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Overview of CERN & the physics raison d’être The search for elementary particles explanation of the universe Historical perspective Particle physics & forces Slide show – accelerator, experiments, technology http://hepwww.rl.ac.uk/ppdstaff/Tynd CERNs.ppt
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Overview of CERN & the physics raison d’être The search for elementary particles explanation of the universe Historical perspective Particle physics.

Dec 28, 2015

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Page 1: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Overview of CERN & the physics raison d’être

The search for elementary particles

explanation of the universe

Historical perspective

Particle physics & forces

Slide show – accelerator, experiments, technology

http://hepwww.rl.ac.uk/ppdstaff/Tyndel/NZ2006/CERNs.ppt

Page 2: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Sign in Geneva airport

Page 3: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• CERN is:– The European Organization for Nuclear Research

– The world's largest particle physics centre (now)

– It is on the Franco-Swiss border near Geneva.

Page 4: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.
Page 5: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Goal of CERN is particle physics research (which links to the physics of the universe)

Page 6: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• CERN is a laboratory with 2500 staff, 6500 users & 500 associates/fellows who study the building blocks of matter and the forces that hold them together.

• CERN exists primarily to provide them with the necessary tools.

• These are accelerators, which accelerate particles to almost the speed of light and detectors to make the particles visible.

• The budget is 1.3Bn SFr per year– [Figures from 2005]

Page 7: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

An accelerator:

1) produces particles

2) accelerates them using an electric field

3) constrains them using a magnetic field

Page 8: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Particle detectors – devices which can “see” particles and measure their trajectories and energy

Page 9: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• Why accelerate particles?

• Accelerate means giving particles energy

1. This energy allows us to look « inside » matter for substructure (Heisenberg:

p.x ~ h)

2. Also the energy can create new particles (Einstein E = mc2 )

Page 10: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Founded in 1954, the laboratory was one of Europe's first joint ventures and includes now 20 Member States.

Page 11: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.
Page 12: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Historical diversion• William Thomson, Lord Kelvin (1824 – 1907)

Belfast Glasgow , Cambridge , Glasgow

• Thermodynamics, Electricity, Atomic theory, Age of the earth…..

• "Scientific wealth tends to accumulate according to the law of compound interest. Every addition to knowledge of the properties of matter supplies [the physical scientist] with new instrumental means for discovering and interpreting phenomena of nature, which in their turn afford foundations of fresh generalisations, bringing gains of permanent value into the great storehouse of [natural] philosophy." ["Presidential address to British Association", 1871]

• "There is nothing new to be discovered in physics now, All that remains is more and more precise measurement.”

Page 13: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

… but Kelvin was not the first or the last to be wrong about knowing nearly everything

Page 14: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Résumé particle physics BC (before CERN)

• Antiquity : Four elements. Unsuccessful attempt at an atomistic theory during the 5th century BC (Democritus).

• 18th century : Lavoisier and Dalton verify experimentally the validity of the atomic structure.

• 1868 : Mendeleev proposes his chart of elements, containing the 63 atoms known at the time. The “empty cases” he left were soon filed. By 1896, 77 atoms have been discovered, and are considered elementary.

• 1897 : Discovery of the first subatomic particle by J.J Thompson : the electron.

• 1911 : Rutherford discovers the nucleus. Transmutation reactions showed that the hydrogen nucleus played a specific role (4

2He + 147N --> 18

9F --> 17

8O + 11p) . Rutherford named it proton (protos =

first)

Page 15: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Historical diversion

• Baron Ernest Rutherford (1871 – 1937)

New Zealand Cambridge Canada Cambridge

• Chemistry, Structure & splitting of atom

• "All science is either physics or stamp collecting."

Page 16: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• 1932 : Chadwick discovers the neutron, which is not stable when isolated, and decays as follows : n p + e- (+ ¯νe) . The proton, electron and neutron account for all the atoms of all the elements in the Universe.

This was the “simplest” elementary particle set ever described. A small number of particles, a small number of interactions or forces.

• LEPTON (leptos = light) : e- and BARYONS (baryos =

heavy) : p , n

• Gravitational, Electromagnetic & nuclear forces

Page 17: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• And finally we arrive at 1949…– The 2nd world war is over– Physicists had a visible role in ending the war– Europe is considered a “basket case”

• 1949: Louis de Broglie proposes the creation of a European science laboratory during the European Cultural Conference at Lausanne.

• 1950: Rabi puts forward a resolution, which is unanimously adopted, authorising the Director General of UNESCO, "to assist and encourage the formation and organization of regional centres and laboratories in order to increase and make more fruitful the international collaboration of scientists ...".

• 1952: After two UNESCO Conferences, a site near Geneva is selected for the planned laboratory.

• 1954: CERN formally created on 29th September.

CERN beginnings

Page 18: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• 1957: The 600 MeV Synchro-Cyclotron begins operation. One of the first experimental achievements is the long-awaited observation of the decay of a pion directly into an electron and a neutrino.

• 1959: The worlds highest energy accelerator (28GeV PS) and the neutrino beam completed.

• 1963: First bubble chamber pictures of neutrino interactions

• 1968: Electronic detectors (wire chambers) invented A later bubble chamber - BEBC

Page 19: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• 1973: First results from “ISR colliding beams” show that the proton “size” increases with energy.

• 1973: Neutrino neutral currents discovered. Forces unified.

• 1976: A new super accelerator built (500GeV SPS)

• 1981: Stochastic cooling invented allowing conversion of SPS into a collider .

• 1983: Discovery of the “carriers of weak force” (W, Z).

• 1989: LEP, a machine built to investigate the W and Z starts and proves that there are 3 families of quarks

Page 20: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• 1989 : WWW ‘hypertext’ (the world wide web) invented @ CERN to ease communication between computers

• 1989-2000: Results from LEP establish the “Standard model” as the theory of particle physics.

• 1996: Antimatter created at CERN

• 1994: Start of construction of worlds highest energy machine (14,000GeV LHC) – expected in 2007

Page 21: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• So many new particles were being discovered so that in 1955, Willis Lamb started his Nobel Prize speech by saying that “maybe physicists discovering a new particle ought to be fined $10,000”

• Gell Mann saw the pattern in 1961. Just as Mendeleev had done for atoms, a century before, he deduced that there was a substructure with 2 types of quarks held together by gluons.

• And the rest of the quarks were found:– 1974 charm quark– 1977 bottom quark– 1975 tau lepton– 1995 top quark

– 1977 gluon jets

• And in 1998- The neutrino was discoveredto have small mass

…and to complete the global picture

Page 22: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.
Page 23: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.
Page 24: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

In 50 years, there has been a revolution in understanding…

Page 25: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.
Page 26: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• Are we at the end of the road?– [Remember Kelvin]

• Not likely– Hope to see the Higgs (see next slide) at LHC

– Suspect that there is a complete shadow world of particles [SUSY]

– Have a dream that all forces including gravity will be unified

Page 27: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• What is Higgs for?– It is a field that fills the universe and gives particles mass

THE “CELEBRITY AT PARTY” MODEL (quarks or leptons)

THE “rumour” model (Higgs particle)

Particle Mass determined by strength of interaction with higgs field

Page 28: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• Stars and Planets only account for a small

percentage of the universe !

Page 29: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

27KM tunnel 100m below the surfaceWorld’s Largest cryogenic system ((1.8 K, suprafluid helium)

Page 30: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

CERN Technologies

Dipoles for the LHC arrive from industry

Page 31: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.
Page 32: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Magnet – Cryostat Assembly

Page 33: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Magnet installation

Page 34: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

ATLAS Cavern

Page 35: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Concorde(15 Km)

Balloon(30 Km)

CD stack with1 year LHC data!(~ 20 Km)

Mt. Blanc(4.8 Km)

Data in Large Quantities

Page 36: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

What is the Grid?

• The World Wide Web provides seamless access to information that is stored in many millions of different geographical locations

• In contrast, the Grid is an emerging infrastructure that provides seamless access to computing power and data storage capacity distributed over the globe.

Page 37: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

CMS

Page 38: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Technology Transfer Projects

Silicon detector for a Compton camera in nuclear medical imaging

Thin films by sputtering or evaporation

Medipix: Medical X-ray diagnosis with contrast enhancement and dose reduction

Radio-isotope production for medical applications

Radiography of a bat, recorded with a GEM detector

Page 39: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

CERN as Educator

Page 40: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Bringing Nations Together

“…the promotion of contacts between, and

the interchange of, scientists…”

Page 41: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

CERN…

• Seeking answers to questions about the Universe

• Advancing the frontiers of technology• Training the scientists of tomorrow• Bringing nations together through science

Page 42: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• Backup1) Einstein

2) Cosmology slides

Page 43: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• Another motivation drove Rabi. He considered CERN a peaceful compensation for building the nuclear bomb. This was revealed when I invited him to speak at CERN's 30-year anniversary celebration in 1984. Here are excerpts from his comments:

• CERN was founded less than 10 years after the bomb was made. I feel that the existence of the bomb and its success had a large part in making CERN possible. . . . I am not at all surprised at the great achievements of CERN. I expected that. I was sure that Europe, which was the cradle of science, once brought back into the path, would achieve some very great things. . . . I mentioned Los Alamos and the atomic bomb, which is an expression of the power of [the] personalities [involved]. They are here now before you, and it is important to keep them occupied fulfilling the ideals of science. . . .

• I hope that the scientists at CERN will remember that they have other duties than exploring further into particle physics. They represent the combination of centuries and centuries of investigation and study and scholarship to show the power of human spirit. So I appeal to them not to consider themselves as technicians . . . but . . . as guardians of this flame of European unity so that Europe can help preserve the peace of the world.

• By bringing together scientists from Europe and the rest of the world, CERN has lived up to this objective better than its founding fathers expected.

• Herwig Schopper

Page 44: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• Albert Einstein (1879 – 1955)

Germany Switzerland Germany USA

• Photoelectric effect (wave/particle), Relativity, E = mc² , Cosmology & gravitation

• “I never think of the future - it comes soon enough.” • • "If we knew what it was we were doing, it would not be called research”

• “Only two things are infinite, the universe and human stupidity, and I'm not sure about the former." --Albert Einstein”

• “Imagination is more important than knowledge...”

Arguably the greatest scientist ever – and his views remain fashionable

Page 45: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Gravity at large distances

Einstein

Newton

“UniversalGravitation”

Mass and energyCurve space-time

Page 46: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Gravity at small distances

Collapsing stars produceBlack holes

Observation of a black hole candidate

What is a singularity ?

Page 47: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

really small distances Gravity : dominant force at r ~ 10-33 cm

Quantum Gravity ?

Superstrings in 11 dimensions?

Does gravity only act in 3 dimensions?

- Macroscopic : YES ( 1/r2 law)- Microscopic : no information for r < 10 µm

What is a particle ?

Page 48: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• Stars and Planets only account for a small percentage of the universe !

Page 49: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Cosmology – Big Bang•

< 10-43 sec: Planck era

~10-34 sec: inflation

10-32 sec “big bang”

10-10 ... 1 sec particles

380,000 yrs atoms

BB

Page 50: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Before the Big BANG ?•

The primordial vacuum: 1094 GeV/cm3 ?

Page 51: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

• Evidence No. 1 - Cosmic Microwave backgroundEvidence No. 2 - Expansion history of universe

COSMIC EXPANSION SPEED INCREASES!

Driven by ‘dark energy’

Page 52: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Courtesy: NASA/WMAP

FIT observation with BIG BANG MODEL - 1) Inflation stretches ‘quantum ripples’2) Light element synthesis (matter)3) Dark (=non-baryonic) matter4) Age and shape of universe

Page 53: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

Cosmic Microwave background Temperature Distribution on earth (for comparison)

Temperature Distribution In Universe

T/T ~ 0.3

T/T ~ 3·10-5

Courtesy: NASA/WMAP

Page 54: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.

A non-baryonic dark halo

Milky Way:Mhalo ~ 10 x Mvisible

Microlensing baryonic matternot the solution

A dark non-baryonic halo, ~ 0.3 GeV / cm3

v ~ 220 km / s

Excluded by

MACHO

MACHOdetection

Page 55: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.
Page 56: Overview of CERN & the physics raison d’être The search for elementary particles  explanation of the universe Historical perspective Particle physics.