4e the quantum universe
play

4E : The Quantum Universe Lecture 29, May 24 Vivek Sharma - PowerPoint PPT Presentation

4E : The Quantum Universe Lecture 29, May 24 Vivek Sharma modphys@hepmail.ucsd.edu 2 Zeeman Effect Due to Presence of External B field Energy Degeneracy Is Broken Electron has Spin: An additional degree of freedom Electron possesses


  1. 4E : The Quantum Universe Lecture 29, May 24 Vivek Sharma modphys@hepmail.ucsd.edu

  2. 2 Zeeman Effect Due to Presence of External B field Energy Degeneracy Is Broken

  3. Electron has “Spin”: An additional degree of freedom Electron possesses additional "hidden" degree � of freedom : " Spinning around itself" ! s s + � |S| = ( 1) 1 s = Spin Quantum # (either Up or Down) 2 ⇒ How do we know this ? Stern-Gerlach expt � Spin Vector (a form of a n gu l ar momentum) S is also Quantized � 3 + = � � |S| = ( 1) s s 4 1 = = ± � & S ; m m z s s 2 Spinning electron is an en titity defying any simple Spin angular momentum S classical description. . ... dd hi e n D.O. F also exhibits Space quantization 3

  4. Stern-Gerlach Expt ⇒ An additional degree of freedom: “Spin” In an inhomogeneous field perpendicular to beam direction, magnetic moment µ experiences a force F z whose direction depends on Z component of the net magnetic moment & inhomogeneity dB/dz. The force deflects magnetic moment up or down. Space Quantization means expect (2 l + 1) deflections. For l =0, expect all electrons to arrive on the screen at the center (no deflection) � � � µ in inhomogenous B field, experiences force F � � � ∇ = −∇ − µ F= - U ( .B) B ∂ ∂ ∂ B B B ≠ = = When gradient only along z, 0; 0 ∂ ∂ ∂ z x y ∂ B = µ ( ) moves particle up or down F m ∂ z B z � µ (in addition to torque causing magnetic m o me n t to precess about B field direction 4

  5. An Additional degree of freedom: “Spin” for lack of a better name ! Expected Observed ! Hydrogen or l = 1 Silver ( l =0) This was a big surprise for Stern-Gerlach ! They had accidentally Discovered a new degree of freedom for electron : “spin” which Can take only two orientations for angular momentum S : up or down Leads to a new quantum number s=1/2. As a result: = � Z Component of Spin Angular Momentum S m z s = + � The magnitude | | ( 1) is FIXED, never changes ! S s s + = Allowed orientations are ( 1) 2 s s � � ⇒ µ S ; The corresponding Spin Magnetic Moment S 5

  6. What Stern&Gerlach Saw in l=0 Silver Atoms B Field On ! B Field off Picture changes instantaneously as the external Field is switched off or on….discovery ! 6

  7. Four (not 3) Numbers Describe Hydrogen Atom � n,l,m l ,m s � µ "Spinning" charge gives rise to a dipole moment : s ∆ q Imagine (semi-clasically , in correctl y ! ) electron as s phere : charge q, radius r ∑ ∆ Total charg e uniformly dist ribut ed : q= q ; i i � ⇒ ⇒ µ a s electron spins, each "chargelet" rotates current dipole moment s i � ⎛ ⎞ ⎛ ⎞ � � q q ∑ µ = µ = = ⎜ ⎟ ⎜ ⎟ ; 2 g S g s s ⎝ 2 ⎠ ⎝ 2 ⎠ m i m i e e � � � ⇒ = µ In a Magnetic Field B magnetic energy due to s pin U . B S s � � � Net Angular Momentum in H Atom J = L + S � � ⎛ ⎞ − � � � e µ = µ + µ = + Net Magnetic Moment of H atom : ⎜ ⎟ ( ) L gS 0 s ⎝ 2 ⎠ m e � � µ � Notice that since g=2, net dipole moment vector is not to J (There are many such "ubiq t ui ous" quantum numbers for elementary particles!) 7

  8. Magnetic Energy in an External B Field Contributions from Orbital and Spin motions. Defining Z axis to be the orientation of the B field: � � � e e { } { } µ = + = + U=- . B B L gS B m gm z z l s 2 2 m m Example: Zeeman spectrum in B=1T produced by Hyd rogen initially in n=2 state ⇒ = − = − 2 after taking spin into account: n=2 E 13.6 / 2 3.40 eV eV 2 = ± = m ω � Since m 0, 1, orbital contribution to Magnetic energy U l 0 l L ± ω = ± � This splits energy levels to E=E ; for m 1 sta tes 2 l L These states get further split in pairs due to spin magnetic moment 1 = ± ω � Since g=2 and m ; spin energy is again Zeeman energy= s L 2 As a result electrons in this shell have one of the following energi e s ± ω ± ω � � E E E 2 2 2 2 L L ∆ ± This leads to a variety of allowed ( (m +m )=0, 1) energy transitions with different l s intensities (Principal an d satellites) which a re vi sible when B field is large (ignore LS coupling See energy level diagram on next page 8

  9. Doubling of Energy Levels Due to Spin Quantum Number Under Intense B field, each {n , m l } energy level splits into two depending on spin up or down In Presence of External B field 9

  10. Spin-Orbit Interaction: L and S Momenta are Linked Magnetically B B B -e +Ze Equivalent to -e +Ze Electron revolving around Nucleus finds itself in a "internal" B field because in its frame of reference, the nucleus is orbiting around it � µ This B field, due to orbital motion , interacts with electron's spin dipole moment s � � � � = − µ ⇒ . Energy larger when S || B, smaller when anti-paralle l U B m � ⇒ ⇒ States with same ( , , ) but diff. spins e e n rg y level splitting/doubling due to S n l m l 10

  11. Spin-Orbit Interaction: Angular Momenta are Linked Magnetically B B B -e +Ze Equivalent to -e +Ze � µ This B field, due to orbital motion , interacts with electron's spin dipole moment s � � � � = − µ ⇒ . Energy larger when S || B, smaller when anti-paralle l U B m � ⇒ ⇒ States with same ( , , ) but diff. spins e e n rg y level splitting/doubling due to S n l m l Under No External B Field There is Sodium Doublet Still a Splitting! & LS coupling 11

  12. 12 Vector Model For Total Angular Momentum J j 3/2 2P n

  13. Vector Model For Total Angular Momentum J ⇒ Coupling of Orbital & Spin magnetic moments Neither Orbital nor Spin angular Momentum are conserved seperately! � � � J = L + S is conserv e d so long as there are no ex ternal torque s pr esen t Rules for Tota l Angular Momentum Quanti zat ion : = + = + + + � | | ( 1) w ith | |, -1, - 2......,... .,| - | J j j j l s l s l s l s = = � J with , -1, - 2.. ....., - m m j j j j z j j 1 = = Example: state with ( 1, ) l s 2 = ⇒ − 3/ 2 = -3/ 2, 1/ 2,1/ 2,3/ 2 j m j ⇒ ± j = 1/ 2 = 1/ 2 m j + In general takes (2 1) values m j j ⇒ Even # of or ientations 13

  14. Addition of Orbital and Spin Angular Momenta When l =1, s=1/2; According to Uncertainty Principle, the vectors can lie anywhere on the cones, corresponding to definite values of their z component 14

  15. Complete Description of Hydrogen Atom Full description of the Hydr oge n atom : { , , , } n l m m 2P l s n 3/2 ⇓ j LS Coupling ⇓ { , , , } n l j m How to describe multi-electrons atoms like He, Li etc? s corresponding How to order the Periodic table? 4 D .O F. . to • Four guiding principles: • Indistinguishable particle & Pauli Exclusion Principle •Independent particle model (ignore inter-electron repulsion) •Minimum Energy Principle for atom •Hund’s “rule” for order of filling vacant orbitals in an atom 15

  16. Multi-Electron Atoms : >1 electron in orbit around Nucleus ψ θ φ Θ θ Φ φ ≡ In Hydrogen Atom (r, , )=R(r ). ( ). ( ) { , , , } n l j m j e - In n-electron atom, to simplify, ignore electron-electron inte rac tions complete wavefunction, in "independent"part icle ap prox" : ψ ψ ψ ψ ψ (1,2, 3,..n)= (1). (2). (3)... ( ) ??? n e - → Complication Electrons are identical particles, labeling meanin gless! Question: How many electrons can have same set of quan t um #s? Answer: No two elec trons in an atom can have SAME set of quantum#s (if not, all electrons would occupy 1s state (least energy). .. no struct ure!! Example of Indistinguishability: elec tron-ele ctron scatte ring Small angle scatter large angle scatter If we cant follow electron Quantum Picture path, don’t know between which of the two scattering events actually happened 16

Recommend


More recommend