Perturbations and harmonic oscillator

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SUMMARY

This discussion focuses on the analysis of a diatomic molecule's potential energy function, specifically V(r) = V_0[(r_0/r)^{12} - 2(r_0/r)^{6}]. The participants derive the harmonic oscillator approximation by expanding V(r) around the equilibrium distance r0, leading to the ground state wave function and energy expression E = (3ħ√(2V0/r0²μ)). They also explore the effects of perturbation theory on the ground state energy, incorporating higher-order terms to refine their calculations. The discussion highlights the importance of normalization and integration limits in wave function analysis.

PREREQUISITES
  • Understanding of quantum mechanics, specifically harmonic oscillators
  • Familiarity with perturbation theory in quantum mechanics
  • Knowledge of potential energy functions in molecular physics
  • Proficiency in calculus, particularly integration techniques
NEXT STEPS
  • Study the derivation of the harmonic oscillator wave function in quantum mechanics
  • Learn about higher-order perturbation theory and its applications
  • Investigate the normalization of wave functions in quantum mechanics
  • Explore the implications of potential energy functions on molecular stability
USEFUL FOR

Students and researchers in quantum mechanics, particularly those studying molecular physics, harmonic oscillators, and perturbation theory. This discussion is beneficial for anyone looking to deepen their understanding of diatomic molecular behavior and energy calculations.

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Homework Statement


In a diatomic molecule with atom masses m1 and m2, the atoms are bound by a potential
V(r)=V_0\big[ \big(\frac{r_0}r\big)^{12} - 2\big(\frac{r_0}r\big)^{6}\big]
where r is the distance between the atom centra, r0 is the equilibrium istance, and V0 is a constant depending on the atoms.

1) Expand V(r) in series close to r0 and keep only the term that corresponds to a harmonic oscillator. Find for this case the ground state wave function and the corresponding energy.

2) Keep another term in the series of V(r) that gives a contribution to the ground state energy calculated with first order perturbation theory. Find the new (approximate) energy for this state.


Homework Equations


Wave function for harmonic oscillator, ground state:
\psi_0(x) = \big(\frac{m \omega}{\pi \hbar}\big)^{1/4} e^{-\frac{m \omega}{2\hbar}x^2}

E_0^1 = <\psi_0^0 | H' |\psi_0^0>
where
E_0^1= ground state energy with first order perturbation

\psi_0^0= ground state wave function in unperturbed state

H'= the perturbation

The Attempt at a Solution


Serialize V (I'll drop the ordo-terms):
V(r)= V(r_0)+V'(r_0)(r-r_0) + \frac 12 V''(r_0) (r-r_0)^2
V'(r0)=0 because it's the equilibrium point
V(r0) = constant and can be removed since this doesn't change the force
Conclusion:
V(r) = \frac 12 V''(r_0) (r-r_0)^2
V''(r_0)=\frac{72}{r_0^2}V_0
V(r) = \frac{36}{r_0^2}V_0 (r-r_0)^2 = \alpha (r-r_0)^2
So compared with the harmonic oscillator's
V(x) = \frac 12 \mu \omega^2x^2
I get that
\alpha = \frac {\mu \omega^2}2 \rightarrow \omega = \frac 6r_0 \sqrt{\frac{2V_0}{\mu}} \rightarrow E=\frac 12 \hbar \omega = 3\hbar \sqrt{\frac{2V_0}{r_0^2 \mu}}

So far all good...

The wave function should become
\psi_0(r) = \big( \frac{6\sqrt{2\mu V_0}}{\pi r_0 \hbar}\big)^{1/4} e^{-\frac{3\sqrt{2\mu V_0}}{r_0 \hbar}r^2}
I'm not especially certain about this, because of two reasons:
1) the given wave function under 2 is in x, and has been normalized with an integral from -infinity to infinity. As I'm using r, and it's a distance between two atoms, it should be 0 to infinity the get the correct wavefunction.
2) the given wave function is for an oscillator with r0=0. Is it correct to use r in the exponential function or should it be r-r0?

That was for part 1. Second question:
Serialize like before but keep the third order term...
V'''(r_0) = -\frac{1512}{r_0^3}V_0
V(r) = \frac{36}{r_0^2}V_0 (r-r_0)^2 - 252\frac{V_0}{r_0^3} (r-r_0)^3
Last term will be H' - the perturbation.
E_0^1 = <\psi_0^0 | H' |\psi_0^0> = -252 \frac{V_0}{r_0^3} \big(\frac{6\sqrt{2\mu V_0}}{\pi r_0 \hbar}\big)^{1/4} \int_{-\infty}^\infty e^{- \frac{6\sqrt{2\mu V_0}}{r_0 \hbar}r^2}(r-r_0)^3 dr = 252 V_0 + \frac{63\hbar}{r_0} \sqrt{\frac{V_0}{2\mu}}
Once again I'm confused about the integration limits.

And this is definitely not the correct answer. If I would divide the energy from the first question with the perturbed one, I would get a constant term of 21/4 that is way too great to make sense.
 
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nevermind... I found out where I went wrong.
 

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