

Q = E (GeV)

e+e– colliders at higher energies

e+e– b b (the th quark: e = )

e+e– Z q q

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The two orthogonal views of an event Z q q hadrons at LEP(ALEPH detector)

Page 72: INTRODUCTION TO PARTICLE PHYSICS From atoms to quarks An elementary historical review of concepts, discoveries and achievements Recommended reading: D.H

CONCLUSIONSThe elementary particles today:

3 x 6 = 18 quarks + 6 leptons = 24 fermions (constituents of matter)+ 24 antiparticles 48 elementary particlesconsistent with point-like dimensions within theresolving power of present instrumentation

( ~ 10-16 cm)

12 force carriers (, W±, Z, 8 gluons)

+ the Higgs spin particle (NOT YET DISCOVERED) responsible for generating the masses of all particles