Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 1 PHYS 3446 – Lecture #20 Monday, Nov. 20, 2006 Dr. Jae Yu 1. Parity Properties of Parity Determination.

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Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 1 PHYS 3446 – Lecture #20 Monday, Nov. 20, 2006 Dr. Jae Yu 1. Parity Properties of Parity Determination of Parity Conservation and violation of parity 2. Time Reversal and Charge Conjugation 3. The Standard Model Quarks and Leptons Gauge Bosons Symmetry Breaking and the Higgs particle

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 2 2 nd term exam –In class, this Wednesday, Nov. 22 –Covers: Ch 4 – CH11 Workshop on Saturday, Dec. 2 –10am – 5pm –CPB 303 and other HEP areas Write up due: Before class Wednesday, Dec. 6 Announcements

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 3 Due date: Prior to class on Wednesday, Dec. 6 Requirements –Need to put the name(s) of the person(s) who wrote the given sections –Professionally prepared in MS words No spelling or grammar mistakes The style of the write up should be unified so that it looks like written by one person –All contents on the template and more should be contained in the write up –Pictures, diagrams and photos should be added w/ appropriate figure captions numbered in order of appearance. The captions should go at the bottom of the figure. –References must be indicated throughout the text in order of appearance. They must be properly matched in the list of bibliography at the end of the document. –Tables must be added and numbered in order of appearance. The caption should go on top of the table. Key evaluation points –Quality of the document – 30% –Content and organization of the document – 20 % –Satisfaction of the above requirements – 25% –Thoughtfulness, usefulness and relevance of contents of the document – 25% E.g. The contact information of vendors must be usable for the construction Write Up Requirements and Evaluation

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 4 Requirements –Professionally prepared using power points Need your presentations 30 min prior to the class –Each presentation must be 10min (presentation) + 2min (question and answer) –Must have the following components: General Introduction Motivation Design considerations and requirements Design features Test of design and its functionality Conclusions and future improvements Key evaluation points – 25% each –Quality of the slides –Content and organization of the slides –Knowledge on presentation material – answers to questions –Manner of presentation Presentation Requirements

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 5 Monday, Dec. 4: 1.Shane 2.Daniel 3.Heather 4.Justin 5.Cassie 6.Layne Wednesday, Dec. 6: 1.Pierce 2.Jessica 3.James 4.Matt 5.Lauren Presentation Schedule

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 6 To keep local gauge invariance, new particles had to be introduced in gauge theories – U(1) gauge introduced a new field (particle) that mediates the electromagnetic force: Photon – SU(2) gauge introduces three new fields that mediate weak force Charged current mediator: W+ W+ and W-W- Neutral current: Z0Z0 – SU(3) gauge introduces 8 mediators (gluons) for the strong force Unification of electromagnetic and weak force SU(2)xU(1) gauge introduces a total of four mediators –Neutral current: Photon, Z0Z0 –Charged current: W+ W+ and W-W- Gauge Fields and Mediators

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 7 The space inversion transformation (mirror image)  Switch right- handed coordinate system to left-handed How is this different than normal spatial rotation? –Rotation is continuous in a given coordinate system Quantum numbers related to rotational transformation are continuous –Space inversion cannot be obtained through any set of rotational transformation Quantum numbers related to space inversion is discrete Parity is an example of the discrete transformation Parity

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 8 Position and momentum vectors change sign under space inversion Where as their magnitudes do not change signs Vectors (particles w/ J P =1 - ) change signs under space-inversion while the scalars (particles w/ J P =0 + ) do not. Properties of Parity

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 9 Some vectors, however, behave like a scalar –Angular momentum –These are called pseudo-vectors or axial vectors (particles w/ J P =1 + ) Likewise some scalars behave like vectors –These are called pseudo-scalars (particles w/ J P =0 - ) Two successive application of parity operations must turn the coordinates back to original – –The possible values (eigen values) of parity, P, are +1 (even) or (odd). Parity is a multiplicative quantum number Properties of Parity

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 10 Two parity quantum numbers –Intrinsic parity: Bosons have the same intrinsic parities as their anti-particles while fermions have opposite parity than its anti- particle (odd) Why? –Parity under spatial transformation that follows the rule: P=(- 1) l l is the orbital angular momentum quantum number Are electromagnetic and gravitational forces invariant under parity operation or space inversion? –Newton’s equation of motion for a point-like particle –For electromagnetic and gravitational forces we can write the forces, and thus are invariant under parity. Parity

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 11 How do we find out the intrinsic parity of particles? –Use observation of decays and production processes –Absolute determination of parity is not possible, just like electrical charge or other quantum numbers. –Thus the accepted convention is to assign +1 intrinsic parity to proton, neutron and the  hyperon. The parities of other particles are determined relative to these assignments through the analysis of parity conserving interactions involving these particles.  hyperon is always produced with a K in pair. So one can only determine parity of K if parity of  is fixed. Determination of Parity Quantum Numbers

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 12 When the parity is conserved, it can restrict decay processes that can take place. Consider a parity conserving decay: A  B+C –Conservation of angular momentum requires both sides to have the same total angular momentum J. –If B and C are spinless, their relative orbital angular momentum ( l ) must be the same as J(= l +s). –Thus conservation of parity implies that –If the decay products have spin zero, for the reaction to take place we must have between the intrinsic parities Parity Determination

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 13 Therefore, the allowed decays must have –Where the spin intrinsic parity of the particles are expressed as JPJP Are the following decays allowed under parity conservation? Parity Determination

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 14 Consider the absorption of low energy - - in deuterium nuclei The conservation of parity would require What are the intrinsic parity of deuteron and of the two neutrons? –Deuteron: +1; Neutrons: +1 This capture process is known to proceed from an l i =0 state, thus we obtain Example 1,  - parity

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 15 Since spin of the deuteron J d =1, only a few possible states are allowed for the final state neutrons Since the two neutrons are identical fermions, their overall wave functions must be anti-symmetric due to Pauli’s exclusion principle  leaves only (3) as the possible solution Making pion a pseudo-scalar w/ intrinsic parity Example 1,  - parity, cont’d or

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 16 Until the observation of “  ” puzzle in cosmic ray decays late 1950’s, parity was thought to be conserved in (symmetry of) all fundamental interactions The  and  particles seem to have identical mass, lifetimes, and spin (J=0) but decay differently These seem to be identical particles. Then, how could the same particle decay in two different manner, violating parity? Parity Violation

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 17 T.D. Lee and C.N. Yang studied all known weak decays and concluded that there were no evidences of parity conservation in weak decays –Postulated that weak interactions violate parity –See, for more interesting readings These turned out to be Parity is conserved in strong and EM interactions but not in weak interactions w/ very little degree of violation Parity Violation

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 18 Invert time from t  - t. How about Newton’s equation of motion? –Invariant under time reversal Time Reversal

Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 19 Conversion of charge from Q  - Q. Under this operation, particles become antiparticles What happens to the Newton’s equation of motion? –Invariant under charge conjugate Charge Conjugate