Fundamentals of Particle Physics

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    A short journey to the infinitely small

    Fundamentals of

    Particle Physics

    Stefania Ricciardi

    RAL, March 2009

    Building blocks: particles and forces Current areas of research

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    Warning

    This journey may change your vision of the Universe.

    What you will hear may alter your perception of reality.

    We are entering a Quantum World..

    Stay awake and keep an open mind!

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    We and all things around us aremade of atoms

    Human Hair~ 50 m = 50 10-6 m

    = 0.000050 m

    Atom ~ 10-10 m= 0.0000000001 m

    Magritte

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    Atoms

    Atoms are all similarly made of:- protons and neutrons in the nucleus- electrons orbiting around

    electron

    proton

    neutron

    Protons,neutrons are

    made up ofquarks

    The electron was thefirst elementary

    particle to bediscovered(JJ Thomson 1897)

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    From the atom to the quark

    Atoms and sub-atomic particles are much smaller than visible light wave-lengthTherefore, we cannot really see them (all graphics are artists impressions)To learn about the sub-atomic structure we need particle accelerators

    How small are the smallest constituents of matter?

    ~ 10-10 m~ 10-14 m

    ~ 10-15 m

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    Wave-particle duality of Nature

    Central concept of quantum mechanics:all particles present wave-like properties

    De Broglie showed that moving particles have anequivalent wavelength l

    p

    1

    lSo high momentum gives usshort wavelengths so we canmake out small details

    Example: electron microscope

    Not only light has a dual nature

    Electron Microscope Image

    Gold atoms(0.2 nm apart)

    Copyright FEI

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    1911Rutherford found a nucleus in theatom by firing alpha particles at gold

    and observing them bounce back

    Rutherford: atoms are notelementary particles!

    Precursor of modern scattering experiments at accelerator

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    Quarks detected within protons

    Stanford (SLAC), California, late 1960sFire electrons at proton: big deflections seen!

    2 miles long accelerator

    End Station Aexperimental area

    Freeway 280

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    Protons and neutronsin the quark model

    proton (charge +1) neutron (charge 0)

    u d

    d

    u u

    d

    Quarks have fractional electric charge!u electric charge + 2/3d electric charge -1/3

    13

    1

    3

    2

    3

    2

    -

    pduu 0

    3

    1

    3

    1

    3

    2nddu

    -

    -

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    Neutrinos get under your skin!

    Within your body at any instant:roughly 30 million neutrinos fromthe Big Bang

    No worries!Neutrinos do not harm us.

    Our bodies are transparent to neutrinos

    14 neutrinosper second from Sun

    are zipping through you

    n

    Every cm2

    of Earth surface iscrossed every second by morethan 10 billion (1010) neutrinosproduced in the Sun

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    The particles of ordinary matter

    ne

    e-

    u

    d-1/3

    +2/30

    -1

    charge

    All stable matter around uscan be described using

    electrons, neutrinos, u and d quarks

    Quarks:u = up

    d = down

    Leptons:neutrino

    e = electron

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    3 Families (or Generations)

    nm

    m-

    c

    s

    nt

    t-

    t

    b

    Ordinary matter Cosmic rays Accelerators

    1st generation 2nd generation 3rd generation

    3 generations in everything similar but the mass

    -1/3-1/3

    +2/3 +2/3

    ne

    e-

    u

    d-1/3

    +2/3

    We believe these to be the fundamentalbuilding blocks of matter

    -1 -1 -1

    0 00

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    Quark masses

    0

    20

    40

    60

    80

    100

    120

    140

    160180

    Mass

    (GeV)

    Quarks

    Up Down Strange Charm Bottom Top

    0.003 0.006 0.095 1.2 4.5

    Top(discovered 1995)

    175 GeV

    E= mc2

    1 proton mass ~ 1GeV (10-27 Kg)

    The mass grows larger in each successive family

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    Anti-matter

    For every fundamental particle of matter there is an anti-particlewith same mass and properties but opposite charge

    ne

    e-

    u

    d

    -1/3

    +2/3

    ne

    e+

    u

    d

    +1/3

    -2/3

    +1

    0

    -1

    0

    positron

    Correspondent anti-particles exist for all three families Anti-matter can be produced using accelerators

    Matter Anti-Matter

    Bar on topto indicateanti-particle

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    Matter-antimatter pair creation

    Electron-positron pair created out ofphotons hitting the bubble-chamberliquid

    Example of conversion of photonenergy into matter and anti-matter

    Matter and anti-matter spiral in oppositedirections in the magnetic field due tothe opposite charge

    Energy and momentum is conserved

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    Quarks and colourAll quark flavours come in 3 versions, called colours

    u d+2/3 -1/3uu ddup down

    Quarks combine together to form colourless particles

    -Baryons(three quarks: red+ green + blue = white)

    -Mesons(quark-antiquark pair)such as red+anti-red u-ubar state

    proton

    uu

    pion

    p

    Strong forcesglue quarks

    together inbound states

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    Building more particles

    b b

    J/y

    c c

    Y

    b u

    B-

    u b

    B+

    b d

    B0

    d b

    B0

    B mesons (bq)

    Many more mesons and baryons

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    The Particle Physicists Bible:

    Particle Data Book

    https://pdg.lbl.gov

    "Young man, if I could rememberthe names of these particles,

    I would have been a botanist!

    E.Fermi to his student

    L. Lederman (both Nobellaureates)

    Most particles are not stable and can decay to lighter particles..

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    THE WEAK FORCEBeta Decay

    n p

    Antineutrino

    Electron

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    Neutron b-decay

    A (free) neutron decays after 15 min

    u d

    d

    n u ud

    p e-

    d u e-

    ne

    ne

    15 min

    At quark level:

    Long life time (15min is an eternity in particle physics!) weak

    without such weak interactions the Sun would shut down!

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    The 4 forces of Nature

    Weak Beta-decay pp fusion

    StrongQuark binding

    ElectromagneticTV, PCs Magnets

    e- e+ creation

    GravityResponsible of

    Keeping uswell-planted on earth

    Electriccharge

    mass

    weak

    charge

    strongcharge

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    Electromagnetic force

    e- e-

    Photon

    The repulsive force that two approaching electrons feel

    Photon is the particleassociated to the electromagnetic forcesmallest bundle of force

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    Weak force: W-,W+,Z0

    b-decaynpene

    Electric chargeconserved at each

    vertex

    W-

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    Strong force: gluons

    Gluons interact with quarks Gluons interact with other gluons

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    Quark confinementThere are no free quarks, quarks and antiquarks are confined

    in colourless doublet (mesons) or triplets (baryons) by the exchangeof gluons

    The new quarks boundto the old quarksand form new mesons

    until the gluon connectionsnaps, and other quark-antiquarkpairs are created out of theenergy released

    Gluon hold quarkstogether as they movefurther apart

    Z0

    Decay

    S.Ward

    Force Particles (summary)

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    Force Particles (summary)

    Particles interact and/or decay thanks to forcesForces are also responsible of binding particles together

    Strong: gluons

    Only quarks

    (because of their

    colour charge)

    Weak: W+, W-, Z0

    Leptons and quarks (onlyforce for neutrinos)

    Electromagnetic:gQuarks and charged leptons(no neutrinos)

    Gravity: graviton?Still to be discovered

    Negligible effects onparticles

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    O ti :

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    Open question:

    Why is the Universe made of

    matter and not equallyof anti-matter?

    We have seen that for every fundamental

    particle there is a corresponding antiparticle.

    Where are these anti-particles?

    Large amount of matter but no evidence oflarge amount of antimatter in the Universe..

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    Why has all the anti-matter gone?

    Anti-matter

    The development of the Universe containing

    matter and no antimatter requires thatmatter and antimatter behave differently

    This phenomenon is due to CP violation..

    matter Puff

    Good thing for us that there is no antimatter around!

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    CP Violation

    CP = Charge Conjugation (reverse charge) x Parity (reverse spatialcoordinates as in a mirror)

    CP

    beauty anti-beauty

    B0 B0

    Nobody

    is perfect

    CP-Violation: B0 and B0 do not behave exactly in the same way

    (their decay pattern as a function of time is different)

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    Discovery of CP violation in theB-meson system at Babar (SLAC, 2001)

    A visible difference is detected, but tiny, not enoughto explain the matter-antimatter asymmetry in the Universe

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    The CPV quest will go on at LHC

    CMS ALICE

    CERN

    LHCb experiment:700physicists

    50institutes15countries

    LHCb cavern

    LHCb

    ATLAS

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    Recent view of the LHCb cavern

    Its complete!

    RICH-1

    The experiment is fully installed and ready for first collisions

    RICH2 RICH1

    Muondetector

    Calorimeters OT Magnet

    VELO

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    Another open question:What is the Dark Matter?

    Astronomical observations have shown that observable mass

    represent less than 4% of the Universe!

    What is dark matter? We dont really know

    Perhaps partially composed of neutrinos, or possibly neutralinos particlespredicted by super-symmetric theories beyond the Standard Model?

    Dark MatterVisible Matter

    False-color imagesThe brightness ofclumpscorresponds to thedensity of mass.

    http://imagine.gsfc.nasa.gov/docs/dict_ad.htmlhttp://imagine.gsfc.nasa.gov/docs/dict_ad.html
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    Looking for Dark Matter at theBoulby Underground Laboratory

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    Neutrinos do matter to us:If there were no neutrinosthe sun would not shine!

    Almost no interactions (only weak)

    Can cross light-years of material without being affected Can travel from the most remote corners of the Universebringing information from the origin of space and time

    Puzzling neutrinos

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    R. Davis: measuring the solar neutrinoflux in a gold mine in South Dakota for

    30 years (1969-1999)

    and observing only 1/3 of the expected flux!! Why?

    R. DavisSolar neutrinospioneer

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    Neutrino oscillationsIf you let the neutrino travel enough,

    it can change its flavour!nm

    nt

    ent

    a huge neutrino detectorin the right place exists!

    A detector heredoes not see any nm

    Kamioka Observatory, ICRR (Institute for

    Cosmic Ray Research),The University of Tokyo

    a huge neutrino detectorexists!

    A detector heresees all nm

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    in the Kamioka mine in JapanSuperKamiokande is measuring neutrinos born in the atmospherabove the detector..

    flux from below only of flux from above!

    ..and below the detector (on the other side of the Earth!!)

    Total neutrino flux from below = total flux from above _

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    Discovery of neutrino oscillationSuper-Kamiokande (1998)

    Half of the nm are lost!

    Oscillated to undetected nt

    2002 Nobel PrizeKoshiba

    (superK Spokesman)shared with Davis

    Up-going Down-going

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    What have we learnt?

    A number of surprising things:

    A limited number of forces and matter particlesdescribe all the Universe we know about;

    A theory of the interactions of matter with forcescalled the Standard Model describes successfully thephenomena of the subatomic world;

    There are evidences that there is lot more that we donot know about and our research should find: such asthe missing anti-matter, dark matter, puzzling neutrinoproperties, but also the Standard Model key-vault..the Higgs!

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    Looking into the future

    The Higgs should be found at theLHCplease be patient for a few more

    hours.and you will learn about the

    Higgs, the LHC, and much more!

    NOT