Physics Beyond the Standard Model

Slides:



Advertisements
Similar presentations
Bruce Kennedy, RAL PPD Particle Physics 2 Bruce Kennedy RAL PPD.
Advertisements

Black Holes and Particle Species Gia Dvali CERN Theory Division and New York University.
The Standard Model and Beyond [Secs 17.1 Dunlap].
STRING THEORY: CHALLENGES AND PROSPECTS John H. Schwarz October 2008.
Beyond the SM: SUSY and ToE A romantic dream for an unified description of the universe? Part III.
Higgs Boson Mass In Gauge-Mediated Supersymmetry Breaking Abdelhamid Albaid In collaboration with Prof. K. S. Babu Spring 2012 Physics Seminar Wichita.
Grand Unified Theory, Running Coupling Constants and the Story of our Universe These next theories are in a less rigorous state and we shall talk about.
Nuclear Physics UConn Mentor Connection Mariel Tader.
AAAS 2001 San Francisco1 Supersymmetry The Coming Revolutions in Particle Physics Hitoshi Murayama (UC Berkeley)
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE  5-Feb pm Physics LRA Dr M Burleigh Intro lecture  9-Feb-04.
Richard Howl The Minimal Exceptional Supersymmetric Standard Model University of Southampton UK BSM 2007.
27 km ring Large Hadron Collider went online on Sept
Fermion Masses and Unification Steve King University of Southampton.
Nailing Electroweak Physics (aka Higgs Hunting) with the Next Linear Collider Bob Wilson High Energy Physics Group CSU Physics Research Evening November.
The Ideas of Unified Theories of Physics Tareq Ahmed Mokhiemer PHYS441 Student.
Schlüsselexperimente der Elementarteilchenphysik:.
Chapter 43 Elementary Particles
Modern Physics LECTURE II.
Lecture 3: The Standard Model
8/5/2002Ulrich Heintz - Quarknet Particle Physics what do we know? Ulrich Heintz Boston University.
Particle Physics From Strings To Stars. Introduction  What is Particle Physics?  Large Hadron Collider (LHC)  Current Experiments – ALICE – ATLAS –
Elementary particles atom Hadrons Leptons Baryons Mesons Nucleons
The Pursuit of Unification: Fulfilling Einstein’s Dream N. Seiberg Institute for Advanced Study 2004.
The Big Bang, the LHC and the Higgs Boson Dr Cormac O’ Raifeartaigh (WIT)
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.
CERN, 21 February 2001 Egil Lillestøl, CERN & Univ. of Bergen Recorded at
Particle Physics at the Energy Frontier Tevatron → LHC & The Very Early Universe Tony LissAir Force Institute of TechnologyApril 10, 2008.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 26-Jan pm LRB Intro lecture 28-Jan pm LRBProblem solving.
Particle Physics Chris Parkes 5 th Handout Electroweak Theory 1.Divergences: cancellation requires.
Strings: Theory of Everything, Something, or Nothing? Robert N. Oerter.
Fermion Masses and Unification Steve King University of Southampton.
ROY, D. (2011). Why Large Hadron Collider?. Pramana: Journal Of Physics, 76(5), doi: /s
My Chapter 30 Lecture.
Center for theoretical Physics at BUE
The Dark Side of the Universe What is dark matter? Who cares?
August 22, 2002UCI Quarknet The Higgs Particle Sarah D. Johnson University of La Verne August 22, 2002.
P Spring 2003 L12Richard Kass The properties of the Z 0 For about ten years the Z 0 was studied in great detail at two accelerator complexes: LEP.
Standard Model A Brief Description by Shahnoor Habib.
From Luigi DiLella, Summer Student Program
Quarks, Leptons, Bosons, the LHC and all that. Tony Liss OLLI Lecture September 23, 2008.
Wednesday, Apr. 23, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #24 Wednesday, Apr. 23, 2003 Dr. Jae Yu Issues with SM picture Introduction.
Elementary particles and their forces -- how can we understand them and what do they imply about our early universe? Barbara Hale Physics Department Missouri.
String/M Theory – what is it? Branes and brane world Holography The Landscape Nick Evans Strong Force Origins Superstrings Ten & eleven dimensions.
Particles and Strings Nick Evans “The search for a fundamental theory of the building blocks of nature and their interactions” University of Southampton.
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 30: Particle Physics Fundamental.
1 Supersymmetry Yasuhiro Okada (KEK) January 14, 2005, at KEK.
INVASIONS IN PARTICLE PHYSICS Compton Lectures Autumn 2001 Lecture 8 Dec
© John Parkinson 1 e+e+ e-e- ANNIHILATION © John Parkinson 2 Atom 1x m n n n n Nucleus 1x m U Quarks 1x m U D ? ? ?
Modern Physics. Reinventing Gravity  Einstein’s Theory of Special Relativity  Theorizes the space time fabric.  Describes why matter interacts.  The.
The Higgs Boson Observation (probably) Not just another fundamental particle… July 27, 2012Purdue QuarkNet Summer Workshop1 Matthew Jones Purdue University.
STANDARD MODEL class of “High Energy Physics Phenomenology” Mikhail Yurov Kyungpook National University November 15 th.
CERN, 8 February, 2001 Egil Lillestøl, CERN & Univ. of Bergen Lectures recorded at :
H. Quarks – “the building blocks of the Universe” The number of quarks increased with discoveries of new particles and have reached 6 For unknown reasons.
Compelling Scientific Questions The International Linear Collider will answer key questions about matter, energy, space and time We now sample some of.
The Search For Supersymmetry Liam Malone and Matthew French.
ELECTROWEAK UNIFICATION Ryan Clark, Cong Nguyen, Robert Kruse and Blake Watson PHYS-3313, Fall 2013 University of Texas Arlington December 2, 2013.
Standard Model - Standard Model prediction (postulated that neutrinos are massless, consistent with observation that individual lepton flavors seemed to.
Jonathan Nistor Purdue University 1.  A symmetry relating elementary particles together in pairs whose respective spins differ by half a unit  superpartners.
Quantum quivering of gravity The search for the unified field theory.
1 The Standard Model of Particle Physics Owen Long U. C. Riverside March 1, 2014.
More on the Standard Model Particles from quarks Particle interactions Particle decays More conservation laws Quark confinement Spin.
Physics 222 UCSD/225b UCSB Lecture 12 Chapter 15: The Standard Model of EWK Interactions A large part of today’s lecture is review of what we have already.
Grand Unified Theory, Running Coupling Constants and the Story of our Universe These next theories are in a less rigorous state and we shall talk about.
HCP: Particle Physics Module, Lecture 3
The symmetry of interactions
Particle Physics what do we know?
The MESSM The Minimal Exceptional Supersymmetric Standard Model
What do we hope to understand?
Particle Physics and The Standard Model
Presentation transcript:

Physics Beyond the Standard Model Summary by Dennis Silverman Physics and Astronomy UC Irvine

Where Does Mass Come From? The electroweak “gauge” theory only has conserved currents for its weak charges if the W’s and Z are massless, like the photon is. It also helps if quarks and leptons are massless in the Energy. To maintain this, but yet have physical masses, we fill the vacuum with some sludge. A particle’s mass is then proportional to the amount each particle couples to this sludge. The sludge is the everywhere constant vacuum value of the neutral Higgs.

The Higgs Fields in the SM Three extra Higgs fields, H+, H-, anti-H0 make up the extra component of the W and Z spins needed to make them massive. The W’s have a mass of 81 GeV, and the Z of 90 GeV. The H0 has a constant vacuum density, and can also make a physical particle.

How to Find the Higgs The Higgs vacuum value is uniform, neutral, appears the same at all velocities, and undetectable – except for the fact that it gives mass to everything. A particle’s mass is proportional to its coupling to the Higgs and therefore to its vacuum density. The excitations of the Higgs is a real particle, predicted to be at about 115-130 GeV. This should show up in the LHC in some rare decays. It would have shown up at the Fermilab Tevatron, except that the intensity has not met expectations.

Increasingly General Theories Grand Unified Theories of electroweak and strong interactions Supersymmetry Superstring Theories – 10 dimensions with gravity Superstring Unification to M Theory

Running Coupling Constants Charged particles have virtual quantum allowed clouds around them of photons and electron-positron pairs. Colored particles have virtual gluons and q-anti-q pairs. So the total coupling at long distance or “charge”, is different from the coupling at short distance, where the the cloud is penetrated. Electromagnetic coupling 1 = e2/c increases with energy from 1/137 to 1/40 at 1017 GeV Unification Scale Strong coupling 3 = g2/c decreases from ~1 to 1/40 Weak coupling to W’s is 2. So couplings come together at unification scale

Running Gluonic Coupling 3 = (g3)2 /c

Running Couplings

Fundamental Particles for Unification Unification means that at a GUT scale, where masses can be ignored, all fundamental particles appear in the same multiplet. This allows their charges to be the same or given fractions of each other, and accounts for the proton and electron charge being equal. The particles from the SM to include for the first generation are the 16 (left handed): ur ug ub dr dg db anti-(ur ug ub dr dg db) e e- anti-e e+ Recently, neutrino oscillations and mass were found, adding the anti-e. In the GUT, there are vector bosons that take fundamental particles into another in the multiplet.

Sequence of GUTS Standard Model of electroweak doublets for quarks and leptons plus photon (SU(2)xU(1)) and three colors (xSU(3)). It has , W±, Z, and 8 gluons as bosons. Combine 3 colors and electroweak doublet (SU(5)) – ruled out as causes proton decay at level not seen – has 5 + 10 fundamental particles. It has 24 bosons. Add extra neutrino mode for massive neutrinos – 16 fundamental (SO(10)) There are 45 gauge bosons in SO(10). 27 fundamentals (E6), including singlet quarks and neutrinos. E7, E8 (heterotic string) Three generations of each fundamental multiplet

A Bit of History of Unification Electricity unified with magnetism (M. Faraday and J. C. Maxwell). Relativity and General Relativity (A. Einstein). Quantum Mechanics (Planck, Bohr, Schrodinger and Heisenberg). Relativistic quantum mechanics (P. Dirac). Quantum Electrodynamics (R. Feynman, Tomonaga, Schwinger). Quarks and Quantum Chromodynamics (Nemann, M. Gell-Mann and G. Zweig). Unification of Electromagnetism with Weak Interactions to form Electroweak theory (S. Weinberg, A. Salam). Grand Unified Theories Supersymmetry Superstring Theory of Everything including gravity.

Proton Decay In a GUT there are X and Y gauge bosons that can transform a quark into an antiquark, and a quark into a lepton, since they are in the same multiplet. This allow protons in quarks to decay into a lighter pi or K meson and a lepton. Don’t worry, the lower limit on the lifetime is 1034 years, far longer than the age of the universe of 1010 years. It takes a detector the size of Super-K to see a few proton decays a year in these theories.

Proton Decay dr dr p0 anti-danti-r ug P Xanti-r ub e+

Particle Spin Orbital angular momentum is quantized to integer units of Planck’s constant over 2:  = h/2. Quarks and leptons have half a unit of angular momentum as spin, or are spin 1/2 particles, also called fermions. Photons and W’s and Z are spin 1 particles, also called bosons. Gravitons have spin 2, and are bosons.

Particle Supersymmetry In a Grand Unified Theory, all quarks and leptons are in a generation are united into one family. The GUT gauge bosons transform one quark or lepton to another, such a gluon changing one color quark into another. A grander symmetry would be to transform all gauge bosons to fermions with the same charges, and vice versa. Thus for every spin ½ fermion there would be a spin 0 boson with the same charges and flavor, and to every gauge boson, there would be a like charged and coupled spin ½ fermion. These look-alikes, except for spin, are called sparticles.

Conserved Supersymmetry If supersymmetryness is conserved, sparticles can only be created or destroyed in pairs Sparticles would then decay to the ordinary particles plus another sparticle, until they reach the lightest supersymmetric particle (LSP) The LSP should be neutral and is a leading dark matter candidate They should have masses about 1 TeV They should be produced in pairs at the LHC in 2007 The Next Linear Collider (NLC) will be needed to map out the sparticles and Higgs interactions in detail.

Sparticle Names Thus with quarks there would be spin 0 squarks Leptons would have spin 0 sleptons (selectron and sneutrino) The photon also would have a spin ½ photino The W’s and Z’s would have spin ½ Winos and Zinos (after Wess and Zumino) Spin 0 Higgs would have spin ½ Higgsinos In a supergravity theory, spin 2 gravitons have spin 3/2 gravitino look-alikes.

Why Supersymmetry (SUSY)? It’s believers think it is a beautiful symmetry between fermions and bosons, and should be a part of nature. If the sparticles are at about 1 TeV, then the running coupling constants actually do meet at a GUT scale of 1017 GeV. GUT scale (mass) Higgs’s would normally couple to the light SM Higgs and bring its mass up to the GUT scale. Adding sparticles to particles cancel this coupling to leave the SM Higgs light, solving the so-called Heirarchy problem. String Theory requires SUSY, again for similar cancellations.

Minimal SUSY Standard Model The MSSM has two Higgs doublets, as opposed to the one in the standard model. The doublets also have distinct anti-Higgs. Thus there are 8 Higgs particles. Three are “eaten” to make the W± and Z massive. One makes the neutral mass generating Higgs. Four more are observable, of which two are charged.

Evolution of Gauge Couplings (reciprocals) Standard Model Supersymmetry

Meeting of the Running Couplings (reciprocals) in MSSM

What is String Theory? It is the theory that elementary particles are really strings with tension, that obey relativity and quantum mechanics. By dispersing the particle away from a point, it avoids infinities in the treatment of gravity or gravitons by pointlike particles. The string size is close to the Planck size of 10-32 cm, which is the smallest size where gravity becomes strong. To avoid “anomaly” infinities requires supersymmetry and 10 dimensions (1 time and 9 space dimensions). String theory then provides a quantum theory of gravity. Andre Neveu, John Schwarz, Michael Green and Pierre Ramond were founders.

Pictures of John Schwarz and Ed Witten

Types of Superstring Theories There are five superstring theories. There is one open superstring theory with left (L) moving waves (SO(32)). There are two closed superstring theories: Type IIA: L-R parity symmetric Type IIB: L only, parity violating There are two heterotic string theories of a product of a string theory in 26 dim (with L moving waves) x a superstring in 10 dim (with R moving waves). (SO(32)) and (E8 x E8).

Unification of Superstring Theories Recently, in the second string revolution, it was discovered that there are transformations between all five superstring theories. (Ed Witten) This means they are all views of a larger theory which is not well understood, but is called M theory. It may be in 11 dimensions. For further information, see http://superstringtheory.com/, run by Patricia Schwarz, John Schwarz’s wife. “The Elegant Universe” by Brian Greene, http://www.pbs.org/wgbh/nova/elegant

Towards Verification of Superstring Theory Since superstring theory included the three unified forces of GUTS and gravity, it has been called the Theory of Everything. It has not been possible to “solve” superstring theory to find a unique physical model. There are a half-million ways to topologically “compactify” the extra six dimensions to very short distances, and leave the four dimensional world that we live in. So many GUTS and breakup paths of GUTS to the SM are still possible

Verification of Superstring Theory The masses of sparticles are not well predicted. If they are in the TeV range, they will appear in the LHC. Once they are found, the NLC e+ e- collider will more precisely determine their properties. The convergence of the running coupling strengths at a GUT scale is more successful with SUSY particles than in the SM. If SUSY is found, it will be considered a success of string theory. If not found, it could spell its demise. The lightest neutral SUSY particle (LSP) could be dark matter, and there are experiments to directly detect them, but they will take a while to reach large enough scale.

How do strings scatter? Via the “pants” diagram, where two strings merge to one, and then go back to two.

Speculative Models of Extra Dimensions Large Extra Dimensions and Branes Early Unification with a Strong Gravity

Brane Solutions String Theories have membrane solutions The most used is that all our 4 dimensional world is a membrane in the 10 dimensional world. Open string ends are attached to the membrane. Quarks, leptons and interacting bosons for strong and electroweak particles are confined to the brane. But gravitons as closed strings can leave the brane and spread out in the extra dimensions.

Brane with attached string and graviton in extra dimension

Large Extra Dimension Models By experimental limits, extra dimensions could still be as large as 0.1 millimeter, and this will be tested by gravity, which behaves as F ~ M1 M2/ rn+2 for n extra dimensions, at r < R. In these, gravity could become strong at 1 TeV and unify with the other forces there. (Nima Arkani-Hamed, Dimopoulos and Dvali) The extra dimension could be curled up with 1 TeV excitations, or at the String or Planck Scale. The former would show up in experiment at Fermilab or the LHC as invisible missing energy disappearing into the extra dimensions in excitations there, or as one micro black hole a second being produced.

Plane Extra Dimension The extra dimension could be between two flat branes, one of which is physical, and one of which has gravity (unphysical brane). The gravity field exponentially decreases from the unphysical to the physical brane. Thus gravity appears weak to us on the physical brane, but is strong on the unphysical brane. Called the Randall-Sundrum model. The extra dimension models so far do not give GUT theories, spoiling the supersymmetry triumph of explaining the convergence of coupling constants at the GUT scale.

Relevance of Particle Physics We are closer to accounting for some leftover matter, possibly requiring three generations of quarks and leptons. We may someday account for inflation and dark matter (SUSY?) and dark energy. We understand how the Sun shines through weak interactions. We understand how color forces and quarks form nucleons. We may soon find how a Higgs gives mass to everything”. There may be Grand Unification to keep charges of everything the same and allow particle changing interactions. We may have found a way to have gravity that is consistent with quantum mechanics.