Monopoles The Mystery.

Slides:



Advertisements
Similar presentations
5th May 2010Fergus Wilson, RAL1 Experimental Particle Physics PHYS6011 Looking for Higgs and SUSY at the LHC or...what can you get for $10,000,000,000.
Advertisements

Black Holes and Particle Species Gia Dvali CERN Theory Division and New York University.
The Standard Model and Beyond [Secs 17.1 Dunlap].
Searching for Magnetic Monopoles
ATLAS Experiment at CERN. Why Build ATLAS? Before the LHC there was LEP (large electron positron collider) the experiments at LEP had observed the W and.
The Standard Model of the Atom. Reminders In-class Quiz #6 today (start or end of class?) Mallard-based reading quiz due prior to start of class on Thursday,
MAGNETIC MONOPOLES Andrey Shmakov Physics 129 Fall 2010 UC Berkeley.
Nailing Electroweak Physics (aka Higgs Hunting) with the Next Linear Collider Bob Wilson High Energy Physics Group CSU Physics Research Evening November.
Smashing the Standard Model: Physics at the CERN LHC
The Ideas of Unified Theories of Physics Tareq Ahmed Mokhiemer PHYS441 Student.
1 New Frontiers in Particle Physics Jeff Forshaw University of Manchester.
J.5.1State what is meant by deep inelastic scattering. J.5.2Analyze the results of deep inelastic scattering. J.5.3Describe what is meant by asymptotic.
A review on magnetic monopoles What is a RPP review good for ? Why are monopoles important ? What is already in the RPP ? Why is a monopole review desirable.
Particle Physics at the Energy Frontier Tevatron → LHC & The Very Early Universe Tony LissAir Force Institute of TechnologyApril 10, 2008.
Discovery of the Higgs Boson Gavin Lawes Department of Physics and Astronomy.
ROY, D. (2011). Why Large Hadron Collider?. Pramana: Journal Of Physics, 76(5), doi: /s
Particle Physics J4 Leptons and the standard model.
The Higgs Boson: without the maths and jargon David Hall Graduate Seminar Series St Catherine’s College MCR 11 th May 2011.
My Chapter 30 Lecture.
August 22, 2002UCI Quarknet The Higgs Particle Sarah D. Johnson University of La Verne August 22, 2002.
School of Arts & Sciences Dean’s Coffee Presentation SUNY Institute of Technology, February 4, 2005 High Energy Physics: An Overview of Objectives, Challenges.
Higgs Boson-The God’s Particle & The mystery of mass Higgs Boson-The God’s Particle & The mystery of mass Dr.S.Sanyasi Raju Reader & H.O.D. of Physics.
From Luigi DiLella, Summer Student Program
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 30: Particle Physics Fundamental.
LOGO B. I. Stepanov Institute of Physics National Academy of Sciences of Belarus.
Search for a Z′ boson in the dimuon channel in p-p collisions at √s = 7TeV with CMS experiment at the Large Hadron Collider Search for a Z′ boson in the.
Wave-Particle Duality - the Principle of Complementarity The principle of complementarity states that both the wave and particle aspects of light are fundamental.
SubAtomic Physics & Astrophysics Intimate Connexion between Very Large and Very Small.
22 December 2006Masters Defense Texas A&M University1 Adam Aurisano In Collaboration with Richard Arnowitt, Bhaskar Dutta, Teruki Kamon, Nikolay Kolev*,
The Higgs Boson Observation (probably) Not just another fundamental particle… July 27, 2012Purdue QuarkNet Summer Workshop1 Matthew Jones Purdue University.
Searching for New Matter with the D0 Experiment Todd Adams Department of Physics Florida State University September 19, 2004.
Andrea Linville Office of Science, SULI Program 2009 Stanford Linear Accelerator August 13, 2009.
ELECTROWEAK UNIFICATION Ryan Clark, Cong Nguyen, Robert Kruse and Blake Watson PHYS-3313, Fall 2013 University of Texas Arlington December 2, 2013.
The Standard Model of the elementary particles and their interactions
1 Particle Physics, The Mysteries of the Universe, and The LHC Nhan Tran Johns Hopkins University.
The Standard Model T. Kawamoto The University of Tokyo FAPPS08 Les Houches September 2008.
IoP Masterclass The Physics of Flavour at the Large Hadron Collider Tim Gershon University of Warwick March 30 th 2011.
IoP Masterclass B PHYSICS Tim Gershon University of Warwick March 18 th 2009.
1 Lecture-06 Baryogenesis Ping He ITP.CAS.CN
REVISITING THE GOD PARTICLE …… Bangabasi College, Kolkata
Fundamental Particles, Fundamental Questions
Alessandro Bettini Introduction to Elementary Particle Physics
Elementary Particle Physics
HOW TO TELL DIFFERENCE OF MAJORANA/DIRAC NEUTRINOS
Study of Kaon-pion interaction
5. Wave-Particle Duality - the Principle of Complementarity
Yu. Kulchitsky, N. Rusakovich: JINR, Dubna
The Physics of Neutrinos
Elastic Scattering in Electromagnetism
The Standard Model of the Atom
ATLAS Collaboration 3000 Physicists including 1000 students.
Searching for Magnetic Monopoles
HCP: Particle Physics Module, Lecture 3
Elementary particles Spring 2005, Physics /24/2018 Lecture XXV.
The Four Fundamental Forces
From Last Time… Discussed the weak interaction
HCP: Particle Physics Module, Lecture 2
Radiation Shield Design by UA
SPH4U Elementary Particles.
Section VII - QCD.
THE GOD PARTICLE 1 Shashwat Mandal & Christian Bach 5
CMS Masterclass 2017.
Frontiers of fundamental physics
From Last Time… Discussed the weak interaction
G. A. Krafft Jefferson Lab Old Dominion University Lecture 1
5. Wave-Particle Duality - the Principle of Complementarity
Composite Weak Bosons LHC.
What do we hope to understand?
The Four Fundamental Forces
Presentation transcript:

Monopoles The Mystery

At the beginning there was Maxwell... Vacuum Symmetry under electromagnetic duality

MAXWELL Matter (Source) Duality Symmetry is explicitly Broken In order to restore symmetry is necessary to introduce Magnetic charge(MONOPOLE) and the magnetic current

With this transformation Duality Symmetry is restored in Classical Electromagnetism The Price to be pay is the introduction of MONOPOLE

The following step, Dirac... (1931-1934) Monopole with Quatum Mechanics Schrodinger equation for a particule moving in the electromagnetic fields Invariance under Gauge Transformation

Magnetic Monopole ₊g ∞ Singularity

Big Bang predicts 1000 monopoles per nucleon THE SEARCH Monopoles of the usual Grand Unification have masses of the order m > Could only be produced in the first instants of the Universe and only searchable in cosmic radiation Big Bang predicts 1000 monopoles per nucleon (disagreement with observation = no one observed) The paradox is solved by Inflationary Cosmological Models, that greatily reduced the monopole density

Monopole Searches in Accelarators No Dirac prediction for monopole mass “Lower Bound” using classical electron radius by analogy: Assuming:

e gβ Going from lepton production we replace Two photon s=1/2 Search of Monopole in Accelerators Direct Searches ⇒ Monopole production as free particles Going from lepton production we replace Two photon s=1/2 e gβ Drell-Yan

The experimental limits on monopole mass The most recent limits on the monopole mass HERA e+ p – collisions |n|=1,2,3,6 Tevatron p p – collisions Experiment E-882 (Al) |n|=1, M > 285 GeV (Al) |n|=2, M > 355 GeV (Be) |n|=3, M > 325 GeV (Be) |n|=6, M > 420 GeV LEP 2 e+ e- – collisions (Al) M > 140 GeV 45 ≤ M < 102 GeV

MONOPOLE and EXOTICS DETECTOR At the LCH MoEDAL

MONOPOLIUM DIRAC DIXIT: (1934) BOUND STATE MONOPOLE ANTIMONOPOLE “…THE ATTRACTIVE FORCE BETWEEN TWO MAGNETIC POLES IS 4692 TIME THAT BETWEEN THE ELECTRON AND THE PROTON. THIS VERY LARGE FORCE MAY PERHAPS ACCOUNT FOR WHY THE MONOPOLES HAVE NEVER BEEN SEPARATED …” MONOPOLIUM

Monopolium Dynamics Monopolium production from photon fusion Nonrelativistic bound state Attributed to beam width aprox. 10 G eV

Monopolium production and Decay Monopolium Decay Monopolium Vertex Monopolium production and Decay

Analysis of p-p scattering Processes above the monopole Threshold M M M

Evaluation Energy Diferential Cross Section Elastic Scatering Elastic photon spectrum Elementary photon-photon cross section = C.M energy pp system = C.M energy of the photons This procedure can be generalized easily to semi-elstic and inelastic case

Cross section monopole antimonopole annhilation Compararison Higgs and monopole antimonopole decay

Fixed binding energy 100GeV

Monopolium Cross Section Total Semi-elastic Elastic Inelastic

CROSS - SECTION

Concluding Remarks Dirac felt that he ¨would be surprised If Nature had made no use for it. It, being the Magnetic Monopole¨. Ed Witten once asserted in his Loeb Lecture at Harvard, ¨almost all theoretical physicists believe in the existence of magnetic monopoles, or at least hope that is one¨. Joshep Polchinsky, a string – theorist, described the existence of monopoles as ¨one of the safest bets that one can make about physics not yet seen¨ and that ¨their existence seems inevitable in any framework that explains the quantization of electric charge. Of course their mass scale and abundance are highly uncertain,… ¨

11/23/10 CONCLUSIONS Monopoles are hypothetical, but predicted by the most major theoretical models No confirmed repeatable monopole events have been recorded Strong lower limits on energy probably place Dirac monopoles on the reach of colliders Strong upper limits on cosmic ray flux Maybe finding reasons to their inexistence is more interesting than finding them?