Added Dimensions. Efforts to unify quantum physics and general relativity
|
|
- Eric Thompson
- 5 years ago
- Views:
Transcription
1 Added Dimensions Efforts to unify quantum physics and general relativity - Why are there only 4 extended dimensions? - Symmetry, elementary particles and the Standard Model - Supersymmetry - Kaluza-Klein theory: 5 dimensions - String theory: 10 dimensions - M-theory: 11 dimensions, branes and the multiverse
2 Why are there only 4 dimensions? (3 space and 1 time) - Gravity and electromagnetism would not have an inversesquare law if there were more than 3 space dimensions (first discovered by Immanuel Kant in the 1700 s) - Planetary orbits would not remain stable in more than 3 space dimensions (first discovered by Paul Ehrenfest in 1920) - Electrons would not remain stably in orbitals surrounding atomic nuclei in more than 3 space dimensions (discovered by F. R. Tangherlini in 1963) - Wave impulses would become distorted if there were a number of space dimensions other than 1 or 3 (Ehrenfest) - Protons and electrons would be unstable if there were more than 1 time dimension (Max Tegmark, 1997)
3 - When the number of dimensions is too great or too small, the equations of physics become unpredictable - When the number is too small, observers are not possible - In more than 3 space or time dimensions, atoms are unstable
4 Elementary particles - Fundamental constituents of matter and energy forces - Described by quantum field theory - Matter is made of quarks and leptons (collectively called fermions) There are three generations or families of matter - Energy forces are transmitted by bosons - Particles have anti-particles with opposite electric charges
5
6 Elementary Particles MATTER ENERGY (FORCE CARRIERS) - Quarks - Bosons Up (u), Down (d) Photon (g) Charmed (c), Strange (s) Gluon (g) (8 flavors) Top (t), Bottom (b) W Z - Leptons ( Higgs) Electron (e) ( Graviton) Muon (m) Tau (t) Electron neutrino (n e ) Muon neutrino (n m ) Tau neutrino (n t )
7
8 Particle interactions - Feynman diagrams world lines of particles - Example: two electrons exchanging a photon e - e - time g space - Particles intersect at single points in spacetime
9 Large Hadron Collider at CERN
10
11 Example particle collision in a detector
12 Example particle collision in a detector
13
14 Fermions matter particles - Fermions make up the atoms that make up the matter we experience in our everyday lives - Quarks: Make up atomic nuclei Massive: all but first generation (up and down quark) are short-lived and unstable - Leptons: Orbit atomic nuclei (electrons) and carry weak charge (neutrinos) Very low mass
15 Fermions matter particles
16
17 Quarks and gluons the strong force - There are three strong force charges red, blue and green Each of the quarks in each generation of particles is available with each type of charge - Each charge has an anti-charge (anti-red, anti-blue, anti-green) - Combinations of quarks must be colorless - Gluons carry the charge of the strong interaction, unlike photons which do not carry the charge of the electromagnetic interaction - Leads to the consequence of asymptotic freedom As quarks get closer together the force gets weaker As they get farther apart the force gets stronger Means quarks can never be observed in isolation
18 Computer simulation of gluon flux tubes joining quarks within a baryon
19 The weak force - Changes one particle into another! - Muon and tau can turn into neutrinos - Quarks can turn into other types of quarks - Responsible for nuclear fusion in the sun - Responsible for beta decay in radioactivity - The neutrino interacts only via the weak force (and gravity) This is why it can pass through all types of matter without being stopped
20 Carriers of the weak force - For the weak force, there are three force carrier particles: W + W - Z 0 These are electrically charged in addition to carrying the weak force This one is electrically neutral - These particles are very massive almost as massive as the top quark (the most massive particle known) - This means the weak force is very short range
21 Relative strengths of forces Strength for 2 quarks at m Strength for 2 quarks at 3x10-17 m Gravity Weak Electromagnetic Strong Why do the forces have the strengths they do? - In particular, why is gravity so much weaker than the others? It s a mystery!
22 Summary of forces and carrier particles Interaction Carriers Act On Particles Gravitation (Graviton?) All (infinite) Weak force W +, W -, Z 0 Electrons, (10-16 cm) muons, taus, quarks, neutrinos Electromagnetic Photon Electrons, Force muons, taus, (infinite) quarks, W +, W - Strong force Gluons (8) Quarks, gluons (10-13 cm)
23 Some quantum numbers of particles Each particle has a characteristic - Charge Electromagnetic force charge: + / 0 / - Weak force charge Color charge (strong nuclear force): quarks/gluons only - Spin (angular momentum) Fermions: Integer spins (0, 1, ) Bosons: Half-integer spins (1/2, 3/2, ) There are actually many more quantum numbers involved in defining the behavior of particles Each quantum number is a conserved quantity: the total amount of it does not change in particle interactions
24 The Standard Model - Based on Quantum Field Theory Fields are quantized into particles (e.g. EM field -> photons) Consistent with Special Relativity (Lorentz invariance) Renormalizable does not give infinite answers - Explains observed behavior of all known particles; predicted new particles that were later observed - Unifies electromagnetism, weak force at high energies (electroweak unification) - Suggests possibility of unifying strong force with electroweak force at even higher energies (grand unified theory or GUT) - Does not include gravity or General Relativity
25 The unification of forces in physics
26 The unification of forces in physics? - The goal of unification theories (like string theory) is to explain the?
27 Symmetries in the Standard Model - Particle / anti-particle symmetry - Symmetry of structure of 3 generations of matter particles - Conservation laws Charge Mass/energy Spin (angular momentum) and other quantum numbers Parity (physics is the same for mirror images) True for electromagnetism, gravity and strong forces; Not true for weak force! - Gauge symmetry: invariance under local transformations of the spacetime system, due to the presence of gauge fields
28 Chen Ning Yang Chinese-American physicist - Nobel Prize, With Tsung-Dao Lee, proposed that parity is violated by the weak force; experimentally verified by C.S. Wu - With Robert Mills, developed modern gauge symmetry theory (non-abelian gauge theory, or Yang-Mills theory) - Married a 28-year-old graduate student at age 82 in 2005
29 Gauge Symmetry
30 Electromagnetic Gauge Field U(1) Symmetry
31 Gauge symmetry - A field has a magnitude and direction at every point in spacetime: this combination is the field s potential - Each circle represents the potential at a single point in spacetime a. Potential Magnitude value of = a radius field becomes of circle varied at different points in spacetime Direction = where the arrow in the circle is pointing b. Variation - Suppose of an value initially of potential symmetric is compensated static field: by gauge field (wavy lines) time
32 Gauge symmetry a. Potential value of field becomes varied at different points in spacetime b. Variation of value of potential is compensated by gauge field (wavy lines) c. Original symmetric field configuration is restored
33
34 Gauge symmetry a. Potential value of a field becomes varied at different points in spacetime b. Variation of value of potential is compensated by gauge field (wavy lines) c. Original symmetric field configuration is restored
35 Gauge symmetry a. Potential value of a field becomes varied at different points in spacetime b. Variation of value of potential is compensated by gauge field (wavy lines) c. Original symmetric field configuration is restored
36 Internal symmetry space for gauge field space time world line of particle
37 Internal symmetry space for gauge field internal symmetry space (field potential magnitude) fiber bundle space time world line of particle
38 Path through internal symmetry space with no gauge field present internal symmetry space (field potential magnitude) space fiber bundle path of field magnitude through internal symmetry space time world line of particle
39 Path through internal symmetry space with internal symmetry space (field potential magnitude) space gauge field present fiber bundle path of field magnitude through internal symmetry space time world line of particle
40 Gauge symmetry - Electromagnetism: U(1) Unitary symmetry group with one degree of freedom Represented by rotations around a circle Gauge boson is the photon - Weak force: SU(2) Special unitary symmetry group with two degrees of freedom Represented by rotations on the surface of a sphere Gauge bosons are the W and Z particles - Strong force: SU(3) Special unitary symmetry group with three degrees of freedom Represented by rotations in a complex hyperspace Gauge bosons are the eight gluons
41 Symmetry Breaking - At high energies (e.g. in the Big Bang) all forces are the same (symmetrical) - At lower energies the forces become differentiated (the symmetry breaks) - Similar to the way hot steam has no directionality (it is symmetrical in all directions), but frozen ice crystals have specific directionality
42 Symmetry breaking of forces during Time from Big Bang (seconds) Big Bang
43 Evolution of the universe
44 Masses of elementary particles
45 Why do the particles have the masses that they do? (the hierarchy problem ) - It s a mystery! By gauge theory alone, particles should have no mass at all - The hierarchy problem : why are the particle masses so much less than the force unification energy? - In the Standard Model, particles get their masses from interaction with the Higgs field (whose gauge boson is the Higgs particle recently detected at CERN LHC) - But the model does not predict the specific sizes of particle masses (except for the W and Z bosons)
46 Higgs field vs. Electromagnetic field - Minimum Electromagnetic field potential is at zero energy
47 Higgs field vs. Electromagnetic field - Minimum Higgs field potential is not at zero energy, therefore symmetry breaks and particle gets positive mass
48 The former prime minister of England walks into a cocktail party
49 The former prime minister of England walks into a cocktail party
50 Strength Strength Supersymmetry one solution to the hierarchy problem Strong Strong Weak Weak Electromagnetic Electromagnetic Energy Energy - SM = Standard Model; MSSM = Minimal Supersymmetric Standard Model - Under MSSM the electromagnetic, weak and strong forces unify more precisely at high energy than under the normal Standard Model
51 Bruno Zumino - Italian-American physicist at U. of California - Berkeley: Dirac Medal, With Julius Wess, developed theory of supersymmetry in 1974 (independently developed by Golfand and Likhtman and by Volkov and Akulov in Russia) -The Minimal Supersymmetric Standard Model (MSSM) was first proposed in 1981 by Howard Georgi and Savas Dimopolous
52 Supersymmetry - Basic to String and M Theory
53 What Is Supersymmetry? - Superpartner particles have higher masses than ordinary particles (corresponding to their higher energies) May be detectible by LHC at CERN Supersymmetry breaks at much lower energy than force unification (solves hierarchy problem) - Superpartner particles spins are ½ less than those of their ordinary partner particles
54 History of unification theories in physics
55 Problems in unifying quantum field theory and general relativity - To quantize the gravitational field involves quantizing spacetime itself - The quantum particle of this field is the graviton, a massless spin-2 boson All other particles either have spin ½ (fermions) or spin 1 (bosons) No consistent gauge theory exists for spin-2 particles - The resulting theory is not renormalizable Particle interaction sites are single points in spacetime Single points have zero size Gravitational fields at single points can t be calculated Equations produce infinite results - singularities
56 Theodor Kaluza German mathematician - Spoke 17 languages (favorite was Arabic) - Developed unified theory of gravity and electromagnetism in 1919 by generalizing Einstein s theory of general relativity to 5 dimensions - Sent his results to Einstein, who sat on them for two years before finally encouraging Kaluza to publish in 1921
57 Oskar Klein Son of chief rabbi of Stockholm; physicist at University of Michigan and Stockholm University - Independently discovered 5-D unification of gravitation and electromagnetism in Proposed that the 5 th dimension is curled up ( compactified ) into a sub-nanoscopic circle (r=10-34 m), which is why it is not observed in nature
58 - What we see: Compactification
59 - What we see: Compactification - What an ant sees: Compact dimension
60 Kaluza-Klein space (1 compactified dimension) - Compactified dimension exists at all points in space - It is shown only at grid line intersections for clarity
61 Kaluza-Klein theory - In the 5-D space there is only one force: Gravity - In the 4-D space of our experience this becomes three forces: Gravity (same as Einstein s general relativity) Electromagnetism (electric charge corresponds to the component of the momentum of particles in the 5 th dimension, while electric force corresponds to the component of the gravitational force in the 5 th dimension) A third force (the radion )
62 Problems with original Kaluza-Klein theory - Singularities in the equations describing the behavior of electrons - Electromagnetic and gravitational forces of equal strength - Predicts an extra field (the radion ) not observed in nature - Predicts a tower or set of very massive particles at extremely high energies that are not observed in nature (yet) These are caused by the effects of normal particles entering the extra dimension with enough energy or momentum
63 Kaluza-Klein spaces (2 compactified dimensions) 2 dimensions compactified in the shape of a sphere 2 dimensions compactified in the shape of a torus - Compactified dimensions exist at all points in space - They are shown only at grid line intersections for clarity
64 Attempts at revised Kaluza-Klein theories -1938: Klein tries a 6-D theory including the nuclear strong and weak forces as well as gravity and electromagnetism Theory predicted numerous massless bosons not observed in nature -1938: Einstein, Bergmann and Bargmann try a 5-D theory in which the 5 th dimension is rolled up along one of the other space dimensions into a sub-nanoscopic tube Theory predicted that electromagnetism and gravity should be similar in strength : Cremmer, Julia and Scherk propose an 11-D theory of supersymmetric gravity in which 6 dimensions roll up into sub-nanoscopic hyperspheres
65 String theory - Began in the late 1960s and early 1970s as an attempt to describe bosons as vibrations of stringlike objects Different vibrational modes equate to different quantum number configurations (different particles and particle characteristics) - Later expanded to represent all particles including gravitons Predicts and requires supersymmetric particles - Unifies gravity with electromagnetism, strong and weak forces - Explains hierarchy problem - Can t be tested experimentally at present Energies required are far too large to probe strings directly LHC at CERN may detect supersymmetric particles
66 Example: string vibrational modes and particle mass Low energy mode = low particle mass Intermediate energy mode = intermediate particle mass High energy mode = high particle mass - Above illustration is for a closed string particle vibrating in 2-D only
67 Strings and world sheets time space space
68 Particle interactions in string theory e - e - time g space space - No single points of intersection = no singularities
69 Uncertainty in string theory - Quantum field theory: basic measure of uncertainty given by Planck s constant h = x ev sec Momentum (or position) can t be defined more precisely - String theory: new basic measure of uncertainty given by the string size a = cm 2 Spacetime can t be defined more precisely
70 String theory requires 10 dimensions - Why? Accommodates enough degrees of vibrational freedom to represent all the different quantum numbers (mass, charge, spin, etc.) Incorporates all standard model gauge symmetries Mathematically consistent (no negative probabilities, no singularities, etc.) - What happens to the other 6 dimensions? They may compactify, as in the Kaluza-Klein theory Or they may be large, but inaccessible to us (leads to concept of branes in M-theory) - Size of the compactified dimensions: ~10-34 m (as in Kaluza-Klein theories)
71 How do the extra dimensions compactify? - Not all compactification mechanisms lead to valid physics The shape of the compactified dimensions must allow for the proper kinds of string vibrations to generate the particles and quantum properties we observe in nature - In 10-D theories: Extra 6 dimensions compactify into Calabi-Yau spaces
72 Shing-Tung Yau Chinese-American mathematician, chair of Harvard University mathematics department; Fields Medal, In 1976, proved a conjecture of Eugenio Calabi about the existence of good metrics on complex manifolds, thereby discovering Calabi-Yau spaces
73 Animation of 3-D projection of 6-D Calabi-Yau space
74 3-D projection of a 6-D Calabi-Yau space - The pattern of holes in the space affects the vibrational patterns of the strings, which determines the quantum numbers of the particles (charge, spin, etc.)
75 3-D projection of another 6-D Calabi-Yau space -There are tens of thousands of Calabi-Yau spaces and very few criteria for choosing which one represents our universe - It should have 3 holes, since there are 3 particle families
76 10-D space with 6 dimensions compactified in a Calabi-Yau shape - Compactified dimensions exist at all points in space - They are shown at grid intersection points only for clarity
77 Summary of string theories Type IIB Type IIA E 8 x E 8 Heterotic SO(32) Heterotic Type I SO(32) String Type Closed Closed Closed Closed Open (& closed) 10d Supersymmetry N=2 (chiral) N=2 (nonchiral) N=1 N=1 N=1 10d Gauge symmetry none none E 8 x E 8 SO(32) SO(32)
78 Summary of string theories Type IIB Type IIA E 8 x E 8 Heterotic SO(32) Heterotic Type I SO(32) String Type Closed Closed Closed Closed Open (& closed) 10d Supersymmetry N=2 (chiral) N=2 (nonchiral) N=1 N=1 N=1 10d Gauge symmetry none none E 8 x E 8 SO(32) SO(32) - At low energies, the E 8 x E 8 Heterotic theory compactified on a Calabi-Yau space resembles the Standard Model
79 How E 8 x E 8 heterotic theory compactified on Calabi-Yau space resembles SM physics Flat 10-D Superstring E 8 x E 8 theory 6 compact dimensions, 4 ordinary dimensions Superstring E 8 x E 8 theory Calabi-Yau compactification Massive particles with fractional electric charges shadow matter Magnetic monopoles Unified U(1) x SU(2) x SU(3) + supergravity + U(1) x SU(2) x? New forces Electromagnetism Weak force Strong force Gravity Particles Superparticles
80 Edward Witten Physicist, Institute for Advanced Study, Princeton; Fields Medal, Key developer of string theory, along with Andre Neveu, John Schwarz, Michael Green and Pierre Ramond - Originator of M-theory as a unifying concept uniting several different types of string theories - String theory is a part of 21 st century physics that fell by chance into the 20 th century
81 Witten s question: Search for a realistic Kaluza-Klein theory What is the minimum dimension of a space which can have SU(3) x SU(2) x U(1) gauge symmetry? U(1) = electromagnetic field symmetry (represented by rotations around a circle): needs 1 dimension SU(2) = weak force symmetry (represented by rotations on the surface of a sphere): needs 2 dimensions SU(3) = strong force symmetry (represented by rotations in a space with several complex variables): needs 4 dimensions Adding these 7 dimensions to the 4 dimensions of spacetime gives 11 total dimensions
82 M-Theory - 11 dimensions (10 space, 1 time) - Not all the extra dimensions are compactified some are extended - Our universe is a 4-dimensional subset (4-brane) of the whole 11-dimensional space (the bulk ) - There may be other subsets besides ours!
83 Heterotic SO(32) Heterotic E8 x E8
84 Virtual string pair formation and space string coupling constants space time String interaction String splits into virtual string pair Strings recombine Interaction termination - Coupling constant determines the probability of one string splitting into a virtual string pair - Weak coupling (constant <1) means probability can be ignored for multiple successive loops; strong coupling (constant >1) means it can not be ignored - S-Duality: physics of one theory s strong coupling = physics of another theory s weak coupling
85 Closed string winding modes on compactified dimensions r radius of compactified dimension - Winding creates energy in addition to the string vibrations and the motion of the string along or around the dimension - In certain cases the sum of winding and vibration/motion energy is the same for radius = r and radius = 1/r - In these cases the physics of large and small dimensions and unwound and wound strings is the same: T-duality
86 M-Theory and relationships among different string theories - T-duality: Physics of theory compactified at radius r = physics of alternate theory compactified at radius 1/r - S-duality: Physics of one theory s strong coupling = physics of alternate theory s weak coupling
87 Shrinking a 2-D toroidal brane s radius to zero to form a closed string 11-D M-theory 10-D Type IIA string theory r - r = radius of toroidal brane
88 Example: Relationship between M-theory in 11 dimensions and Type IIA string theory in 10 dimensions 11-dimension M-theory compactified on sub-nano-circle Wrap 2-D brane on circle, join ends to form torus and reduce radius of torus to zero Shrink membrane to zero size IIA in 10 dimensions IIA superstring point particle Unwrapped brane Wrap 5-D brane on circle flat plane 4-D space-time
89 Large Extra Dimension Models - By experimental limits, extra dimensions could still be as large as 0.1 millimeter This will be tested by gravity, which behaves as F ~ M 1 M 2 / r n+2 for n extra dimensions - Large extra dimensions would show up in experiments at the LHC as invisible missing energy disappearing into the extra dimensions, or as one micro black hole a second being produced
90 String Theory (or M-Theory): Multiverse - Particles = vibrating strings in 11-D space-time (the Bulk ) - Universes = subsets of the Bulk (ours is a 4-D brane ) - String vibrational patterns determine particle characteristics (e.g. charge, mass-energy, spin, etc.) - M-theory parameters specify and restrict strings behavior Hundreds of parameters ( moduli ) - Countably infinite number ( 0 ) of branes (universes) Each described by a different M-theory Vast majority will be unstable and vanish Tiny fraction but still huge number (~ ) of stable ones remain, of which ours is one - Because of this huge number we can t tell exactly which M-theory describes our specific universe
91 Strings and branes in the bulk Open strings (attached to brane) Closed strings (can leave brane) Brane Another brane
92 The Multiverse
93 The M-Theory Multiverse Landscape - Graph axes show only 2 out of hundreds of M-theory parameters ( moduli ) that determine how strings behave Potential energy density - Each point on the Landscape represents a single Universe with a particular range of string behaviors - Each Universe could be realized in a separate post-inflation bubble
94 Lisa Randall Professor of Physics, Harvard University - Winner of Westinghouse Science Talent Search as high school student - With student Raman Sundrum, authored seminal 1999 paper suggesting that extra dimensions did not need to be compactified and that gravity could move among branes while other forces would remain stuck to individual branes
95 String size = cm Randall-Sundrum Model (RS-1) String size = cm ( Bulk )
96 Paul Steinhardt Albert Einstein Professor of Physics, Princeton University; Dirac Medal, With Neil Turok of Cambridge, developed the ekpyrotic universe theory, in which the big bang is replaced by a cyclic collision between branes (with a cycle time approximating 1 trillion years)
97 M-Theory: Two Branes Colliding in the Bulk - The distance between the branes in the bulk may be about 0.1 millimeter
98
99 Issues with M-theory and string theory - Can not be experimentally tested (yet) Hopes placed on LHC at CERN to detect supersymmetric particles, but this will not prove the theory - Mathematics to fully develop the theory largely doesn t exist General relativity and quantum field theory: mathematics mostly developed 50+ years before the physics M-theory: similar to development of calculus with Newton and Leibniz physics is stimulating the creation of completely new mathematics (e.g. non-commutative geometry, quantum geometry) - Does not really describe a specific universe No principles for selecting which of the zillions of choices in the multiverse landscape represents our universe
100 Actually, I would not even be prepared to call string theory a theory imagine that I give you a chair, while explaining that the legs are still missing, and that the seat, back, and armrest will be delivered soon; whatever I did give you, can I still call it a chair? Gerard t Hooft, Nobel Prize winner in Physics
101
102 Matter and force carrier particles and their major characteristics - Note the three generations or families of matter particles (fermions) every particle also has an anti-particle
103
104 space time
105 Bosons Force carrying particles (8) massless
106 Kinds of quarks and anti-quarks
107
108 The unification of forces in physics - Strong Force - Weak Force -Electro Magnetic Force - The goal of unification theories (like string theory) is to explain the?
109 Relative strengths of forces in Standard Model ( hierarchy problem ) -The hierarchy problem is the problem of explaining the difference in the strengths of the four forces
110 Gauge symmetry 1. Potential value of a field at different points in spacetime
111 Gauge symmetry 1. Potential value of a field at different points in spacetime 2. Variation of value of potential at different points in spacetime
112 Gauge symmetry 1. Potential value of a field at different points in spacetime 2. Variation of value of potential at different points in spacetime 3. Variation of value is compensated by gauge field (represented by curved arrows)
113 Gauge symmetry 1. Potential value of a field at different points Variation of value of potential at different points 3. Variation of value is compensated by gauge field (represented by curved arrows) 4. Original field configuration is restored - Quantum of the gauge field is called a gauge boson
114
115
116 The Higgs Field - Minimum potential is not at zero - Therefore symmetry breaks and particle gets positive mass
117 Feynman diagram of neutral weak current (muon neutrino scattering off electron) n m Z o e n m e
118 Symmetry breaking of forces during Big Bang
119 Supersymmetry one solution to the hierarchy problem - SM = Standard Model; MSSM = Minimal Super Symmetric Model - Under the MSSM the electromagnetic (EM), weak (W) and strong (S) forces unify more precisely at high energy than they do under the standard model
120 Supersymmetry one solution to the hierarchy problem - MSSM = Minimal Super Symmetric Model - Under the MSSM the electromagnetic (U(1)), weak (SU(2)), and strong (SU(3)) forces unify more precisely at high energy than they do under the standard model
121 What is supersymmetry? - All particles have superpartners that exist only at very high energies force-carrying bosons have matter fermion partners and vice versa Names of boson superpartners of fermions all start with s e.g., squark, selectron, etc. Names of fermion superpartners of bosons all end with ino - e.g., photino, Wino, gravitino, etc. - Superpartner particles have higher masses than ordinary particles (corresponding to their higher energies) May be detectible by LHC Supersymmetry breaks at much lower energy than force unification (solves hierarchy problem) - Superpartner particles spins differ by ½ from spins of their ordinary partner particles (superpartners spins are ½ less) - Supersymmetry is a basic assumption of string and M-theory
122 Evidence for supersymmetric particles? Observed rotational speed based on Doppler shift data Rotational speed models based on visible light observations of galactic halo, disk and gas - Rotation of galaxies (for example NGC6503) is much faster than predicted from the mass of the visible matter in them - This is evidence for dark matter which could be made up of supersymmetric particles (other explanations possible)
123 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.
124 Symmetries and conservation laws Symmetry Under Implies Conservation of Time dimension translation Space dimension translation Rotation Energy Momentum Angular momentum
125 Closed string vibrating in 3D
126 Gauge symmetry We can illustrate the concept of gauge symmetry as follows: - Electric and magnetic fields can be expressed using potential functions. - These can be exchanged (gauge-transformed ) according to a certain rule without changing the fields. The simplest transformation is to add a constant to the electric potential Physically this illustrates the well-known fact that electric potential can be calculated from an arbitrary zero point, since only the differences in potential are significant. This is why a squirrel can walk along a highvoltage cable without being injured. - That the zero point can be moved in this way is perceived by physicists as a symmetry in the theory, gauge symmetry.
127 How E 8 x E 8 heterotic string compactified on Calabi-Yau space resembles SM physics
128 Type I SO(32) Heterotic M-Theory Type IIA 11-D Supergravity E8xE8 Heterotic Type IIB
129 - Exist in M-theory Branes - N-dimensional membranes or hypersurfaces that are subsets of the whole 11-dimensional spacetime (the bulk ) - Our universe is a 4-dimensional brane (or D4-brane ) - There may be other branes of varying dimensionality - Open strings live on branes (are permanently attached) If open strings represent fermions and bosons, it means that all normal matter plus the strong, weak and electromagnetic forces are stuck in our own D4-brane - Closed strings can move through the bulk If closed strings represent gravitons, it means that gravitational forces can be felt across branes Suggests another possible explanation for dark matter
130 Collision of proton and antiproton in a brane - Collision produces normal particles (blue balls), graviton (ripples in brane), and Kaluza-Klein mode of graviton (ball going up out of brane)
131 M-Theory Multiverse - Different universes may be formed by different branes in the bulk - Each universe may have a different number of dimensions, different laws of physics, etc. Based on a number of free parameters in the M-theory describing each universe - There are an infinite number of different universes in the multiverse landscape Each described by a different M-theory The vast majority of them will be unstable and vanish A tiny fraction but still huge number (estimated at > ) of stable ones will remain, of which ours is one
132 Strings, Branes and Black Holes Surface of 5D torus - Hawking radiation: open strings travel in both directions down the D1-brane, emitting closed strings (radiation) when they interact. The system decays into the configuration on the right
133 Ekpyrotic vs. Big Bang model with inflation EKPYROTIC EKPYROTIC MODEL
Physics Beyond the Standard Model. Marina Cobal Fisica Sperimentale Nucleare e Sub-Nucleare
Physics Beyond the Standard Model Marina Cobal Fisica Sperimentale Nucleare e Sub-Nucleare Increasingly General Theories Grand Unified Theories of electroweak and strong interactions Supersymmetry
More informationFinal Exam: Sat. Dec. 18, 2:45-4:45 pm, 1300 Sterling Exam is cumulative, covering all material. From last time
Final Exam: Sat. Dec. 18, 2:45-4:45 pm, 1300 Sterling Exam is cumulative, covering all material From last time Quantum field theory is a relativistic quantum theory of fields and interactions. Fermions
More informationBeyond the standard model? From last time. What does the SM say? Grand Unified Theories. Unifications: now and the future
From last time Quantum field theory is a relativistic quantum theory of fields and interactions. Fermions make up matter, and bosons mediate the forces by particle exchange. Lots of particles, lots of
More informationFundamental Particles and Forces
Fundamental Particles and Forces A Look at the Standard Model and Interesting Theories André Gras PHYS 3305 SMU 1 Overview Introduction to Fundamental Particles and Forces Brief History of Discovery The
More informationAn Introduction to Particle Physics
An Introduction to Particle Physics The Universe started with a Big Bang The Universe started with a Big Bang What is our Universe made of? Particle physics aims to understand Elementary (fundamental)
More informationLecture PowerPoint. Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli
Lecture PowerPoint Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the
More informationParticles and Strings Probing the Structure of Matter and Space-Time
Particles and Strings Probing the Structure of Matter and Space-Time University Hamburg DPG-Jahrestagung, Berlin, March 2005 2 Physics in the 20 th century Quantum Theory (QT) Planck, Bohr, Heisenberg,...
More informationReview Chap. 18: Particle Physics
Final Exam: Sat. Dec. 18, 2:45-4:45 pm, 1300 Sterling Exam is cumulative, covering all material Review Chap. 18: Particle Physics Particles and fields: a new picture Quarks and leptons: the particle zoo
More informationWhat ideas/theories are physicists exploring today?
Where are we Headed? What questions are driving developments in fundamental physics? What ideas/theories are physicists exploring today? Quantum Gravity, Stephen Hawking & Black Hole Thermodynamics A Few
More informationThe following diagram summarizes the history of unification in Theoretical Physics:
Summary of Theoretical Physics L. David Roper, roperld@vt.edu Written for the Book Group of Blacksburg VA For the discussion of The Elegant Universe by Brian Greene, 10 October 004 This file is available
More informationA first trip to the world of particle physics
A first trip to the world of particle physics Itinerary Massimo Passera Padova - 13/03/2013 1 Massimo Passera Padova - 13/03/2013 2 The 4 fundamental interactions! Electromagnetic! Weak! Strong! Gravitational
More informationFACULTY OF SCIENCE. High Energy Physics. WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON
FACULTY OF SCIENCE High Energy Physics WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON AIM: To explore nature on the smallest length scales we can achieve Current status (10-20 m)
More informationPhysics 4213/5213 Lecture 1
August 28, 2002 1 INTRODUCTION 1 Introduction Physics 4213/5213 Lecture 1 There are four known forces: gravity, electricity and magnetism (E&M), the weak force, and the strong force. Each is responsible
More informationGravity, Strings and Branes
Gravity, Strings and Branes Joaquim Gomis Universitat Barcelona Miami, 23 April 2009 Fundamental Forces Strong Weak Electromagnetism QCD Electroweak SM Gravity Standard Model Basic building blocks, quarks,
More informationMost of Modern Physics today is concerned with the extremes of matter:
Most of Modern Physics today is concerned with the extremes of matter: Very low temperatures, very large numbers of particles, complex systems Æ Condensed Matter Physics Very high temperatures, very large
More informationMost of Modern Physics today is concerned with the extremes of matter:
Most of Modern Physics today is concerned with the extremes of matter: Very low temperatures, very large numbers of particles, complex systems Æ Condensed Matter Physics Very high temperatures, very large
More informationString Theory to the Rescue Proof of String Theory & Extra Dimensions?
String Theory to the Rescue Proof of String Theory & Extra Dimensions? EVERY POINT IN THE UNIVERSE IS NO MORE THAN ONE BLOCK FROM A STARBUCKS! Yale Physics 120 4/23/2018 Quantum Physics and Beyond John
More informationOrigin of the Universe - 2 ASTR 2120 Sarazin. What does it all mean?
Origin of the Universe - 2 ASTR 2120 Sarazin What does it all mean? Fundamental Questions in Cosmology 1. Why did the Big Bang occur? 2. Why is the Universe old? 3. Why is the Universe made of matter?
More informationChapter 46. Particle Physics and Cosmology
Chapter 46 Particle Physics and Cosmology Atoms as Elementary Particles Atoms From the Greek for indivisible Were once thought to be the elementary particles Atom constituents Proton, neutron, and electron
More informationBlack holes in D>4 dimensional space-times
Black holes in D>4 dimensional space-times Key-words: extra dimensions, string theory, brane world models, LHC, stability, perturbations, quasinormal modes, Hawking radiation R. A. Konoplya May 20, 2010
More informationElectron-positron pairs can be produced from a photon of energy > twice the rest energy of the electron.
Particle Physics Positron - discovered in 1932, same mass as electron, same charge but opposite sign, same spin but magnetic moment is parallel to angular momentum. Electron-positron pairs can be produced
More informationOverview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions.
Overview The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions. Our understanding is about to take a giant leap.. the Large Hadron Collider
More informationSome PPPs (particle physics puzzles)
Some PPPs (particle physics puzzles) What s up with neutrinos? What is dark matter? What is dark energy? Where does inflation come from? Why is there more matter than antimatter? Are there even more fundamental
More informationParticle Physics. All science is either physics or stamp collecting and this from a 1908 Nobel laureate in Chemistry
Particle Physics JJ Thompson discovered electrons in 1897 Rutherford discovered the atomic nucleus in 1911 and the proton in 1919 (idea of gold foil expt) All science is either physics or stamp collecting
More informationLarge Hadron Collider
Large Hadron Collider Himadri Barman TSU, JNCASR September 18, 2008 0-0 Large Hadron Collider (LHC): Plan We ll see 4 short videos. In between I ll give you a little guideline. Purpose is to understand
More informationChapter 32 Lecture Notes
Chapter 32 Lecture Notes Physics 2424 - Strauss Formulas: mc 2 hc/2πd 1. INTRODUCTION What are the most fundamental particles and what are the most fundamental forces that make up the universe? For a brick
More informationCuriosités géométriques et physique de l'univers
Curiosités géométriques et physique de l'univers MidiSciences, Grenoble, 05/2010 String Theory & Invisible Dimensions Ecole Normale Supérieure de Lyon plan fundamental interactions standard model vs. general
More informationINTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS
INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS Class Mechanics My office (for now): Dantziger B Room 121 My Phone: x85200 Office hours: Call ahead, or better yet, email... Even better than office
More informationAstronomy 182: Origin and Evolution of the Universe
Astronomy 182: Origin and Evolution of the Universe Prof. Josh Frieman Lecture 12 Nov. 18, 2015 Today Big Bang Nucleosynthesis and Neutrinos Particle Physics & the Early Universe Standard Model of Particle
More informationAnnouncement. Station #2 Stars. The Laws of Physics for Elementary Particles. Lecture 9 Basic Physics
Announcement Pick up your quiz after this lecture as you leave the lecture hall. Homework#2 due on Thursday No hand-written homework! Please staple them! Put it in the box before the lecture begins! Station
More informationGravity, Strings and Branes
Gravity, Strings and Branes Joaquim Gomis International Francqui Chair Inaugural Lecture Leuven, 11 February 2005 Fundamental Forces Strong Weak Electromagnetism QCD Electroweak SM Gravity Standard Model
More informationKiwoon Choi (KAIST) 3 rd GCOE Symposium Feb (Tohoku Univ.)
Exploring New Physics beyond the Standard Model of Particle Physics Kiwoon Choi (KAIST) 3 rd GCOE Symposium Feb. 2011 (Tohoku Univ.) We are confronting a critical moment of particle physics with the CERN
More informationElementary particles and typical scales in high energy physics
Elementary particles and typical scales in high energy physics George Jorjadze Free University of Tbilisi Zielona Gora - 23.01.2017 GJ Elementary particles and typical scales in HEP Lecture 1 1/18 Contents
More informationThe God particle at last? Astronomy Ireland, Oct 8 th, 2012
The God particle at last? Astronomy Ireland, Oct 8 th, 2012 Cormac O Raifeartaigh Waterford Institute of Technology CERN July 4 th 2012 (ATLAS and CMS ) A new particle of mass 125 GeV I The Higgs boson
More informationFinish up our overview of small and large
Finish up our overview of small and large Lecture 5 Limits of our knowledge Clicker practice quiz Some terminology... "Elementary particles" = objects that make up atoms (n,p,e) or are produced when atoms
More informationLecture 03. The Standard Model of Particle Physics. Part III Extensions of the Standard Model
Lecture 03 The Standard Model of Particle Physics Part III Extensions of the Standard Model Where the SM Works Excellent description of 3 of the 4 fundamental forces Explains nuclear structure, quark confinement,
More informationSupersymmetry and how it helps us understand our world
Supersymmetry and how it helps us understand our world Spitalfields Day Gauge Theory, String Theory and Unification, 8 October 2007 Theoretical Physics Institute, University of Minnesota What is supersymmetry?
More informationPH5211: High Energy Physics. Prafulla Kumar Behera Room: HSB-304B
PH5211: High Energy Physics Prafulla Kumar Behera E-mail:behera@iitm.ac.in Room: HSB-304B Information Class timing: Wed. 11am, Thur. 9am, Fri. 8am The course will be graded as follows: 1 st quiz (20 marks)
More informationLecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM
Lecture 03 The Standard Model of Particle Physics Part II The Higgs Boson Properties of the SM The Standard Model So far we talked about all the particles except the Higgs If we know what the particles
More informationChapter 27: The Early Universe
Chapter 27: The Early Universe The plan: 1. A brief survey of the entire history of the big bang universe. 2. A more detailed discussion of each phase, or epoch, from the Planck era through particle production,
More informationElementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016
Elementary Particle Physics Glossary Course organiser: Dr Marcella Bona February 9, 2016 1 Contents 1 Terms A-C 5 1.1 Accelerator.............................. 5 1.2 Annihilation..............................
More informationMATTER AND FORCES MATILDE MARCOLLI
MATTER AND FORCES MATILDE MARCOLLI Contents 1. The Standard Model of Particle Physics 2 2. The Geometrization of Physics 8 2.1. Evolution of the Kaluza-Klein idea 10 3. What is a good mathematical model?
More informationParticle + Physics at ATLAS and the Large Hadron Coillder
Particle + Physics at ATLAS and the Large Hadron Coillder Discovering the elementary particles of the Universe Kate Shaw The International Centre for Theoretical Physics + Overview Introduction to Particle
More informationSupersymmetry. Physics Colloquium University of Virginia January 28, Stephen P. Martin Northern Illinois University
Supersymmetry Physics Colloquium University of Virginia January 28, 2011 Stephen P. Martin Northern Illinois University 1 The Standard Model of particle physics The Hierarchy Problem : why is the Higgs
More informationarxiv:hep-ph/ v1 8 Feb 2000
Gravity, Particle Physics and their Unification 1 J. M. Maldacena Department of Physics Harvard University, Cambridge, Massachusetts 02138 arxiv:hep-ph/0002092v1 8 Feb 2000 1 Introduction Our present world
More informationUNVEILING THE ULTIMATE LAWS OF NATURE: DARK MATTER, SUPERSYMMETRY, AND THE LHC. Gordon Kane, Michigan Center for Theoretical Physics Warsaw, June 2009
UNVEILING THE ULTIMATE LAWS OF NATURE: DARK MATTER, SUPERSYMMETRY, AND THE LHC Gordon Kane, Michigan Center for Theoretical Physics Warsaw, June 2009 OUTLINE! Some things we ve learned about the physical
More information1 Introduction. 1.1 The Standard Model of particle physics The fundamental particles
1 Introduction The purpose of this chapter is to provide a brief introduction to the Standard Model of particle physics. In particular, it gives an overview of the fundamental particles and the relationship
More informationFUNDAMENTAL PARTICLES CLASSIFICATION! BOSONS! QUARKS! FERMIONS! Gauge Bosons! Fermions! Strange and Charm! Top and Bottom! Up and Down!
FUNDAMENTAL PARTICLES CLASSIFICATION! BOSONS! --Bosons are generally associated with radiation and are sometimes! characterized as force carrier particles.! Quarks! Fermions! Leptons! (protons, neutrons)!
More informationSymmetry Groups conservation law quantum numbers Gauge symmetries local bosons mediate the interaction Group Abelian Product of Groups simple
Symmetry Groups Symmetry plays an essential role in particle theory. If a theory is invariant under transformations by a symmetry group one obtains a conservation law and quantum numbers. For example,
More informationThe Standard Model of Particle Physics
The Standard Model of Particle Physics Jesse Chvojka University of Rochester PARTICLE Program Let s s look at what it is Description of fundamental particles quarks and leptons Three out of Four (Forces)
More informationIf I only had a Brane
If I only had a Brane A Story about Gravity and QCD. on 20 slides and in 40 minutes. AdS/CFT correspondence = Anti de Sitter / Conformal field theory correspondence. Chapter 1: String Theory in a nutshell.
More information1. What does this poster contain?
This poster presents the elementary constituents of matter (the particles) and their interactions, the latter having other particles as intermediaries. These elementary particles are point-like and have
More informationAn intimate relationship between Higgs forces, dark matter, and dark energy. Copyright June 2014, by Antonio A. Colella
Antonio A. Colella 1 1 Introduction M062914 An intimate relationship between Higgs forces, dark matter, and dark energy Copyright June 2014, by Antonio A. Colella Abstract. Our universe s eight permanent
More informationSupersymmetry and Supergravity History and Perspectives. Dmitri Sorokin INFN, Sezione di Padova
Supersymmetry and Supergravity History and Perspectives Dmitri Sorokin INFN, Sezione di Padova Supersymmetry and supergravity A hypothetical symmetry of Nature which implies that every elementary particle
More informationUnsolved Problems in Theoretical Physics V. BASHIRY CYPRUS INTRNATIONAL UNIVERSITY
Unsolved Problems in Theoretical Physics V. BASHIRY CYPRUS INTRNATIONAL UNIVERSITY 1 I am going to go through some of the major unsolved problems in theoretical physics. I mean the existing theories seem
More informationThe Correct Interpretation of the Kaluza-Klein Theory
Copyright 2014 by Sylwester Kornowski All rights reserved The Correct Interpretation of the Kaluza-Klein Theory Sylwester Kornowski Abstract: Here, within the Scale-Symmetric Everlasting Theory (S-SET),
More informationThe Large Hadron Collider, and New Avenues in Elementary Particle Physics. Gerard t Hooft, Public Lecture, IPMU Tokyo, April 16, 2015
The Large Hadron Collider, and New Avenues in Elementary Particle Physics Gerard t Hooft, Public Lecture, IPMU Tokyo, April 16, 2015 CERN European Center for Nuclear Research LHC Large Hadron Collider
More informationTHE PHYSICS/COSMOLOGY CONNECTION. 1. Summary of Particle Physics: The Standard Model limitations of the standard model
THE PHYSICS/COSMOLOGY CONNECTION 1. Summary of Particle Physics: The Standard Model limitations of the standard model 2. Summary of Cosmology: The Big Bang Model limitations of the Big Bang model 3. Unifying
More informationI. Antoniadis CERN. IAS CERN Novice Workshop, NTU, 7 Feb 2014
I. Antoniadis CERN IAS CERN Novice Workshop, NTU, 7 Feb 2014 1 2 3 the Large Hadron Collider (LHC) Largest scientific instrument ever built, 27km of circumference >10 000 people involved in its design
More informationChapter 27 The Early Universe Pearson Education, Inc.
Chapter 27 The Early Universe Units of Chapter 27 27.1 Back to the Big Bang 27.2 The Evolution of the Universe More on Fundamental Forces 27.3 The Formation of Nuclei and Atoms 27.4 The Inflationary Universe
More informationThe God particle at last? Science Week, Nov 15 th, 2012
The God particle at last? Science Week, Nov 15 th, 2012 Cormac O Raifeartaigh Waterford Institute of Technology CERN July 4 th 2012 (ATLAS and CMS ) A new particle of mass 125 GeV Why is the Higgs particle
More informationEinige interessante Aspekte der in der Zielsetzung genannten Fragestellungen. Appetithappen -> Antworten spaeter in der Vorlesung.
0. Einführung Einige interessante Aspekte der in der Zielsetzung genannten Fragestellungen. Appetithappen -> Antworten spaeter in der Vorlesung. Folien auf Englisch (aus anderer Vorlesung ausgeliehen)
More informationPHY323:Lecture 11 SUSY and UED Higgs and Supersymmetry The Neutralino Extra Dimensions How WIMPs interact
PHY323:Lecture 11 SUSY and UED Higgs and Supersymmetry The Neutralino Extra Dimensions How WIMPs interact Candidates for Dark Matter III The New Particle Zoo Here are a few of the candidates on a plot
More informationWeak interactions and vector bosons
Weak interactions and vector bosons What do we know now about weak interactions? Theory of weak interactions Fermi's theory of weak interactions V-A theory Current - current theory, current algebra W and
More informationExtra Dimensions in Physics? Shamit Kachru Stanford University
Extra Dimensions in Physics? Shamit Kachru Stanford University One of the few bits of fundamental physics that becomes obvious to most of us in childhood: our playing field consists of three spatial dimensions,
More informationCosmology and particle physics
Cosmology and particle physics Lecture notes Timm Wrase Lecture 5 The thermal universe - part I In the last lecture we have shown that our very early universe was in a very hot and dense state. During
More informationHiggs Field and Quantum Gravity
Higgs Field and Quantum Gravity The magnetic induction creates a negative electric field, causing an electromagnetic inertia responsible for the relativistic mass change; it is the mysterious Higgs Field
More informationIt is possible for a couple of elliptical galaxies to collide and become a spiral and for two spiral galaxies to collide and form an elliptical.
7/16 Ellipticals: 1. Very little gas and dust an no star formation. 2. Composed of old stars. 3. Masses range from hundreds of thousands to 10's of trillions of solar masses. 4. Sizes range from 3000 ly
More informationLecture 39, 40 Supplement: Particle physics in the LHC era
Lecture 39, 40 Supplement: Particle physics in the LHC era The Matter Particles (Fermions) plus their antiparticles... What is measured? quarks confined into hadrons A zoo of strongly interacting particles...
More informationThe Scale-Symmetric Theory as the Origin of the Standard Model
Copyright 2017 by Sylwester Kornowski All rights reserved The Scale-Symmetric Theory as the Origin of the Standard Model Sylwester Kornowski Abstract: Here we showed that the Scale-Symmetric Theory (SST)
More informationParticles and Interactions. Prof. Marina Cobal Corso Particelle ed interazioni fondamentali 2013/2014
Particles and Interactions Prof. Marina Cobal Corso Particelle ed interazioni fondamentali 2013/2014 What is the world made of? In the ancient time: 4 elements 19 century atoms Beginning 20 th century
More informationPhysics 662. Particle Physics Phenomenology. February 21, Physics 662, lecture 13 1
Physics 662 Particle Physics Phenomenology February 21, 2002 Physics 662, lecture 13 1 Physics Beyond the Standard Model Supersymmetry Grand Unified Theories: the SU(5) GUT Unification energy and weak
More informationIntroduction. Read: Ch 1 of M&S
Introduction What questions does this field address? Want to know the basic law of nature. Can we unify all the forces with one equation or one theory? Read: Ch 1 of M&S K.K. Gan L1: Introduction 1 Particle
More information2. The evolution and structure of the universe is governed by General Relativity (GR).
7/11 Chapter 12 Cosmology Cosmology is the study of the origin, evolution, and structure of the universe. We start with two assumptions: 1. Cosmological Principle: On a large enough scale (large compared
More informationThe Four Fundamental Forces. The Four Fundamental Forces. Gravitational Force. The Electrical Force. The Photon (γ) Unification. Mass.
The Four Fundamental Forces What are the four fundamental forces? The Four Fundamental Forces What are the four fundamental forces? Weaker Stronger Gravitational, Electromagnetic, Strong and Weak Nuclear
More informationString Theory. Three String Theories STRING THEORY 1. John H. Schwarz
STRING THEORY 1 String Theory John H. Schwarz Traditional studies of the relativistic quantum physics of elementary particles assume that the particles can be described as mathematical points without any
More informationFrom Quantum Mechanics to String Theory
From Quantum Mechanics to String Theory Relativity (why it makes sense) Quantum mechanics: measurements and uncertainty Smashing things together: from Rutherford to the LHC Particle Interactions Quarks
More informationToday. The goals of science. The nature of the Universe - Beyond the Standard Model
Today The nature of the Universe - Beyond the Standard Model Dark Matter and Dark Energy String Theory and the quest to unify gravity and quantum theory Begin watching PBS NOVA special The Elegant Universe
More informationToday. The nature of the Universe - Beyond the Standard Model
Today The nature of the Universe - Beyond the Standard Model Dark Matter and Dark Energy String Theory and the quest to unify gravity and quantum theory Begin watching PBS NOVA special The Elegant Universe
More informationg abφ b = g ab However, this is not true for a local, or space-time dependant, transformations + g ab
Yang-Mills theory Modern particle theories, such as the Standard model, are quantum Yang- Mills theories. In a quantum field theory, space-time fields with relativistic field equations are quantized and,
More informationParticle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo
Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo Particle Physics Fall 2015 1 Course Overview Lecture 1: Introduction, Decay Rates and Cross Sections Lecture 2: The Dirac Equation and Spin
More informationExam Results. Force between charges. Electric field lines. Other particles and fields
Exam: Exam scores posted on Learn@UW No homework due next week Exam Results F D C BC B AB A Phy107 Fall 2006 1 Particles and fields We have talked about several particles Electron,, proton, neutron, quark
More informationThe Standard Model of particle physics and beyond
The Standard Model of particle physics and beyond - Lecture 3: Beyond the Standard Model Avelino Vicente IFIC CSIC / U. Valencia Physics and astrophysics of cosmic rays in space Milano September 2016 1
More informationWhat lies beyond? Erich Poppitz University of Toronto
What lies beyond? Erich Poppitz University of Toronto A theorist s view on the problems and perspectives of particle physics beyond the standard model general principles facts What are the smallest constituents
More informationElectroweak Symmetry Breaking
Electroweak Symmetry Breaking An enduring mystery of the standard model of particle physics and how we hope to solve it David Schaich Department of Physics and Center for Computational Science Boston University
More informationParticle physics today. Giulia Zanderighi (CERN & University of Oxford)
Particle physics today Giulia Zanderighi (CERN & University of Oxford) Particle Physics Particle Physics is fundamental research, as opposed to many applied sciences (medicine, biology, chemistry, nano-science,
More informationParticles, Energy, and Our Mysterious Universe
Particles, Energy, and Our Mysterious Universe 1 The End of Physics "The more important fundamental laws and facts of physical science have all been discovered, and these are now so firmly established
More informationOption 212: UNIT 2 Elementary Particles
Department of Physics and Astronomy Option 212: UNIT 2 Elementary Particles SCHEDULE 26-Jan-15 13.00pm LRB Intro lecture 28-Jan-15 12.00pm LRB Problem solving (2-Feb-15 10.00am E Problem Workshop) 4-Feb-15
More informationSupersymmetry and a Candidate for Dark Matter
Supersymmetry and a Candidate for Dark Matter Elizabeth Lockner Department of Physics, University of Maryland College Park, MD 20742 April 20, 2007. The Standard Model has been a powerful tool in understanding
More informationChapter 29 Lecture. Particle Physics. Prepared by Dedra Demaree, Georgetown University Pearson Education, Inc.
Chapter 29 Lecture Particle Physics Prepared by Dedra Demaree, Georgetown University Particle Physics What is antimatter? What are the fundamental particles and interactions in nature? What was the Big
More informationThe Multiverse Next Step in Our Growing Understanding of Reality? Gerald B. Cleaver
Astronomy, OFotU The Multiverse Next Step in Our Growing Understanding of Reality? Gerald B. Cleaver To understand the whole of reality has been the pursuit of humankind since the appearance of our species.
More informationThe Standard Model, Supersymmetry and ZooFinder at CDF. Matthew C. Cervantes Department of Physics Texas A&M University Master defense: 7/21/2006
The Standard Model, Supersymmetry and ZooFinder at CDF Matthew C. Cervantes Department of Physics Texas A&M University Master defense: 7/21/2006 1 Outline The Standard Model of Particle Physics Supersymmetry
More informationChapter 22 Lecture. The Cosmic Perspective. Seventh Edition. The Birth of the Universe Pearson Education, Inc.
Chapter 22 Lecture The Cosmic Perspective Seventh Edition The Birth of the Universe The Birth of the Universe 22.1 The Big Bang Theory Our goals for learning: What were conditions like in the early universe?
More informationChapter 22: Cosmology - Back to the Beginning of Time
Chapter 22: Cosmology - Back to the Beginning of Time Expansion of Universe implies dense, hot start: Big Bang Future of universe depends on the total amount of dark and normal matter Amount of matter
More informationThe Building Blocks of Nature
The Building Blocks of Nature PCES 15.1 Schematic picture of constituents of an atom, & rough length scales. The size quoted for the nucleus here (10-14 m) is too large- a single nucleon has size 10-15
More informationParticles and Forces
Particles and Forces Particles Spin Before I get into the different types of particle there's a bit more back story you need. All particles can spin, like the earth on its axis, however it would be possible
More informationThe mass of the Higgs boson
The mass of the Higgs boson LHC : Higgs particle observation CMS 2011/12 ATLAS 2011/12 a prediction Higgs boson found standard model Higgs boson T.Plehn, M.Rauch Spontaneous symmetry breaking confirmed
More informationSaturday Morning Physics -- Texas A&M University. What is Matter and what holds it together? Dr. Rainer J. Fries. January 27, 2007
Saturday Morning Physics -- Texas A&M University Particles and Forces What is Matter and what holds it together? Dr. Rainer J. Fries January 27, 2007 Zooming in on the World around us Particles and Forces
More informationSaturday Morning Physics -- Texas A&M University Dr. Rainer J. Fries
Saturday Morning Physics -- Texas A&M University Particles and Forces What is Matter and what holds it together? Dr. Rainer J. Fries January 27, 2007 Zooming in on the World around us Particles and Forces
More informationQUANTUM FIELD THEORY. A Modern Introduction MICHIO KAKU. Department of Physics City College of the City University of New York
QUANTUM FIELD THEORY A Modern Introduction MICHIO KAKU Department of Physics City College of the City University of New York New York Oxford OXFORD UNIVERSITY PRESS 1993 Contents Quantum Fields and Renormalization
More information