sum rules in non-relativistic quantum mechanics: a ... · sum rules in non-relativistic quantum...
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Sum rules in non-relativistic quantum mechanics: A pedagogical tutorial
R. W. Robinett (Penn State University)
(M. Belloni – Davidson College)
Foundations of Nonlinear Optics Tuesday, August 9th, 2016
Tufts University
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Background/reference papers (all in the conference file)
• M. Belloni and RWR, ``Quantum mechanical sum rules for two (three) model systems’’, Am. J. Phys. 76, 798-806 (2008).
• M. Belloni and RWR, ``The infinite well and Dirac delta function potentials as pedagogical, mathematical, and physical models in quantum mechanics’’, Phys. Rep. 540, 25-122 (2014).
• M. Belloni and RWR, ``Less than perfect quantum wavefunctions in momentum-space: How φ(p) senses disturbances in the force”, Am. J. Phys. 79, 94-102 (2011).
• M. Belloni and RWR, ``Supersymmetric extensions of the infinite square well: Quantum wave functions and applications to energy-weighted sum rules”, (in preparation) – Thanks to the organizers for the push to finish this!
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Overview/outline of topics • A different (non sum rule) pedagogical example
– φ(p) at large |p| in 1D • Derivations of sum rules • 1D examples of how they ‘work’ (checking them)
1. Harmonic oscillator 2. Infinite square well (ISW) 3. Single δ-function
• Sum rules in (almost) iso-spectral quantum systems – How energy-weighted sum rules ‘work’ in
supersymmetric extension(s) of the ISW
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Momentum-space wave functions - ø(p)
• Pedagogical use, for semi-classical connections
ISW Harmonic oscillator Either ψn(x) or φn(p)
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Measuring φ(p) (for large p) for reals! Power-law behavior for ‘spikey’ potentials
• Hydrogen atom
• Short-range (δ) interactions
D. Jin et al. group
E. Weigold, Am. J. Phys. 51, 152-152 (1983) A real “thought” experiment for the hydrogen atom
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“Obi-Wan Kenobi Theorem”
• If…
• …then
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• k = -1 – infinite potential (ISW/δ-function) - 1/p2
• k = 0 – discontinuous potential (finite well) - 1/p3
• k = +1 – potential with cusp (‘V’ potential) - 1/p4 • ... • Harmonic oscillator – perfectly behaved !
• Not power-law behavior – e-p^2
• Why do we even care about this for sum rules? – Convergence of the sums (steepest descent ideas)
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Quantum mechanical sum rules • What do students need to know to derive sum rules?
– Complete set of states – OK to multiply by ① anywhere – Commutation relations
• Good references
– Bethe and Jackiw, Intermediate Quantum Mechanics – R. Jackiw, Phys. Rev. D 157, 1220-1225 (1967) – Belloni and RWR, AJP, 76, 798-806 (2008)
• Derivations most often relegated to ‘end-of-chapter’
problems
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Just completeness first
• First of the Bethe-Jackiw dipole moment sum rules
Insert ①
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Thomas-Reiche-Kuhn (TRK) sum rule: Start using commutators
Insert ① twice!
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Historically important!
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Lots of dipole moment sum rules with different powers of (Ek-En)
1. Closure
2. TRK
3. ‘Energy’
4. ‘Force times
momentum’
5. ‘Force squared’
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And another energy-difference weighted quantity
• 2nd order perturbation theory result
• for Stark effect (or any linear potential, V(x) = Fx)
• …has the same format, but with energy differences
on the bottom – so same ‘math tricks’ should work
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Even more sum rules
• Monopole
• Bethe-Bloch
• Wang* general result (TRK case using F(x) = x) * S. Wang, Phys. Rev. A 60, 262-266 (1999)
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Pedagogical uses • Deriving sum rules (QM formalism)
• Checking/confirming identities for familiar model
cases (math formalism) 1. Harmonic oscillator 2. Infinite square well 3. Single δ-function
• Math methods (‘tricks’) for evaluating the sums (integrals) that appear
• How do the convergence properties of these sums relate to φ(p) and the ‘smoothness’ of the original ψ(x) and potential V(x)
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Harmonic oscillator example • V(x) = mω2 x2/2 and En = (n+1/2)ħω and wave
functions well-known • Dipole (or any xp) matrix elements, <n|xp|k>,
can be obtained by using 1. identities for integrals over Hermite polynomials, 2. raising/lowering operators (much nicer!)
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• Dipole matrix elements are easy to evaluate
• So the infinite sums are actually finite sums and
the series are ‘super-convergent’ • The TRK sum rule is trivial to verify for the SHO
SHO example (cont’d)
Φ(p) ~ e-p^2 !
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Stark effect (linear potential) for the SHO
• 2nd order shift
• which is actually a classical result since
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Infinite square well (ISW) (The workhorse, not showhorse, of QM)
• Convergence properties? Now it matters! • <n|x|k> ~ 1/k3 ,while ΔE ~ k2 for large k • The first three sum rules converge (as they must!)
but the rest do not
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How to do the resulting sums • The TRK sum rule is given by • …with similar expressions for other (convergent)
sum rules • One ‘basic’ trick allows you to evaluate all such
sums and confirm the identities
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Stark effect for the ISW
• Shift to ground state (n=1) energy is negative • Shifts to all other states (n>1) are positive! • Agrees with ‘Dalgarno-Lewis’ method calculations • Consistent with WKB ‘guess’ for power-law
potentials - Vk(x) = |x/a|k giving αn ~ n 2(2-k)/(2+k)
Same math tricks!
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Single δ-function – the continuum matters!
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Single δ-function (cont’d) • Matrix elements go like 1/k3 while ΔE goes like k2, so
again the first three sum rules converge • Same φ(p) behavior (1/p2, via the OWK theorem) as
well as matrix elements as ISW • The TRK (and all other convergent) sum rules require
integrals – use contour integration - math trick!
• The 2nd order Stark shift also works (Dalgarno-Lewis method or solving the problem with Airy functions)
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Exploring energy weighted sum rules What role do the energies play?
• Each sum rule is an infinite set of constraints
• The energy differences are like the ‘rows’ in a tapestry
• The matrix elements (dynamics) are like the columns
• Can we have two systems with the same energies, but different dynamics?
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Sum rules in isospectral systems • Supersymmetry allows you to generate pairs
of potentials with (almost) the same energy spectra
• Uses just raising and lowering operators The SUSY version of the SHO is the SHO!
Familiar 1D state -> Supersymmetric version V(-)(x) -> V(+)(x)
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The SUSY version of the ISW
You can generate all of the new
ψn(x) and øn(p)
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Super-ISW • For the Super-ISW, because of the smoother walls
– Ψn(x) → x2 as x → 0 – due to an “angular momentum barrier”
– Φn (p) → 1/p3 as p→∞ (Obi-Wan Kenobi theorem) – <n|x|k> → 1/k4 as k gets large, so all sums converge
faster and one additional sum rule is convergent
Blue – ISW Red = SUSY version
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Super(symmetrize) me (again and again and again…..)
• You can repeatedly super-symmetrize the ISW*
• Note the “angular momentum” like S(S+1) factor • Increasingly ‘smooth’ wave functions at the
boundaries with ψn(x) → x(1+S)
• With φn(p) → 1/p(2+S) and matrix elements which converge faster and more sum rules converge
* A. Khare, AIP Conference Proceedings 744, 133 (2004)
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Conclusions (and apologies!) • I talked way too long! • Sum rules are a great ‘quantum playground’
for many types of QM formalism • There are an infinite number of ‘parallel
universe’ playgrounds due to SUSY (ISWS!)
• Thanks again for the motivation to work on this new problem!