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Variational Method in Quantum Mechanics

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Table of Contents

  1. Introduction
  2. Motivation and Importance
  3. The Variational Principle
  4. Statement of the Theorem
  5. Constructing a Trial Wavefunction
  6. Applying the Variational Method
  7. Example: Ground State of the Hydrogen Atom
  8. Example: Helium Atom Approximation
  9. Rayleigh-Ritz Variational Method
  10. Choosing Good Trial Functions
  11. Variational Bounds and Limits
  12. Variational Method in Quantum Field Theory
  13. Applications in Quantum Chemistry
  14. Limitations of the Method
  15. Conclusion

1. Introduction

The variational method is a powerful approximation technique in quantum mechanics used to estimate the ground-state energy of complex systems. It is especially valuable when the Schrรถdinger equation cannot be solved exactly, such as for many-electron atoms and molecules.


2. Motivation and Importance

Exact solutions are rare in quantum mechanics. For most real-world systems, including atoms with more than one electron, molecules, and solids, analytical solutions are impossible. The variational method provides a way to estimate energies by optimizing trial wavefunctions, making it an essential tool in theoretical and computational physics.


3. The Variational Principle

The core of the method is the variational principle, which states:

For any normalized trial wavefunction \( |\psi_{\text{trial}}\rangle \), the expectation value of the Hamiltonian provides an upper bound to the ground-state energy \( E_0 \):

\[
E_0 \leq \langle \psi_{\text{trial}} | \hat{H} | \psi_{\text{trial}} \rangle
\]

Equality holds only if \( |\psi_{\text{trial}}\rangle \) is the true ground-state wavefunction.


4. Statement of the Theorem

Let \( \hat{H} \) be a Hermitian Hamiltonian and \( |\psi_{\text{trial}}\rangle \) a normalized state:

\[
\langle \psi_{\text{trial}} | \psi_{\text{trial}} \rangle = 1
\]

Then:

\[
E[\psi_{\text{trial}}] = \langle \psi_{\text{trial}} | \hat{H} | \psi_{\text{trial}} \rangle \geq E_0
\]

This principle holds because any non-exact wavefunction has contributions from excited states that increase the energy.


5. Constructing a Trial Wavefunction

Key considerations:

  • Must satisfy the same boundary conditions and symmetries as the true wavefunction.
  • Should include variational parameters to allow optimization.
  • Simpler functions often yield good estimates with minimal effort.

6. Applying the Variational Method

Steps:

  1. Choose a trial wavefunction \( \psi(\vec{r}; \alpha_1, \alpha_2, โ€ฆ) \).
  2. Compute the energy functional:

\[
E[\psi] = \frac{\langle \psi | \hat{H} | \psi \rangle}{\langle \psi | \psi \rangle}
\]

  1. Minimize \( E[\psi] \) with respect to the parameters \( \alpha_i \).

7. Example: Ground State of the Hydrogen Atom

Use trial wavefunction:

\[
\psi(r) = A e^{-\alpha r}
\]

where \( \alpha \) is a variational parameter. Evaluate:

\[
E(\alpha) = \frac{\int \psi^* \hat{H} \psi \, d^3r}{\int |\psi|^2 \, d^3r}
\]

and minimize with respect to \( \alpha \). The result is close to the true ground state energy \( -13.6 \, \text{eV} \).


8. Example: Helium Atom Approximation

For helium, exact solutions are not possible. Use a trial wavefunction:

\[
\psi(r_1, r_2) = e^{-\alpha r_1} e^{-\alpha r_2}
\]

Minimize the total energy with respect to \( \alpha \), accounting for electron-electron repulsion. This gives a very good estimate of the ground state energy.


9. Rayleigh-Ritz Variational Method

This method generalizes the variational principle:

  • Expand the trial function in terms of basis functions:

\[
\psi = \sum_n c_n \phi_n
\]

  • Construct the matrix:

\[
H_{mn} = \langle \phi_m | \hat{H} | \phi_n \rangle
\]

Solve the resulting eigenvalue problem to find optimal energies and coefficients.


10. Choosing Good Trial Functions

Tips for selecting effective trial wavefunctions:

  • Include the correct asymptotic behavior.
  • Incorporate physical intuition (e.g., shielding, correlation).
  • Start simple and refine iteratively.
  • Use known solutions as basis functions (e.g., hydrogenic orbitals).

11. Variational Bounds and Limits

  • The variational estimate is always an upper bound.
  • The tighter the bound, the closer the trial function is to the true wavefunction.
  • Provides error estimates and confidence in approximations.

12. Variational Method in Quantum Field Theory

The variational method extends beyond non-relativistic quantum mechanics:

  • Used in quantum field theory to study vacuum structure.
  • Variational ansatz functions describe vacuum fluctuations and condensates.

13. Applications in Quantum Chemistry

  • Used in Hartree-Fock theory and configuration interaction methods.
  • Central to density functional theory (DFT).
  • Helps compute molecular orbitals, binding energies, and spectra.

14. Limitations of the Method

  • Only gives ground-state estimates (not excited states unless modified).
  • Highly dependent on the choice of trial function.
  • Optimization can become numerically intensive with many parameters.
  • May converge to a local minimum instead of the global one.

15. Conclusion

The variational method is an elegant and practical approximation tool in quantum mechanics. It provides accurate estimates for ground-state energies and insights into wavefunction structures. Its wide applicability in atomic, molecular, and condensed matter physics underscores its foundational importance. With thoughtful choice of trial functions and rigorous optimization, the variational method remains indispensable in modern theoretical physics.


Today in History – 12 August

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today in history 12 august

30

Cleopatra, queen of Egypt and lover of Julius Caesar and Mark Antony, took her life following the defeat of her forces against Octavian, the future first emperor of Rome.

1602

Abul Fazal, Akbar‘s minister, was killed on the instructions of Jahangir.

1868

Frederick JNT Lord Chelmsford, Viceroy of British-India (1916-21), was born.

1898

The brief and one-sided Spanish-American War came to an end when Spain formally agreed to a peace protocol on U.S. terms: the cession of Cuba, Puerto Rico, and Manila in the Philippines to the United States pending a final peace treaty.

1914

A week after Britain declared war on Germany and entered the First World War, the British Parliament passed the Defense of the Realm Act, aimed at providing the British government with the means to support the countryโ€™s war effort.

1919

Dr. Vikram Ambalal Sarabhai, the father of Indian space technology and scientist, was born at Ahmedabad.

1928

The Olympic Games hosted by Amsterdam fully realized Pierre de Coubertin’s vision: ‘the nations of the world in friendly competition’. After a succession of Olympics dominated by North America and Western Europe, Amsterdam welcomed more than 3,000 competitors.

1946

Viceroy announced invitation to Congress to form provisional Government.

1953

Less than one year after the United States tested its first hydrogen bomb, the Soviets detonate a 400-kiloton device in Kazakhstan. The explosive power was 30 times that of the U.S. atomic bomb dropped on Hiroshima, and the mushroom cloud produced by it stretched five miles into the sky. Known as the โ€œLayer Cake,โ€ the bomb was fueled by layers of uranium and lithium deuteride, a hydrogen isotope. The Soviet bomb was smaller and more portable than the American hydrogen bomb, so its development once again upped the ante in the dangerous nuclear arms race between the Cold War superpowers.

1961

In an effort to stem the tide of refugees attempting to leave East Berlin, the communist government of East Germany begins building the Berlin Wall to divide East and West Berlin. Construction of the wall caused a short-term crisis in U.S.-Soviet bloc relations, and the wall itself came to symbolize the Cold War.

1964

On August 12, 1964, Charlie Wilson, part of the gang who pulled off the 1963 Great Train Robbery, one of the biggest heists of its kind, escaped from Winson Green Prison in Birmingham, England.

1990

On this day in 1990, fossil hunter Susan Hendrickson discoverd three huge bones jutting out of a cliff near Faith, South Dakota. They turn out to be part of the largest-ever Tyrannosaurus rex skeleton ever discovered, a 65 million-year-old specimen dubbed Sue, after its discoverer.

1991

Parliament passed the Terrorist and Disruptive Activities (prevention) amendment bill.

1997

Bar Council of India debars full-time law teachers from practising as lawyers.

1997

Gulshan Kumar of Super Cassette Industries was shot dead by four unidentified persons in north-west Mumbai.

2000

Neelam Jaswant Singh heaves the discus to a National mark (59.53m) in the Travancore National circuit athletics meet in Thiurvananthapuram.

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Fermiโ€™s Golden Rule in Quantum Mechanics

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fermi golden rule

Table of Contents

  1. Introduction
  2. Historical Background and Significance
  3. Motivation for the Rule
  4. Derivation from Time-Dependent Perturbation Theory
  5. Mathematical Expression
  6. Transition Rate and Density of States
  7. Physical Interpretation
  8. Validity Conditions
  9. Example: Spontaneous Emission of a Photon
  10. Example: Particle Scattering in a Potential
  11. Comparison with Classical Rates
  12. Applications in Atomic, Nuclear, and Condensed Matter Physics
  13. Limitations and Cautions
  14. Variants and Extensions
  15. Conclusion

1. Introduction

Fermi’s Golden Rule provides a formula for computing the transition rate between quantum states under the influence of a weak time-dependent perturbation. It is one of the most widely used results in quantum physics, particularly in atomic transitions, scattering theory, and decay processes.


2. Historical Background and Significance

Enrico Fermi developed this rule in the 1930s while analyzing beta decay. It helped bridge quantum theory with measurable decay rates and laid the foundation for the quantum theory of radioactive processes. Today, it is indispensable in both theoretical derivations and experimental calculations.


3. Motivation for the Rule

When a system is exposed to a weak perturbation, it may transition from an initial quantum state \( |i\rangle \) to a final state \( |f\rangle \). The goal is to compute the transition probability per unit time (i.e., rate) for this process, particularly when the final states form a continuum.


4. Derivation from Time-Dependent Perturbation Theory

Assume a perturbing Hamiltonian of the form:

\[
\hat{H}(t) = \hat{H}_0 + \lambda \hat{H}'(t)
\]

Let \( \hat{H}'(t) = \hat{V} e^{-i\omega t} + \hat{V}^\dagger e^{i\omega t} \), and suppose \( \hat{H}'(t) \) couples the initial and final states. From first-order time-dependent perturbation theory, the transition amplitude is:

\[
c_f(t) = \frac{1}{i\hbar} \int_0^t \langle f | \hat{H}'(t’) | i \rangle e^{i\omega_{fi} t’} dt’
\]

The probability is then:

\[
P_{i \to f}(t) = |c_f(t)|^2
\]


5. Mathematical Expression

Fermiโ€™s Golden Rule gives the transition rate \( \Gamma \) as:

\[
\Gamma_{i \to f} = \frac{2\pi}{\hbar} |\langle f | \hat{H}’ | i \rangle|^2 \rho(E_f)
\]

Where:

  • \( \Gamma_{i \to f} \): Transition probability per unit time.
  • \( \langle f | \hat{H}’ | i \rangle \): Matrix element of the perturbation.
  • \( \rho(E_f) \): Density of final states at energy \( E_f \).

6. Transition Rate and Density of States

The density of states \( \rho(E) \) measures how many quantum states exist per unit energy near a given energy level. In systems where the final states form a continuum, this density is essential to compute the transition rate:

\[
\rho(E) = \frac{dn}{dE}
\]


7. Physical Interpretation

  • The transition rate is proportional to the square of the coupling strength between initial and final states.
  • It is also proportional to the number of available final states.
  • Intuitively, stronger interactions and more available final states result in higher transition probabilities.

8. Validity Conditions

Fermiโ€™s Golden Rule applies under the following conditions:

  • The perturbation is weak.
  • The perturbation is time-independent or slowly varying.
  • The final state is part of a quasi-continuum.
  • The interaction time is long enough for energy conservation to emerge via the delta function \( \delta(E_f – E_i – \hbar\omega) \).

9. Example: Spontaneous Emission of a Photon

An excited atom decays to a lower energy level and emits a photon. Fermiโ€™s Golden Rule yields the spontaneous emission rate:

\[
\Gamma = \frac{2\pi}{\hbar} |\langle f | \hat{d} \cdot \vec{E} | i \rangle|^2 \rho(\omega)
\]

Where \( \hat{d} \) is the dipole operator and \( \vec{E} \) is the electric field mode.


10. Example: Particle Scattering in a Potential

A particle incident on a scattering center may be deflected. The potential acts as a perturbation \( \hat{H}’ = V(\vec{r}) \). Fermi’s Golden Rule computes the differential cross-section by integrating over all final momenta.


11. Comparison with Classical Rates

Unlike classical physics, which may assume deterministic transitions, quantum rates depend on probability amplitudes and the interference of different quantum paths. Fermiโ€™s Golden Rule quantifies these inherently probabilistic effects.


12. Applications in Atomic, Nuclear, and Condensed Matter Physics

  • Atomic transitions (optical and microwave frequencies).
  • Nuclear decay rates.
  • Semiconductor band transitions.
  • Phonon emission and absorption in solids.
  • Quantum tunneling rates and ionization processes.

13. Limitations and Cautions

  • Not valid for short times or strong perturbations.
  • Assumes non-degenerate initial states unless modified.
  • Energy conservation is enforced statistically over time, not instantaneously.
  • Corrections needed for resonant or divergent behaviors.

14. Variants and Extensions

  • Golden Rule for degenerate states.
  • Time-dependent generalizations for pulsed interactions.
  • Extensions in many-body and field-theoretic contexts (e.g., Fermi’s Golden Rule in QED).

15. Conclusion

Fermiโ€™s Golden Rule is a cornerstone of quantum transition rate calculations. By linking microscopic interaction strengths with macroscopic transition probabilities, it serves as a bridge between quantum dynamics and observable decay and scattering phenomena. Mastery of this concept is essential for physicists across all specializations of quantum theory.


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Today in History – 11 August

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today in history 11 august

today in history 11 august

1347

Allau’d-din Hasan Gangu alias Jafar Khan. The Muslim kingdom of Bahmani dynasty in the south as Sultan Allau’d-din Khalji. He renamed Gulbarga, his capital as ‘Hasanabad’.

1856

A hurricane hits the Louisiana coast, killed more than 400 people. Isle Derniere, a resort community, was totally submerged by the storm surges.

1893

First Hindu-Muslim riots in Maharashtra.

1908

Khudiram Bose was hanged on this day in Central Jail at Mujaffarpur, Bihar at the age of 19 years. He along with Prafulla Chaki had planned to bomb the carriage supposed to be carrying Kingsford, unfortunately he was betrayed and was caught and finally was sentenced to death and hanged. This day is observed as “Martyr’s Day” in memory of the great freedom fighter. Even today the soul stirring songs composed in his honour are sung by Bengali folk-singer.

1919

Friedrich Ebert, a member of the Social Democratic Party and the provisional president of the German Reichstag (government), signed a new constitution, known as the Weimar Constitution, into law, officially creating the first parliamentary democracy in Germany.

1943

On this day in 1943, German forces began a six-day evacuation of the Italian island of Sicily, having been beaten back by the Allies, who invaded the island in July.

1956

The Lok Sabha passed the States Reorganisation Act.

1961

Dadra and Nagar Haweli declared as Union Territory States.

1973

Like any style of music, hip hop has roots in other forms, and its evolution was shaped by many different artists, but thereโ€™s a case to be made that it came to life precisely on this day in 1973, at a birthday party in the recreation room of an apartment building in the west Bronx, New York City. The location of that birthplace was 1520 Sedgwick Avenue, and the man who presided over that historic party was the birthday girlโ€™s brother, Clive Campbellโ€”better known to history as DJ Kool Herc, founding father of hip hop.

1984

A small cloud of toxic chemicals escaped from a Union Carbide plant near Charleston, West Virginia, this morning, and at least 135 residents were treated for eye, throat, and lung irritation. Last December, methyl isocyanate gas escaped from a Union Carbide plant in India, killing 2,000 people. No MIC escaped today, plant officials said. Aldicarb oxime, a much less toxic gas, is declared as one constituent of the gas cloud.

1999

The last total solar eclipse of the millenium was seen in northern parts of India and France. This eclipse lasted for 2 min and 23 sec.

2000

Koneru Humpy was crowned the youngest British Ladies chess champion at the end of eleventh and final round in the Smith and Williamson British chess championship in Somerset.

2000

The World Bank signed an agreement for a $713 million aid to India for three infrastructure projects.

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Time-Dependent Perturbation Theory in Quantum Mechanics

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time dependent perturbation

Table of Contents

  1. Introduction
  2. Motivation and Relevance
  3. General Setup of Time-Dependent Perturbation
  4. The Interaction Picture
  5. First-Order Time-Dependent Perturbation Theory
  6. Transition Probabilities
  7. Fermiโ€™s Golden Rule
  8. Periodic Perturbations and Resonance
  9. Example: Two-Level Atom in an Oscillating Field
  10. Sudden and Adiabatic Perturbations
  11. Transition Amplitudes and Matrix Elements
  12. Harmonic Perturbations and Selection Rules
  13. Applications in Quantum Optics
  14. Limitations and Cautions
  15. Conclusion

1. Introduction

Time-dependent perturbation theory is used in quantum mechanics to study how a quantum system evolves when its Hamiltonian changes with time. While time-independent perturbation theory handles stationary systems, many important physical phenomena involve time-varying interactions, such as electromagnetic fields or sudden kicks.


2. Motivation and Relevance

This theory is crucial for understanding:

  • Absorption and emission of light.
  • Atomic transitions and decay processes.
  • Response to external fields in quantum optics.
  • Particle scattering and time-dependent forces.

3. General Setup of Time-Dependent Perturbation

We split the Hamiltonian as:

\[
\hat{H}(t) = \hat{H}_0 + \hat{H}'(t)
\]

where:

  • \( \hat{H}_0 \): Time-independent part with known solutions.
  • \( \hat{H}'(t) \): Time-dependent perturbation, assumed small.

We expand the wavefunction in the eigenbasis of \( \hat{H}_0 \):

\[
|\psi(t)\rangle = \sum_n c_n(t) e^{-i E_n t/\hbar} |n\rangle
\]


4. The Interaction Picture

To simplify calculations, we use the interaction picture, where operators evolve like in the Heisenberg picture but states evolve under the perturbation:

\[
i\hbar \frac{d}{dt} |\psi_I(t)\rangle = \hat{H}’_I(t) |\psi_I(t)\rangle
\]

with:

\[
\hat{H}’_I(t) = e^{i\hat{H}_0 t/\hbar} \hat{H}'(t) e^{-i\hat{H}_0 t/\hbar}
\]


5. First-Order Time-Dependent Perturbation Theory

We solve the differential equation perturbatively. The first-order transition amplitude from state \( |i\rangle \) to \( |f\rangle \) is:

\[
c_f^{(1)}(t) = \frac{1}{i\hbar} \int_{0}^{t} \langle f | \hat{H}'(t’) | i \rangle e^{i\omega_{fi} t’} dt’
\]

Where \( \omega_{fi} = (E_f – E_i)/\hbar \).


6. Transition Probabilities

The probability of transitioning from \( |i\rangle \) to \( |f\rangle \) is:

\[
P_{i \rightarrow f}(t) = |c_f^{(1)}(t)|^2
\]

This gives us measurable quantities like decay rates and absorption strengths.


7. Fermiโ€™s Golden Rule

For perturbations that are constant in time or turned on suddenly, and observed over long times:

\[
P_{i \rightarrow f}(t) \approx \frac{2\pi}{\hbar} |\langle f | \hat{H}’ | i \rangle|^2 \rho(E_f)
\]

Here \( \rho(E_f) \) is the density of final states. This rule is crucial in particle and nuclear physics.


8. Periodic Perturbations and Resonance

For oscillatory perturbations:

\[
\hat{H}'(t) = \hat{V} \cos(\omega t)
\]

Transitions are enhanced (resonant) when:

\[
\hbar \omega = E_f – E_i
\]

This underpins spectroscopy, lasers, and resonance phenomena in quantum systems.


9. Example: Two-Level Atom in an Oscillating Field

A system with two states \( |g\rangle \) and \( |e\rangle \), interacting with an external electric field:

\[
\hat{H}'(t) = \hbar \Omega \cos(\omega t)(|g\rangle \langle e| + |e\rangle \langle g|)
\]

Time-dependent perturbation theory predicts Rabi oscillations and transition probabilities dependent on detuning and field strength.


10. Sudden and Adiabatic Perturbations

  • Sudden: Perturbation changes faster than the system’s natural time scale. The wavefunction remains unchanged but expands in the new eigenbasis.
  • Adiabatic: Perturbation changes slowly, and the system adapts continuously, staying in the instantaneous eigenstate.

These are limits used in both analytic calculations and quantum control.


11. Transition Amplitudes and Matrix Elements

The core quantity is:

\[
\langle f | \hat{H}'(t) | i \rangle
\]

which determines how “connected” the initial and final states are. Strong matrix elements lead to high transition rates.


12. Harmonic Perturbations and Selection Rules

Perturbations like:

\[
\hat{H}'(t) = q E_0 x \cos(\omega t)
\]

lead to dipole transitions. The selection rules are derived from symmetry and parity considerations. E.g., \( \Delta \ell = \pm 1 \), \( \Delta m = 0, \pm 1 \) in atoms.


13. Applications in Quantum Optics

  • Stimulated emission and absorption.
  • Laser physics and coherent control.
  • Photon-atom interaction in cavity QED.
  • Nuclear magnetic resonance (NMR) and electron spin resonance (ESR).

14. Limitations and Cautions

  • Assumes perturbation is small compared to level spacing.
  • Higher-order effects can be significant in strong fields.
  • Breakdown near level crossings and avoided crossings.
  • Doesnโ€™t account for dissipation or decoherence unless extended.

15. Conclusion

Time-dependent perturbation theory is a foundational tool in quantum mechanics that allows physicists to analyze transitions between quantum states under external influences. From understanding atomic spectra to designing quantum control protocols, it plays a central role in both theoretical and experimental quantum science.


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