Inequality for the time evolution of an overlap

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SUMMARY

The discussion focuses on proving that the uncertainty in energy for a normalized quantum state limits the speed at which the state can become orthogonal to itself. The specific problem referenced is number 2 from the MIT OpenCourseWare assignment for Quantum Physics II (Fall 2013). The autocorrelation function, denoted as ##\left<\psi (0)|\psi(t)\right>##, is highlighted as a key concept, particularly in the context of a two-state system spanned by energy eigenstates ##|\psi_1 >## and ##|\psi_2 >##. Participants suggest exploring the dependence of the autocorrelation function on the coefficients ##a## and ##b## of the state vector.

PREREQUISITES
  • Understanding of quantum mechanics concepts, specifically energy eigenstates.
  • Familiarity with autocorrelation functions in quantum systems.
  • Basic knowledge of normalized states in quantum physics.
  • Experience with two-state systems and their mathematical representation.
NEXT STEPS
  • Explore the properties of autocorrelation functions in quantum mechanics.
  • Investigate the implications of energy uncertainty on state evolution.
  • Learn about the mathematical representation of two-state systems in quantum physics.
  • Study the relationship between coefficients in quantum state superpositions and their impact on orthogonality.
USEFUL FOR

Students and researchers in quantum mechanics, particularly those studying state evolution and energy uncertainty, as well as educators seeking to enhance their understanding of quantum state interactions.

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You should post this in the Homework forum, using the correct question template.

The function ##\left<\psi (0)|\psi(t)\right>## is called an autocorrelation function. You could start by playing with a two-state system where the state space is spanned by only two vectors, and finding out how the autocorrelation function of ##a|\psi_1 > + b|\psi_2 >## depends on how similar in absolute value the coefficients ##a,b## are. ##|\psi_1 >## and ##|\psi_2 >## are the energy eigenstates here.
 

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