Advanced beam manipula/ons
|
|
- Annabella Reynolds
- 5 years ago
- Views:
Transcription
1 Advanced beam manipula/ons Beam manipula+ons involves the interac+on of the beam with external fields: laser tailored RF field (e.g. mul+ frequency) external beams The beam manipula+ons topics explored so far were aimed at tailoring the beam s phase spaces The same type of manipula+ons can be used to cool the beam 1
2 What is cooling? Reduc+on of the phase space volume Liouville s theorem states that in a well- behaved system (linear, non interac+ng, ) this cannot happen When collec+ve effects and aberra+ons are taken into account the phase space actually dilutes No magnet can provide such a phase space reduc+on (cooling) effect 2
3 Cooling principle most cooling schemes are based on an exchange of energy with an external system We already saw one type of cooling: radia+on cooling due to synchrotron- radia+on emission (t) =Ae Et cos( t ) (t) =Be Et sin( t ) 3
4 Type of cooling Radia+on cooling: light par+cles (electrons) cool themselves by emizng radia+on. Can also be performed with an external laser Electron cooling for low/medium- energy protons, an+protons and ions* Stochas+c cooling for medium/high- energy protons, an+protons and ions Laser cooling for a few kinds of atomic ions Ioniza+on cooling, soon, for muon cooling 4
5 Electron cooling Invented by Budker (1966) Cool hot ions beam using a cold electron beam Relies on the rela+ve fric+on force between ions and electrons Consider the Rutherford cross sec+on Z: ion charge state, and ( ) = µ m im e m i + m e Z 2 e 4 1 4(4 ") 2 µ 2 u 4 sin 4 /2 ion at rest 5
6 Fric/on force The change in e- longitudinal velocity is u z = u(1 cos ) =2usin 2 /2 so that the average change is h u z i = Z can integrate [Maxima]: where the Coulomb log is =2 u z Z max ( )ud min u z ( )u sin d h u z i = 4 Ze L c log sin( max/2) sin( min /2) 2 L c µ 2 u 2 6
7 Fric/on force Can be generalized to the ion velocity as (invoking momentum conserva+on in the ion s frame) to yield h v i i = 4 Ze corresponding to a force : F m i h v i i = 4 2 Ze 2 L c m e m i v i v e v i v e Lc m e v i v e v i v e 3 which can be average over the e- distribu+on 7
8 Prac/cal implementa/on velocity of ion and electron should match for prolonged interac+on 8
9 Stochas/c cooling Beam informa+on is picked- up manipulated and fed back to the beam Liouville s theorem does not apply Simple model a difference pick- up measures the bary- center of a beam slice A kicker correct for the measured displacement from H. Danared, 2005 CERN accelerator school, Zeegse, Netherlands 9
10 Stochas/c cooling The beam is sampled with a +me resolu+on of T 1/! where! is the pick- up bandwidth The cooling rate is es+mated as 1 = 1! TN S N where N s = N T s is the number of T ' N T! sample slices taken large cooling decrement requires large bandwidth 10
11 Experimental implementa/on FNAL pioneered many aspects of stochas+c cooling 11
12 Recent advances coherent electron cooling Phys. Rev. Lei. 102, (2009) Vladimir N. Litvinenko and Yaroslav S. Derbenev E < E h E h E < E h Hadrons Modulator Dispersion section ( for hadrons) E > E h E h Kicker E > E h λ l 1 High gain FEL (for electrons) l 2 Electrons op+cal stochas+c cooling Phys. Rev. Lei. 75, 4146 (1993) A. Mikhailichenko and M. Zolotorev 12
13 ioniza/on cooling par+cle passes through maier all momentum component are reduced longitudinal momentum is restored via accelera+ng cavi+es limited to few par+cle type: scaiering increases emiiance and there is an equilibrium (the beam cannot be cooled indefinitely) 13
14 laser cooling mainly used to cool non- rela+vis+c atoms and trapped ions laser with frequency slightly below a strong transi+on is used Doppler effects is used to provide a velocity- dependent force via the Doppler shil =! 0! k.v transi+on frequency laser frequency p =(~!/c, ~k) 14
15 what is the ul/mate cooling limit? in principle the beam can be cooled to the quantum limit " ~ the beam is then described by its wave func+on (cannot take the classical approach anymore) in prac+ce because of repulsive forces in mono- species beams there is an equilibrium between cooling force and space charge forma+on of crystals 15
16 Crystalline beams condi+on for forma+on: kine+c energy of par+cle << elec. poten+al in such a case par+cle are trapped in the electrosta+c poten+al and get cooled in an ordered fashion kine+c energy of par+cle is represented by emiiance 16
17 from A. Chao, hip:// 1D Crystalline beams Consider a lazce arranged as a 1D string with par+cle located as where par+cle mass and charge are M and Q the equa+on of mo+on of the nth par+cle is n a Coulomb force contribu+on from lel (not missing) 4 0 Coulomb force contribu+on from right (not missing)
18 from A. Chao, hip:// 1D crystalline beam previous equa+on can be linearized to yield eigenmode of this system of equa+on are 18
19 Example of crystalline beams simula+on of laser cooling in rings 19
20 Experimental forma/on of Coulomb realized in the lab: in ion storage rings in atomic molasse Crystals mostly achieved for species that have an op+cal transi+on (easy to reach with laser) 20
Advanced beam manipula/ons
Advanced beam manipula/ons beam manipula+ons are two fold: transverse (focusing, shaping, ) longitudinal (tailoring the current of energy spectrum of a beam) Transverse shaping is rather straigh>orward
More informationfree- electron lasers I (FEL)
free- electron lasers I (FEL) produc'on of copious radia'on using charged par'cle beam relies on coherence coherence is achieved by insuring the electron bunch length is that desired radia'on wavelength
More informationAccelera'on II. dt = qv.e. Coupling of wave with a charged par4cle. e.m. waves need to be localized in space to maximize interac4on region.
Accelera'on II Coupling of wave with a charged par4cle change in energy de dt = qv.e velocity applied E field e.m. waves need to be localized in space to maximize interac4on region. 1 accelera'on with
More informationPar$cles. Ma#er is made of atoms. Atoms are made of leptons and quarks. Leptons. Quarks. atom nucleus nucleon quark m m m m
Par$cles Ma#er is made of atoms atom nucleus nucleon quark 10-10 m 10-14 m 10-15 m 10-18 m Atoms are made of leptons and quarks Leptons ν e e Quarks u d What Have We Learned? Rela?vis?c Quantum Mechanics
More information- Covered thus far. - Specific Intensity, mean intensity, flux density, momentum flux. - Emission and absorp>on coefficients, op>cal depth
- Covered thus far - Specific Intensity, mean intensity, flux density, momentum flux - Emission and absorp>on coefficients, op>cal depth - Radia>ve transfer equa>on - Planck func>on, Planck spectrum, brightness
More informationBeam Cooling. Beam Cooling. M. Steck, GSI, Darmstadt CERN Accelerator School Chios, Greece September 18 30, Introduction. 1.
Beam Cooling, GSI, Darmstadt CERN Accelerator School, September 18 30, 2011 Beam Cooling Introduction 1.Electron Cooling 2.Ionization Cooling 3.Laser Cooling 4.Stochastic Cooling Beam Cooling Beam cooling
More informationLecture 2: Transfer theory. Credit: Kees Dullemond
Lecture 2: Transfer theory Credit: Kees Dullemond What is radia:ve transfer? Radia:ve transfer is the physical phenomenon of energy transfer in the form of electromagne:c radia:on The propaga:on of radia:on
More informationBeam Cooling. M. Steck, GSI, Darmstadt. JUAS, Archamps, France March 9, 2015
Beam Cooling M. Steck, GSI, Darmstadt JUAS, Archamps, France March 9, 2015 time longitudinal (momentum) cooling Cooling injection into storage ring transverse cooling Xe 54+ 50 MeV/u p/p cooling off with
More informationExperimental Storage Ring - ESR E max = 420 MeV/u, 10 Tm, electron-, stochastic- and laser cooling. Indian Institute of Technology Ropar
Experimental Storage Ring - ESR E max = 420 MeV/u, 10 Tm, electron-, stochastic- and laser cooling Specification of the ESR Particle detectors Re-injection to SIS Two 5 kv rf-cavities Fast Injection Schottky
More informationMagne&c Dissipa&on in Rela&vis&c Jets
Magne&c Dissipa&on in Rela&vis&c Jets Yosuke Mizuno Ins$tute for Theore$cal Physics Goethe University Frankfurt In Black Hole Cam collabora$on (Theory Team) Blazars through Sharp Mul$- Frequency Eyes,
More informationGlasma to plasma: classical coherence, quantum decoherence & thermaliza7on in the li8le Bang. Raju Venugopalan
Glasma to plasma: classical coherence, quantum decoherence & thermaliza7on in the li8le Bang Raju Venugopalan Lecture iv, UCT, February 2012 Outline of lectures Lecture I: QCD and the Quark- Gluon Plasma
More informationInves&ga&on of atomic processes in laser produced plasmas for the short wavelength light sources
Inves&ga&on of atomic processes in laser produced plasmas for the short wavelength light sources Akira Sasaki Quantum Beam Science Directorate Japan Atomic Energy Agency Introduc&on EUV source at λ=6.5nm
More informationNeutrino Oscilla8ons
Neutrino Oscilla8ons Kathleen Tatem Columbia University Neutrino oscilla8on experiments may be seeing signs of a new fundamental par8cle, the sterile neutrino! 1 Outline Neutrinos Proper8es Sources Neutrino
More information7. Quantum Monte Carlo (QMC)
Molecular Simulations with Chemical and Biological Applications (Part I) 7. Quantum Monte Carlo (QMC) Dr. Mar(n Steinhauser 1 HS 2014 Molecular Simula(ons with Chemical and Biological Applica(ons 1 Introduc5on
More informationPhase Space Gymnastics
Phase Space Gymnastics As accelerator technology advances, the requirements on accelerator beam quality become increasingly demanding. Phase space gymnastics becomes a new focus of accelerator physics
More informationMake sure your clickers are out and ready before class starts
No homework due this week and no quiz in Fri/Mon recita7ons. Homework #5 is due next Tuesday 16 Oct at 11:59PM We are gegng the exams graded and I will email you when you can look up the results in the
More informationfree- electron lasers II (FEL)
free- electron lasers II (FEL) undulator radia+on in the lab frame has the wavelength undulator period l = u 2 2 beam Lorentz factor K = eb 0 = eb 0 u mck u 2 mc ' 0.934B 0[T] u[cm] 1+ K2 2 + 2 2 angle
More informationφ) = 1 2 [( µφ) 2 m 2 φ 2 ] V(φ)
Status of the theory (Langacker nota3on) Perturba)ve field theory is characterized by weak coupling (finite higher order correc)ons) Lagrangian of a field theory contains interac)on ver)ces L(φ, µ φ) =
More informationClassical and Quantum Proper3es of Screened Modified Gravity
Classical and Quantum Proper3es of Screened Modified Gravity Philippe Brax IPhT Saclay P.B, C. van de Bruck, A.C. Davis, B. Li, H. Winther, G. Zhao etc and in progress «Quantum vacuum» workshop, LKB December
More informationBeam Cooling M. Steck, GSI Darmstadt CAS Advanced Accelerator Physics, Royal Holloway University of London, 3-15 September 2017
Beam Cooling M. Steck, GSI Darmstadt CAS Advanced Accelerator Physics, Royal Holloway University of London, 3-15 September 2017 Observation of Cooling Xe 54+ beam at 400 MeV/u cooled with electron current
More informationMa#er: What it is 1/17/15. What does it Ma#er?
Ma#er: What it is What does it Ma#er? 1. Our world is made of energy and ma7er. 2. Ma7er is a conglomera;on of fundamental par;cles. 3. Some par;cles are composites of fundamental par;cles. 4. The fundamental
More informationCosmic Ray Electrons with CTA. R.D. Parsons
Cosmic Ray Electrons with CTA R.D. Parsons Cosmic Ray Electrons In addi:on to the well known hadronic component of cosmic rays there is a more poorly understood electronic component Has a lower flux than
More informationPar$cle- Driven Plasma Wakefield Accelera$on
Par$cle- Driven Plasma Wakefield Accelera$on James Holloway University College London, London, UK PhD Supervisors: Professor MaHhew wing University College London, London, UK Professor Peter Norreys Central
More informationHc 5: Outline. Book by Tipler, chapter 12.2
Hc 5: Outline Introduc:on Produc:on and iden:fica:on of par:cles Basic concepts: par:cle- an:par:cle, leptons and hadrons Fundamental interac:ons and force carriers Conserva:on laws and symmetries The
More informationLecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Heavier quarks FK
Lecture 6 Isospin What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Heavier quarks FK7003 33 SU() Isospin Isospin introduced based on the observa4on that: m p = 0.9383 GeV and
More informationWeek 12, Lecture 2 Nuclear Synthesis
Week 12, Lecture 2 Nuclear Synthesis Nuclear Reac*ons in Space - - Overview - - Observa
More informationComments About Varied IEC Approaches to Fusion Power
Comments About Varied IEC Approaches to Fusion Power George H Miley NPRE, University of Illinois, Urbana, IL 61801 Email: ghmiley@illinois.edu Abstract IEC Fusion concepts can be broadly categorized as
More informationThe Strong Interaction
The Strong Interaction What is the quantum of the strong interaction? The range is finite, ~ 1 fm. Therefore, it must be a massive boson. Yukawa theory of the strong interaction Relativistic equation for
More informationReversible vs. irreversible processes
Reversible vs. irreversible processes A reversible process is one for which the final states of the universe (system and environment) are iden
More informationLaser- Accelerated Proton Beams and their Medical Applica6ons. By Eric Sacks
Laser- Accelerated Proton Beams and their Medical Applica6ons By Eric Sacks Contents 1) Basics of charged par6cle interac6ons in ma@er. 2) Proton- Therapy 3) Laser- Accelera6on method for producing Proton
More informationA 21 spontaneous radia:ve decay (s - 1 ) B 12 induced excita:on (via photons) [B 12 U ν s - 1 ]
Collisionally- excited emission Lines Excita:on and emission in a - level atom Emission Lines Emission lines result from photon- emiang downward transi:ons, and provide key informa:on on the emiang objects,
More informationPar$cle Astrophysics
Par$cle Astrophysics Produc$on (Early Universe) Signatures (Large Scale Structure & CMB) Accelerator Detector Neutrinos and Dark MaCer were produced in the early universe Star$ng Point: Cosmic Photons
More informationQCD and Modern Theore.cal Nuclear Physics
QCD and Modern Theore.cal Nuclear Physics Strong interac,ons generate the energy in stars Strong interac,ons generate the masses of nucleons and therefore the visible mass of the universe Control the interac,ons
More informationPhysics 2203, Fall 2012 Modern Physics
Physics 2203, Fall 2012 Modern Physics. Monday, Aug. 27 th, 2011: Start Ch. 2: Rela@vis@c Momentum, Energy, Conversion of mass and Energy. Do classical laws of momentum and energy conserva@on remain valid
More informationCollisionally- excited emission Lines
Collisionally- excited emission Lines Excita9on and emission in a 2- level atom Emission Lines Emission lines result from photon- emi@ng downward transi9ons, and provide key informa9on on the emi@ng objects,
More informationAccelerator Physics. Tip World Scientific NEW JERSEY LONDON SINGAPORE BEIJING SHANGHAI HONG KONG TAIPEI BANGALORE. Second Edition. S. Y.
Accelerator Physics Second Edition S. Y. Lee Department of Physics, Indiana University Tip World Scientific NEW JERSEY LONDON SINGAPORE BEIJING SHANGHAI HONG KONG TAIPEI BANGALORE Contents Preface Preface
More informationThe achievements of the CERN proton antiproton collider
The achievements of the CERN proton antiproton collider Luigi DiLella Scuola Normale Superiore, Pisa, Italy Motivation of the project The proton antiproton collider UA1 and UA2 detectors Discovery of the
More informationStudies of trapped modes in the new extraction septum of the CERN Proton Synchrotron
Studies of trapped modes in the new extraction septum of the CERN Proton Synchrotron Serena Persichelli CERN Impedance and collective effects (BE-ABP-ICE) LIU LHC Injectors Upgrade project Università di
More informationNumerical Evolu.on of Soliton Stars Dr. Jayashree Balakrishna (HSSU Saint Louis, Missouri)
Numerical Evolu.on of Soliton Stars Dr. Jayashree Balakrishna (HSSU Saint Louis, Missouri) Collaborators: M. Bondarescu (Ole Miss. ), R. Bondarescu (Penn. State), G. Daues (N.C.S.A), F.S. Guzman (Mexico),
More informationLecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Gell- Mann- Nishijima formula FK
Lecture 6 Isospin What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Gell- Mann- Nishijima formula FK7003 08 SU() Isospin Isospin introduced based on the observa4on that: m p =
More informationThe Color Glass Condensate: Theory, Experiment and the Future
The Color Glass Condensate: Theory, Experiment and the Future Physics Issues: What is the high energy limit of strong interac?ons? How do we compute the gluon and quark distribu?ons relevant for asympto?cally
More informationNoncommuta5ve Black Holes at the LHC
Noncommuta5ve Black Holes at the LHC Elena Villhauer Karl Schwartzschild Mee5ng 2017 25/07/2017 Outline Hierarchy Problem Condi2ons for black hole Produc2on at the LHC Brief tour of results from searches
More informationWhat is Op*cs? Photonics?
What is Op*cs? Photonics? Think of op*cs as the science of light. It s a branch of physics that describes the behavior and proper*es of light and the interac*on of light with ma
More informationThe GSI Anomaly. M. Lindner. Max-Planck-Institut für Kernphysik, Heidelberg. Sildes partially adopted from F. Bosch
The GSI Anomaly M. Lindner Max-Planck-Institut für Kernphysik, Heidelberg Sildes partially adopted from F. Bosch What is the GSI Anomaly? Periodically modualted exponential β-decay law of highly charged,
More informationChallenges and Approaches to Nanoscale Materials Characteriza5on at Atomic Resolu5on
Challenges and Approaches to Nanoscale Materials Characteriza5on at Atomic Resolu5on Ralph G. Nuzzo G. L. Clark Professor of Chemistry and Professor of Materials Science and Engineering University of Illinois
More informationEngines of Discovery
Engines of Discovery R.S. Orr Department of Physics University of Toronto Berkley 1930 1 MeV Geneva 20089 14 TeV Birth of Particle Physics and Accelerators 1909 Geiger/Marsden MeV a backscattering - Manchester
More informationGlobal properties of atomic nuclei
Global properties of atomic nuclei How to probe nuclear size? Electron Sca5ering from nuclei For low energies and under condi0ons where the electron does not penetrate the nucleus, the electron sca5ering
More informationToday: - Heat and Thermal Mo2on
Dec 2nd, 2015 LB 273, Physics I Prof. Vashti Sawtelle Prof. Leanne Doughty Today: - Heat and Thermal Mo2on Slainte! Cheers! Irish Phrasebook (it s really the Gaelic word for health ) Final Exam Announcements
More informationBasic Mathema,cs. Rende Steerenberg BE/OP. CERN Accelerator School Basic Accelerator Science & Technology at CERN 3 7 February 2014 Chavannes de Bogis
Basic Mathema,cs Rende Steerenberg BE/OP CERN Accelerator School Basic Accelerator Science & Technolog at CERN 3 7 Februar 014 Chavannes de Bogis Contents Vectors & Matrices Differen,al Equa,ons Some Units
More informationPART 2. Formalism of rela,vis,c ideal/viscous hydrodynamics
PART 2 Formalism of rela,vis,c ideal/viscous hydrodynamics Adver&sement: Lecture Notes Hydrodynamics Framework to describe space- &me evolu&on of thermodynamic variables Balance equa&ons (equa&ons of mo&on,
More informationElectricity & Magnetism Lecture 12
Electricity & Magnetism Lecture 12 Today s Concept: Magne2c Force on Moving Charges Electricity & Magne2sm Lecture 12, Slide 1 Today s rants I'm struggling a fair bit with this component of the course.
More informationS.Y. Lee Bloomington, Indiana, U.S.A. June 10, 2011
Preface Accelerator science took off in the 20th century. Accelerator scientists invent many innovative technologies to produce and manipulate high energy and high quality beams that are instrumental to
More informationLast week. The diaba)c circula)on. Associated isentropic mass budget in the Middleworld. Possible implica7ons for poten7al vor7city
Aarnout van Delden http://www.staff.science.uu.nl/~delde102/c&hc.htm Diaba%c- Dynamical Interac%on in the General Circula%on (lecture 7) The diaba)c circula)on Associated isentropic mass budget in the
More informationof a Fabry-Perot cavity
Circumven*on of radia*onpressure-induced angular instability of a Fabry-Perot cavity Koji Nagano 1, Yutaro Enomoto 1, Masayuki Nakano 1, Akira Furusawa 2, and Seiji Kawamura 1 Ins*tute for Cosmic Ray Research,
More informationR Process Nucleosynthesis And Its Site. Mario A. Riquelme Theore<cal Seminar Fall 2009
R Process Nucleosynthesis And Its Site Mario A. Riquelme Theore
More informationIntroduction to Collider Physics
Introduction to Collider Physics William Barletta United States Particle Accelerator School Dept. of Physics, MIT The Very Big Picture Accelerators Figure of Merit 1: Accelerator energy ==> energy frontier
More informationChapter 5. Par+cle Physics
Chapter 5 Par+cle Physics Types of Forces Force Range (m) Relative Strength Force Carrier Gravitational! 10-38 Graviton Weak 10-18 10-5 W ±, Z 0 Electromagnetic! =1/137 Photon Strong 10-15 1 Gluon What
More informationRecent Heavy Ion results from ATLAS experiment
Recent Heavy Ion results from ATLAS experiment Andrzej Olszewski (INP PAN Kraków) for the ATLAS Collabora@on International Nuclear Physics Conference Adelaide Convention Centre, Australia 11-16 September
More informationOp#mized Planar Penning Traps for Quantum Informa#on Studies
Op#mized Planar Penning Traps for Quantum Informa#on Studies Joshua Goldman Harvard University, Dept. of Physics Gabrielse Laboratory TCP2010, Saariselkä, Finland 12 April 2010 Outline I. Introduc#on:
More informationAWAKE, the Advanced Proton Driven Plasma Wakefield Accelera9on Experiment at CERN
AWAKE, the Advanced Proton Driven Plasma Wakefield Accelera9on Experiment at CERN Ulrik Uggerhøj many slides from a presenta0on at PSI by Edda Gschwendtner, CERN Main Driver for PWFA: Linear Collider è
More informationCamillo Mariani Center for Neutrino Physics, Virginia Tech
Camillo Mariani Center for Neutrino Physics, Virginia Tech Mo9va9on and Contents Determina9on of neutrino oscilla9on parameters requires knowledge of neutrino energy Modern experiments use complicated
More informationBack to Gauge Symmetry. The Standard Model of Par0cle Physics
Back to Gauge Symmetry The Standard Model of Par0cle Physics Laws of physics are phase invariant. Probability: P = ψ ( r,t) 2 = ψ * ( r,t)ψ ( r,t) Unitary scalar transformation: U( r,t) = e iaf ( r,t)
More informationWelcome to DESY. What is DESY and what kind of research is done here?
Welcome to DESY. What is DESY and what kind of research is done here? Michael Grefe DESY Press and Public Relations (PR) What is DESY? > Deutsches Elektronen-Synchrotron (German electron synchrotron) DESY
More informationCourse overview. Forces 5 lessons
Forces Mechanics Course overview Forces 5 lessons Newton s laws of mo9on (2 lessons) Mass and weight (0.5 lessons) Equilibrium (1 lesson) Unbalanced forces (1.5 lessons) Trolley Lab (DEF) Newton s first
More informationELIC: A High Luminosity And Efficient Spin Manipulation Electron-Light Ion Collider Based At CEBAF
ELIC: A High Luminosity And Efficient Spin Manipulation Electron-Light Ion Collider Based At CEBAF Lia Merminga and Yaroslav Derbenev Center for Advanced Studies of Accelerators, Jefferson Laboratory,
More informationON POSSIBILITIES OF FAST COOLING OF HEAVY PARTICLE BEAMS
ON POSSIBILITIES OF FAST COOLING OF HEAVY PARTICLE BEAMS Ya. S. Derbenev Randall Laboratory of Physics, University of Michigan Ann Arbor, Michigan 48109-1120 USA ABSTRACT Two methods of fast cooling of
More informationTheory of electron cooling
Theory of electron cooling Daria Astapovych 03/12/2014 HSC Meeting Outline Motivation and idea of the particle beam cooling Cooler Low energy, high energy beam Electron beam Kinetics of electron cooling
More informationSpecial Topics in Physics (Experiment) PHYS 8361 Tuesday +Thursday 12:30 pm 1:50 pm Hyer Hall G 021
Special Topics in Physics (Experiment) PHYS 8361 Tuesday +Thursday 12:30 pm 1:50 pm Hyer Hall G 021 Course Objec
More informationBeta decay: helicity
What are the consequences of parity viola:on in beta decay? h =! σ p! p helicity The eigenvalue of h is v/c. For a massless par:cle, the eigenvalues of h can be only +1 or -1. In general, the par:cle with
More informationRadia%ve Magne%c Reconnec%on. in Astrophysical Plasmas. Dmitri Uzdensky. (University of Colorado, Boulder) collaborators:
Radia%ve Magne%c Reconnec%on collaborators: in Astrophysical Plasmas Dmitri Uzdensky (University of Colorado, Boulder) - B. CeruF *, G. Werner, K. Nalewajko, M. Begelman (Univ. Colorado) - A. Spitkovsky
More informationIden%fica%on and energy calibra%on of hadronically decaying tau leptons with the ATLAS experiment.
Iden%fica%on and energy calibra%on of hadronically decaying tau leptons with the ATLAS experiment. Almut Pingel Niels Bohr Ins3tute on behalf of the ALTAS collabora3on ICHEP, Valencia (Spain) 3 July 214
More informationTwo-body weak decay of highly charged ions, a tool to study neutrino properties?
Two-body weak decay of highly charged ions, a tool to study neutrino properties? The detector: ESR Experimental Storage Ring cooling: electron-, stochastic ion detection: Schottky-noise, particle detector
More information(an) INTRODUCTION to HEAVY-ION PHYSICS
Journées de Rencontre des Jeunes Chercheurs 2015 La Saulaie 15-21 Novembre (an) INTRODUCTION to HEAVY-ION PHYSICS Antonio Uras - IPNL Outline Ø From the QCD to the Quark- Gluon Plasma v The strong interac3on
More informationChapter 7: Quantum Statistics
Part II: Applications - Bose-Einstein Condensation SDSMT, Physics 204 Fall Introduction Historic Remarks 2 Bose-Einstein Condensation Bose-Einstein Condensation The Condensation Temperature 3 The observation
More informationReevalua'on of Neutron Electric Dipole Moment with QCD Sum Rules
Reevalua'on of Neutron Electric Dipole Moment with QCD Sum Rules Natsumi Nagata Nagoya University Na1onal Taiwan University 5 November, 2012 J. Hisano, J. Y. Lee, N. Nagata, and Y. Shimizu, Phys. Rev.
More informationEs#ma#ons of Collec#ve Instabili#es for JLEIC
Es#ma#ons of Collec#ve Instabili#es for JLEIC Rui Li JLEIC Collabora#on Mee#ng 4-3-2016 Collec#ve Effects in JLEIC Electron Ring Ion Rings Electron Cooler Incoherent: LasleD tune shie, emidance growth
More informationSta$s$cal mechanics of hystere$c capillary phenomena: predic$ons of contact angle on rough surfaces and liquid reten$on in unsaturated porous media
Sta$s$cal mechanics of hystere$c capillary phenomena: predic$ons of contact angle on rough surfaces and liquid reten$on in unsaturated porous media Michel Louge h@p://grainflowresearch.mae.cornell.edu/
More informationGlobal properties of atomic nuclei
Global properties of atomic nuclei How to probe nuclear size? Electron Sca5ering from nuclei For low energies and under condi0ons where the electron does not penetrate the nucleus, the electron sca5ering
More informationChapter 7: Quantum Statistics
Part II: Applications - Bose-Einstein Condensation SDSMT, Physics 203 Fall Introduction Historic Remarks 2 Bose-Einstein Condensation Bose-Einstein Condensation The Condensation Temperature 3 The observation
More informationChapter 6 Electronic Structure of Atoms
Sec$on 7.1 Electromagne,c Radia,on Chapter 6 Electronic Structure of Atoms Sec$on 7.1 Electromagne,c Radia,on Different Colored Fireworks Copyright Cengage Learning. All rights reserved 2 Sec$on 7.1 Electromagne,c
More informationMolecular Dynamics. Molecules in motion
Molecular Dynamics Molecules in motion 1 Molecules in mo1on Molecules are not sta1c, but move all the 1me Source: h9p://en.wikipedia.org/wiki/kine1c_theory 2 Gasses, liquids and solids Gasses, liquids
More informationIntroduction to Particle Accelerators & CESR-C
Introduction to Particle Accelerators & CESR-C Michael Billing June 7, 2006 What Are the Uses for Particle Accelerators? Medical Accelerators Create isotopes tracers for Medical Diagnostics & Biological
More informationPHY492: Nuclear & Particle Physics. Lecture 4 Nature of the nuclear force. Reminder: Investigate
PHY49: Nuclear & Particle Physics Lecture 4 Nature of the nuclear force Reminder: Investigate www.nndc.bnl.gov Topics to be covered size and shape mass and binding energy charge distribution angular momentum
More informationNAPLES New Algorism for Polymeric Liquids Entangled and Strained. Yuichi Masubuchi ICR, Kyoto University
NAPLES New Algorism for Polymeric Liquids Entangled and Strained Yuichi Masubuchi ICR, Kyoto University The ul:mate goal of polymer rheology Predict viscoelas:c behaviors from Mw Mw/Mn LCB Blends Copolymers
More informationCollec&ve Effects & its Diagnos&cs part 2
The CERN Accelerator School Beam Instrumenta7on, 2-15 June 2018 Collec&ve Effects & its Diagnos&cs part 2 Vladimir Kornilov GSI Darmstadt, Germany Scho@ky signals with collec&ve effects 2 Scho@ky Signals
More informationActive galactic nuclei (AGNs): a brief observational tour
Active galactic nuclei (AGNs): a brief observational tour Yongquan Xue ( 薛永泉 ) Department of Astronomy University of Science and Technology of China http://staff.ustc.edu.cn/~xuey Early history, AGN ABCs,
More informationFrequency and time domain analysis of trapped modes in the CERN Proton Synchrotron
Frequency and time domain analysis of trapped modes in the CERN Proton Synchrotron Serena Persichelli CERN Impedance and collective effects BE-ABP-ICE Abstract The term trapped mode refers to a resonance
More informationBuilding Blocks for Quantum Computing Part IV. Design and Construction of the Trapped Ion Quantum Computer (TIQC)
Building Blocks for Quantum Computing Part IV Design and Construction of the Trapped Ion Quantum Computer (TIQC) CSC801 Seminar on Quantum Computing Spring 2018 1 Goal Is To Understand The Principles And
More informationElectronic Structure Calcula/ons: Density Func/onal Theory. and. Predic/ng Cataly/c Ac/vity
Electronic Structure Calcula/ons: Density Func/onal Theory and Predic/ng Cataly/c Ac/vity Review Examples of experiments that do not agree with classical physics: Photoelectric effect Photons and the quan/za/on
More information3. Synchrotrons. Synchrotron Basics
1 3. Synchrotrons Synchrotron Basics What you will learn about 2 Overview of a Synchrotron Source Losing & Replenishing Electrons Storage Ring and Magnetic Lattice Synchrotron Radiation Flux, Brilliance
More informationOctober 24, 2014 LB273 Prof. Vash9 Sawtelle. Today s Topics: Energy. Comic: Baldo, Carlos Castellanos
October 24, 2014 LB273 Prof. Vash9 Sawtelle Today s Topics: Energy Comic: Baldo, Carlos Castellanos Announcements Homework Ch 9 &10 due tonight midnight Exam 2 on Monday Exam correc9on problem due on Wednesday
More informationThe Sun as a Typical Star. Stellar Spectra. Stellar Spectroscopy
Stellar Spectroscopy Resolved observa7ons of the sun allow us to look at varia7ons across the surface, but we can only look at (almost all) other stars in integrated light. In the visible, we see the photosphere
More informationResearch Topics in Beam Physics Department
Introduction Research Topics in Beam Physics Department The physics of particle beams has been a broad and vibrant research field encompassing the study of charged particle beams and their interactions.
More informationNov 12, 2014 LB273 Prof. Vash6 Sawtelle. Today s Topics: SHM. h<ps:// v=6sas9n3omum&feature=youtu.be&t=16s
Nov 12, 2014 LB273 Prof. Vash6 Sawtelle Today s Topics: SHM h
More information$)ODW%HDP(OHFWURQ6RXUFHIRU/LQHDU&ROOLGHUV
$)ODW%HDP(OHFWURQ6RXUFHIRU/LQHDU&ROOLGHUV R. Brinkmann, Ya. Derbenev and K. Flöttmann, DESY April 1999 $EVWUDFW We discuss the possibility of generating a low-emittance flat (ε y
More informationBeam halo formation in high-intensity beams
Beam halo formation in high-intensity beams Alexei V. Fedotov,1,2 Brookhaven National Laboratory, Upton, NY 11973, USA Abstract Studies of beam halo became an unavoidable feature of high-intensity machines
More informationBunch trains. Linear stability theory; IntegrodifferenQal. eqns; Pseudospectra?
Translator. Amateur both in mathema'cs and in accelerator beam dynamics. (Sta's'cal mechanics, dynamical systems, condensed ma
More informationCalorimetry POGIL.notebook. December 06, 2012 POGIL ACTIVITY. Calorimetry Measurement of Heat Energy. Why?
POGIL ACTIVITY Calorimetry Measurement of Heat Energy Why? The amount of heat energy released or absorbed by a chemical or physical change can be measured using an instrument called a calorimeter. This
More informationCore- Collapse Supernova Neutrinos. Evan O Connor with Chris7an O8 INT 12-2A Workshop 1 July 2-6, 2012
Core- Collapse Supernova Neutrinos Evan O Connor with Chris7an O8 INT 12-2A Workshop 1 July 2-6, 2012 Overview NuLib! Mo7va7on Current Status Core- Collapse Supernovae: Models and Observable Signals: From
More informationIon traps. Trapping of charged particles in electromagnetic. Laser cooling, sympathetic cooling, optical clocks
Ion traps Trapping of charged particles in electromagnetic fields Dynamics of trapped ions Applications to nuclear physics and QED The Paul trap Laser cooling, sympathetic cooling, optical clocks Coulomb
More information