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Quarks, Leptons and the Big Bang 2006. 12.12
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Page 1: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Quarks, Leptons and the Big Bang

2006. 12.12

Page 2: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

particle physics

Study of fundamental interactions of fundamental particles in Nature Fundamental interactions 1. strong interactions 2. weak interactions 3. electromagnetic interactions 4. gravitational interactions

Page 3: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Gravitational force: very weak at atomic scale Electromagnetic force: acts on all electrically charge particles Strong force: the force binding nucleons together Weak force: involved in beta decay acts on all particles

Page 4: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Basic tools

Special relativity and Quantum mechanics -> Relativistic Quantum Field Theory Schrodinger equation is valid only for nonrelativistic particle.

Page 5: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

What is a particle?

Pointlike object with no internal structures. It is characterized by mass and spin. (cf. Baseball ) spin: intrinsic angular momentum spin without spin can be nonzero without rotation in space

Page 6: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Spin statistics theorem

Particle can have either half-integer spin or integer spin in units of Particles with integer spin: Bosons Particles with half-integer spin: Fermions Fermions should obey Pauli’s exclusion principle. No two identical particles can be at the same quantum state, while bosons n

eed not.

h

Page 7: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Fundamental Particles

Fermions : building blocks of matter Paulis’s exclusion principle leptons: electron(e), muon( ), tau( ) neutrinos( ) quarks: u s t d b c Strong force acts on quarks and not on lepto

ns(only weak force and possibly electromagnetic force)

e

Page 8: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
Page 9: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Bosons : mediating the forces between fermions photons (light) no self interactions electromagnetic interactions gluons : quarks, nuclear force W, : weak interactions, decay gravitons : gravitational interactions

Z

Page 10: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

The emergence of the force

Coulomb force When electrons emit and absorb (virtual) photons, momentum transfer occurs. Coulomb force is generated by this process. Virtual photons are those not satisfying energy-time uncertainty relation All other forces arise in the same way

2r

Qq

htE

Page 11: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Relativistic Quantum Field Theory

Basic tools in theoretical particle physics Combination of special relativity and the quantum mechanics -> particle and antiparticle (same mass,

opposite charge, opposite quantum numbers) > pair creation and annihilation occur infinite degrees of freedom strong, weak, electromagnetic interactions well described-> standard model

m

pE

2

2

42222 cmcpE

E 22mc

Page 12: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Why are there more particles than antiparticles?

Page 13: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Some processes and the conservation laws of various kinds Pair annihilation/pair creation

Charge conservation

ee

44pp

Page 14: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
Page 15: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Angular momentum and lepton number conservation

decay process is a weak interaction Muon decay (separate lepton number conservation is needed)

ee

Page 16: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Baryon conservation law

Forbidden process

Assign baryon number B=+1 to every baryon,B=-1 for antibaryon

eep

Page 17: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Hadrons

Bound states of quarks loosely called particles Baryons (qqq): Fermions ex) proton, neutron Mesons ( ): Bosons ex) pions, Kaons

qq

Page 18: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Another conservation law

Strangeness (strange quark) kaon and sigma always produced in pairs

process which does not occur

The above Kaon has S=+1 and sigma particlehas S=-1 Strangeness is preserved in strong interactions

Kp

p

Page 19: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Eightfold way ( hadrons withu,d,s quarks) Classification of 8 spin ½ baryons and nine spin zero mesons via charge and strangeness

Page 20: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
Page 21: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
Page 22: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

u,d,s … quark flavors Why are quarks always bound? quark confinement fractional charges for quarks proton (uud), neutron (udd)

Using the eightfoldway, Gellman predicted the existence of a new particle in a decuplet

)( du

Page 23: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Similar classification scheme can be applied for hadrons involving c,b,t quarks

Page 24: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Beta decay

eeud

eepn

Page 25: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Weak force mediated by massive boson, short range force

W 80.6 GeV Z 91 GeV

m

h

E

ht

Page 26: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Strong force (color force)

Messenger particles are gluons massless, quarks can have various color charges (red, yellow, blue) so can gluons in contrast with the photons All hadron states are color neutral (quark confinement) Quantum chronodynamics (QCD) Linear potential V~kr (color tubes)

Page 27: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Strong forces are responsible for quarks binding into baryons and

mesons. They make the nuclear binding possible. Quantum Gravity so far not by the relativistic quantum

field theory based on the point particle but by the string theory

Page 28: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

General Gravity

Special relativity+gravitation matter and energy make spacetime curved

Page 29: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Universe is expanding

Einstein’s greatest blunder(?) :introducing the cosmological constant for the Einstein’s field equation (No static universe solution for Einstein’s field equation) Hubble’s observation (1929) All stars are moving away from us Universe is expanding (everywhere)

Page 30: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

v=Hr H Hubble’s constant=71.0 km/s Mpc 1 Mpc=3 X km If H is constant, then the estimated age of the universe is 1/H ( 13.7 X year)Based on the Big Bang scenario

1910

910

Page 31: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Cosmic Background Radiation

The universe is filled with the 2.7 K radiation (microwave region)In the early universe, the temperature is very hot and the atoms cannot be formed. (kT=2m ) After the atoms can be formed, lights can be travelled without scattering much about 379000 year old of the universe.)

2c

Page 32: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

If the cosmic background is too uniform this will be problematic for structure formation such as stars and galaxies. Such slight deviation from uniformity has been observed indeed. 1992 Cosmic Backgrouns Explorer(COBE) 2003 Wilikinson Microwave Anisotropy Probe (WMAP)

Page 33: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
Page 34: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
Page 35: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Brief history of the Universe

concepts of the space and time can have meaning inflation (factor of ) Quarks can combine to form protons and neutrons. Slight excess of matter 1min Low mass nuclei form Universe is opaque 379000 year Atoms form, light can travel

farther

sec10 43

sec10 34 3010sec10 4

Page 36: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Black Holes

Gravitational field is so strong, once the light is trapped it cannot escape. Heuristically

R; black hole radiusFor the mass of sun, R few km (extremely dense object)

02 mcr

GMm

2c

GMRr

Page 37: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

Black hole theormodynamics

Black hole has temperature and entropy

1. Black hole temperature Black hole is not black (Hawking radiation; black body radiation with )

M

1

MT

1

Page 38: Quarks, Leptons and the Big Bang 2006. 12.12. particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.

2. Black hole entropy is proportional to the surface area very large number for a black hole of solar mass Entropy ~ number of states (?) Classically black hole has few

parameters (mass, charge and angular momentum)

233 )10/( cmS

7610


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