Emmanuel Tsesmelis - PowerPoint PPT Presentation

1 / 58
About This Presentation
Title:

Emmanuel Tsesmelis

Description:

Emmanuel Tsesmelis – PowerPoint PPT presentation

Number of Views:82
Avg rating:3.0/5.0
Slides: 59
Provided by: emm129
Category:

less

Transcript and Presenter's Notes

Title: Emmanuel Tsesmelis


1
applications of acceleratorsparticle
physics
  • Emmanuel Tsesmelis
  • CERN/Oxford
  • University of Oxford
  • 1 December 2009

2
introduction
3
Evolution of the Universe
Big Bang
4
The Study of Elementary Particles and Fields and
their Interactions
In 50 years, weve come a long way, but there is
still much to learn
5
(No Transcript)
6
Open Questions in Particle Physics
  • What is the origin of particle masses?
  • Why are there so many types of matter particles?
  • What is the cause of matter-antimatter asymmetry?
  • What are the properties of the primordial plasma?
  • What is the nature of the invisible dark matter?
  • Can all fundamental particles be unified?
  • Is there a quantum theory of gravity?
  • The present and future accelerator-based
    experimental programmes will address all these
    questions and may well provide definite answers.

7
Introduction - Accelerators
  • Historically, HEP has depended on advances in
    accelerator design to make scientific progress
  • cyclotron ? synchrocyclotron ? synchrotron ?
    collider (circular, linear)
  • Advances in accelerator design and performance
    require corresponding advances in accelerator
    technologies
  • Magnets, vacuum systems, RF systems,
    diagnostics,...
  • Accelerators enable the study of particle physics
    phenomena under controlled conditions
  • Costs time span of todays accelerator projects
    are high
  • International co-operation and collaboration are
    obligatory

8
Introduction - Accelerators
  • Particle accelerators are designed to deliver two
    parameters to the HEP user
  • Energy
  • Luminosity
  • Measure of collision rate per unit area
  • Event rate for a given event probability
    (cross-section) given by
  • For a Collider luminosity is given by
  • ? Require intense beams and small beam sizes at
    IP

9
Todays Accelerators
  • HEP typically uses Colliders
  • Counter-propagating beams that collide at one or
    more IPs
  • Colliders typically store various types of
    particles
  • Hadrons (protons, ions)
  • Tevatron (p, anti-p), RHIC (p, ions), LHC (p,
    ions)
  • Leptons (electrons)
  • CESR-c, PEP-II, KEK-B

10
Todays Accelerators
  • Hadron Colliders
  • Protons are composite particles
  • Only 10 of beam energy available for hard
    collisions producing new particles
  • Need O(10 TeV) Collider to probe 1 TeV mass scale
  • Desired high energy beam requires strong magnets
    to store and focus beam in reasonable-sized ring.
  • Anti-protons difficult to produce if beam is lost
  • Use proton-proton collisions instead
  • Demand for ever-higher luminosity has led LHC to
    choose proton-proton collisions
  • Many bunches (high bunch frequency)
  • Two separate rings that intersect at select
    locations

11
Todays Accelerators
  • Lepton Colliders (ee-)
  • Synchrotron radiation is the most serious
    challenge
  • Emitted power in circular machine is
  • For a 1 TeV CM energy Collider in the LHC tunnel
    with a 1 mA beam, radiated power would be 2 GW
  • Would need to replenish radiated power with RF
  • Remove it from vacuum chamber
  • Approach for high energies is Linear Collider
    (ILC,CLIC)

12
Future Accelerators
  • Currently, there are several machines under
    design to address open issues in HEP
  • Not all of the future machines are at the same
    stage of development
  • Costs are typically high ? it is likely that not
    all will be built
  • Precision Frontier
  • ILC (ee-) energy frontier
  • Neutrino Factory (µ or µ-)
  • Super-B Factory (ee-)
  • Energy Frontier
  • sLHC
  • CLIC (ee-) precision frontier
  • Muon Collider (µµ-)

13
THE Large hadron Collider
14
CERN Accelerator Complex
15
LHC Accelerator Experiments
CMS/TOTEM
LHCb
ATLAS/LHCf
ALICE
16
The Large Hadron Collider
High repetition rate 40 MHz or 25 ns bunch
spacing
17
LHC Lay-out
  • The LHC is a two-ring superconducting
    proton-proton collider made of eight 3.3 km long
    arcs separated by 528 m Long Straight Sections.
  • While the arcs are nearly identical, the straight
    sections are very different.

18
LHC Nominal Performance
Bunch spacing 25 ns.
19
LHC Main Bending Cryodipole
8.3 T nominal field 11850 A nominal field
20
The LHC Arcs
21
The LHC Experimental Challenge
22
ATLAS and CMS
  • Of central importance for ATLAS CMS and for the
    Collider is to elucidate the nature of
    electroweak symmetry breaking for which the Higgs
    mechanism (and accompanying Higgs boson(s)) are
    presumed to be responsible.
  • Discover the Higgs Boson(s) for mHlt 1 TeV
  • ATLAS CMS are general-purpose detectors and can
    study the production of a variety of particles.
  • e.g. Supersymmetric particle production

23
The ATLAS Experiment
Number of scientists 2200 Number of
institutes 167 Number of countries 37
24
The ATLAS Experiment
25
First Collisions - ATLAS
450 GeV x 450 GeV pp collision
26
Electro-weak phase transition (ATLAS, CMS)
QCD phase transition (ALICE, CMS)
LHC will study the first 10-10 -10-5 seconds
27
Cross sections at the LHC
Well known processes. Dont need to keep all
of them
New Physics!! We want to keep!!
28
The BEH Mechanism()
()Brout-Englert-Higgs
EPS09
29
Higgs Searches
High MH gt 500 GeV/c2
Medium 130ltMHlt500 GeV/c2
Low MH lt 140 GeV/c2

29
30
Search for Higgs at LHC Start-up
  • Sizeable integrated luminosity is needed before
    significant inroads can be made in SM Higgs
    search.
  • However, even with moderate luminosity per
    experiment, Higgs boson discovery is possible in
    particular mass regions.

Example Reach ATLAS CMS
31
Beyond the Higgs Boson
Supersymmetry A New Symmetry in Nature
Candidate Particles for Dark Matter ? Produce
Dark Matter in the lab
SUSY particle production at the LHC

31
Picture from Marusa Bradac
32
Supersymmetry
SUSY could be at the rendez-vous very early on!
10fb-1
Main signal lots of activity (jets, leptons,
taus, missing ET) Needs however good
understanding of the detector SM processes!!

32
33
Peak Luminosity
New Injectors IR Upgrade Phase 2
Linac4 IR Upgrade Phase 1
Early operation
Collimation Phase 2
34
Integrated Luminosity
New Injectors IR Upgrade Phase 2
Linac4 IR Upgrade Phase 1
Early operation
Collimation Phase 2
35
LHC Upgrade
Present Accelerators
Future Accelerators
Proton flux / Beam power
Linac4
Linac2
50 MeV
160 MeV
PSB
LPSPL
1.4 GeV
4 GeV
LPSPL Low Power Superconducting Proton Linac (4
GeV) PS2 High Energy PS ( 5 to 50 GeV 0.3
Hz) SPS Superconducting SPS (50 to1000
GeV) SLHC Superluminosity LHC (up to 1035
cm-2s-1) DLHC Double energy LHC (1 to 14 TeV)
PS
26 GeV
PS2
50 GeV
Output energy
SPS
SPS
450 GeV
1 TeV
LHC / SLHC
DLHC
7 TeV
14 TeV
Intermediate step in reaching 1035 cm-2s-1
36
Layout of the New Injectors
SPS
PS2
ISOLDE
PS
SPL
Linac4
37
Interaction RegionFinal Focusing
38
The Tevatron at FERMILAB
39
The Tevatron at FERMILAB
40
Linear ColliDers
40
41
Colliders Energy vs. Time
  • pp and ee- colliders
  • have been operational
  • simultaneously

42
Linear ee- Colliders
  • The machine which will complement and extend the
    LHC best, and is closest to be realized, is a
    Linear ee- Collider with a collision energy of
    at least 500 GeV.


PROJECTS ? TeV Colliders (CMS energy up to 1
TeV) ? Technology ready NLC/GLC/TESLA? ILC
with superconducting cavities ?
Multi-TeV Collider (CMS energies in multi-TeV
range) ? RD CLIC ? Two Beam Acceleration
43
A Generic Linear Collider
30-40 km
44
International Linear Collider Baseline Design
  • 250

250 Gev
250 Gev
e e- Linear Collider Energy 250 Gev x 250
GeV of RF units 560 of cryomodules
1680 of 9-cell cavities 14560 2 Detectors
push-pull peak luminosity 2 1034 5 Hz rep
rate, 1000 -gt 6000 bunches IP sx 350 620 nm
sy 3.5 9.0 nm Total power 230
MW Accelerating Gradient 31.5 MeV/m
45
The International Linear Collider
46
CLIC Conceptual Design
  • Site independent feasibility study aiming at the
    development of the technologies needed to extend
    e / e- linear colliders into the multi-TeV
    energy range.
  • Ecm range complementary to that of the LHC ILC
  • Ecm 0.5 3 TeV
  • L gt few 1034 cm-2 s-1 with low machine-induced
    background
  • Minimise power consumption and costs

47
CLIC Overall Lay-out
48
Basic Features
CLIC TUNNEL CROSS-SECTION
  • High acceleration gradient gt 100 MV/m
  • Compact collider total length lt 50 km at 3
    TeV
  • Normal conducting acceleration structures at high
    frequency
  • Novel Two-Beam Acceleration Scheme
  • Cost effective, reliable, efficient
  • Simple tunnel, no active elements
  • Modular, easy energy upgrade in stages

4.5 m diameter
Main beam 1 A, 156 ns from 9 GeV to 1.5
TeV 100 MV/m
Drive beam - 95 A, 240 ns from 2.4 GeV to 240 MeV
12 GHz 64 MW
49
Main Parameters Challenges
  • High beam power (several MWatts)
  • Wall-plug to beam transfer efficiency as high as
    possible (several )
  • Generation preservation of beam emittances at
    I.P. as small as possible (few nmrad)
  • Beam focusing to very small dimensions at IP
    (few nm)
  • Beamstrahlung energy spread increasing with c.m.
    colliding energies

50
CLIC Parameters
51
Generic Detector Concepts
A lot of RD work on detectors is in
progress good tracking resolution, jet flavour
tagging, energy flow, hermeticity,
52
Indicative Physics Reach
Ellis, Gianotti, de Roeck Hep-ex/0112004 updates
Units TeV (except WLWL reach)
indirect search (from precision measurements)
53
Muon accelerators
53
54
Physics with Muon Beams
  • Neutrino Sector
  • Decay kinematics well known
  • ?e ? ?µ oscillations give easily detectable
    wrong-sign µ
  • Energy Frontier
  • Point particle makes full beam energy available
    for particle production
  • Couples strongly to Higgs sector
  • Muon Collider has almost no synchrotron radiation
  • Narrow energy spread
  • Fits on existing laboratory sites

55
Muon Beam Challenges
  • Muons created as tertiary beam (p ? ? ? µ)
  • Low production rate
  • Need target that can tolerate multi-MW beam
  • Large energy spread and transverse phase space
  • Need solenoidal focusing for the low-energy
    portions of the facility
  • (solenoids focus in both planes simultaneously)
  • Need acceptance cooling
  • High-acceptance acceleration system and decay
    ring
  • Muons have short lifetime (2.2 µs at rest)
  • Puts premium on rapid beam manipulations
  • Presently untested ionization cooling technique
  • High-gradient RF cavities (in magnetic field)
  • Fast acceleration system
  • Decay electrons give backgrounds in Collider
    detectors and instrumentation heat load to
    magnets

56
Neutrino Factory
Aim for 1021 ?e per year directed towards
detector(s)
57
Muon Collider
e.g. _at_ FNAL
58
Summary and Conclusions
  • Highest priority of the particle physics
    community is to fully exploit the physics
    potential of the LHC.
  • The European Strategy for Particle Physics
    incorporates a number of new accelerator projects
    for the future.
  • The need to renovate the LHC injectors is
    recognised and relevant projects/studies have
    been authorised.
  • The main motivation to upgrade the luminosity of
    the LHC is to explore further the physics beyond
    the Standard Model while at the same time
    completing the Standard Model physics started at
    the LHC.
  • Further down the line, many of the open questions
    from the LHC could be best addressed by lepton
    machines.
  • An electron-positron collider (ILC or CLIC) in
    which all the centre-of-mass energy is made
    available for collisions between the colliding
    elementary particles.
  • A neutrino factory/muon collider is also under
    design.
  • These new initiatives will lead particle physics
    well into the next decades of fundamental
    research.
Write a Comment
User Comments (0)
About PowerShow.com