Basic Quantum Theory Archives - Time Travel, Quantum Entanglement and Quantum Computing https://stationarystates.com/category/basic-quantum-theory/ Not only is the Universe stranger than we think, it is stranger than we can think...Hiesenberg Tue, 18 Feb 2025 16:25:34 +0000 en-US hourly 1 https://wordpress.org/?v=6.7.2 Convolution Integrals for Entangled Quantum States https://stationarystates.com/basic-quantum-theory/convolution-integrals-for-entangled-quantum-states/?utm_source=rss&utm_medium=rss&utm_campaign=convolution-integrals-for-entangled-quantum-states https://stationarystates.com/basic-quantum-theory/convolution-integrals-for-entangled-quantum-states/#respond Tue, 18 Feb 2025 16:25:34 +0000 https://stationarystates.com/?p=757 Convolution Integrals in Schrödinger’s Equation for Entangled Systems 1. Green’s Functions and Propagators The solution to the time-dependent Schrödinger equation often involves propagators, which describe the evolution of a wavefunction […]

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Convolution Integrals in Schrödinger’s Equation for Entangled Systems

1. Green’s Functions and Propagators

The solution to the time-dependent Schrödinger equation often involves propagators, which describe the evolution of a wavefunction over time. The propagator G(x,t;x',t') is often expressed as a convolution integral:

ψ(x,t) = ∫ G(x,t;x',t') ψ(x',t') dx'

For entangled systems, such as two-particle wavefunctions, the Green’s function method involves convolution-like integrals in both configuration and momentum space.

2. Reduced Density Matrices and Decoherence

For a bipartite quantum system, the reduced density matrix of a subsystem ρ_A(x, x') after tracing out another system B can be written as:

ρ_A(x, x') = ∫ ψ(x, y) ψ*(x', y) dy

where the convolution integral over y (the degrees of freedom of the traced-out system) leads to decoherence effects in entangled systems.

3. Convolution in the Context of Quantum Correlations

Entangled wavefunctions of two particles often involve convolution-type integrals in their evolution. For example, in momentum space:

Ψ(p₁, p₂) = ∫ K(p₁, q₁) K(p₂, q₂) Ψ(q₁, q₂) dq₁ dq₂

where K(p, q) represents a transformation kernel that could come from a propagator or measurement process.

Example: EPR State Evolution

Consider an entangled EPR state in momentum representation:

Ψ(p₁, p₂) = δ(p₁ + p₂)

The time evolution of this state under free-particle Hamiltonians involves convolution integrals with propagators:

Ψ(x₁, x₂, t) = ∫ G(x₁ - x₁', t) G(x₂ - x₂', t) Ψ(x₁', x₂', 0) dx₁' dx₂'

Summary

  • Convolution integrals appear in the propagator formalism, Green’s function methods, and reduced density matrices of entangled systems.
  • They play a crucial role in describing the time evolution, measurement effects, and decoherence of entangled states.
  • Specific cases include the evolution of EPR states and the behavior of correlated two-particle systems.

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Finite Abelian Groups and Applications to Quantum Physics https://stationarystates.com/mathematical-physics/finite-abelian-groups-and-applications-to-quantum-physics/?utm_source=rss&utm_medium=rss&utm_campaign=finite-abelian-groups-and-applications-to-quantum-physics Sat, 11 Jan 2025 03:17:43 +0000 https://stationarystates.com/?p=734 Finite Abelian Groups and Applications to Quantum Physics What Are Finite Abelian Groups? A finite abelian group is a group with the following properties: Closure: For any , . Associativity: […]

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Finite Abelian Groups and Applications to Quantum Physics

What Are Finite Abelian Groups?

A finite abelian group is a group G with the following properties:

  • Closure: For any a, b \in G, a \cdot b \in G.
  • Associativity: For all a, b, c \in G, (a \cdot b) \cdot c = a \cdot (b \cdot c).
  • Identity: There exists an identity element e \in G such that a \cdot e = e \cdot a = a for all a \in G.
  • Inverses: For every a \in G, there exists an a^{-1} \in G such that a \cdot a^{-1} = e.
  • Commutativity: For all a, b \in G, a \cdot b = b \cdot a.

If the group has a finite number of elements, it is called finite.

Structure of Finite Abelian Groups

The Fundamental Theorem of Finite Abelian Groups states that every finite abelian group G can be expressed as a direct product of cyclic groups of prime power order:

    \[ G \cong \mathbb{Z}_{n_1} \times \mathbb{Z}_{n_2} \times \cdots \times \mathbb{Z}_{n_k}, \]

where n_1, n_2, \dots, n_k are integers greater than 1.

Examples of Finite Abelian Groups

  • Cyclic Groups:
    • \mathbb{Z}_n, the integers modulo n under addition.
    • Example: \mathbb{Z}_6 = \{ 0, 1, 2, 3, 4, 5 \} with addition modulo 6.
  • Direct Product of Cyclic Groups:
    • \mathbb{Z}_2 \times \mathbb{Z}_2, the Klein four-group:

          \[ \{(0, 0), (1, 0), (0, 1), (1, 1)\}. \]

    • \mathbb{Z}_2 \times \mathbb{Z}_4:

          \[ \{(0, 0), (1, 0), (0, 1), (1, 1), (0, 2), (1, 2), (0, 3), (1, 3)\}. \]

  • Additive Group of Finite Fields: The set of elements of a finite field \mathbb{F}_q under addition forms a finite abelian group.
  • Root of Unity Groups: The n-th roots of unity \{e^{2\pi i k / n} \mid k = 0, 1, \dots, n-1\} under multiplication.

Applications to Quantum Physics

1. Quantum Mechanics and Symmetry

  • Discrete Symmetries: Finite abelian groups often describe symmetries of quantum systems, such as the Klein four-group \mathbb{Z}_2 \times \mathbb{Z}_2, which can describe symmetries in molecular structures or lattice vibrations.
  • Conservation Laws: The symmetries of a system are associated with conserved quantities, often modeled using finite abelian groups.

2. Quantum Computing

  • Quantum Gates: The structure of finite abelian groups is crucial in algorithms like Shor’s algorithm, where periodicity plays a significant role.
  • Quantum Error Correction: Stabilizer codes, used in error correction, leverage abelian group structures to define subspaces.

3. Topological Phases of Matter

  • Abelian Anyons: Quasiparticles in topological systems exhibit abelian statistics, modeled by finite abelian groups.
  • Fractional Quantum Hall Effect: Finite abelian groups describe the ground state degeneracies and quasiparticle statistics of these systems.

4. Crystallography and Solid-State Physics

  • Lattice Symmetries: Finite abelian groups classify vibrational modes (phonons) and electronic band structures.
  • Bloch’s Theorem: Translational symmetry, often modeled as \mathbb{Z}_n, leads to quantized energy levels in the form of Bloch waves.

Conclusion

Finite abelian groups provide the mathematical foundation for understanding symmetry, periodicity, and conserved quantities in quantum systems. They play a crucial role in quantum computing, error correction, and the study of topological phases of matter, highlighting the deep connections between algebra and the physical world.

 

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Trajectories don’t exist https://stationarystates.com/basic-quantum-theory/trajectories-dont-exist/?utm_source=rss&utm_medium=rss&utm_campaign=trajectories-dont-exist Thu, 02 Jan 2025 04:01:43 +0000 https://stationarystates.com/?p=702 One of Heisenberg’s greatest triumphs was simply eliminating the whole thought process around classical electron trajectories. He claimed that there are only observable quantities – and these quantities can be […]

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One of Heisenberg’s greatest triumphs was simply eliminating the whole thought process around classical electron trajectories.

He claimed that there are only observable quantities – and these quantities can be measured. Nothing more, nothing less. One cannot talk about the ‘path’ in between measurements – because there is no such thing.

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Dipole Approximation in Electron-Photon Interaction https://stationarystates.com/basic-quantum-theory/dipole-approximation-in-electron-photon-interaction/?utm_source=rss&utm_medium=rss&utm_campaign=dipole-approximation-in-electron-photon-interaction Wed, 27 Nov 2024 00:43:12 +0000 https://stationarystates.com/?p=672 Dipole Approximation for Electron-Photon Interaction The dipole approximation assumes that the wavelength of the electromagnetic field is much larger than the spatial extent of the electron wavefunction. In this case, […]

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Dipole Approximation for Electron-Photon Interaction

The dipole approximation assumes that the wavelength of the electromagnetic field is much larger than the spatial extent of the electron wavefunction. In this case, the interaction Hamiltonian simplifies significantly.

Interaction Hamiltonian

In the dipole approximation, the interaction term becomes:

Hint = -d·E(t),

where:

  • d = -er is the electric dipole moment of the electron,
  • E(t) is the electric field of the photon.

Simplified Schrödinger Equation

The time-dependent Schrödinger equation becomes:

iℏ∂ψ/∂t = [H0 - d·E(t)]ψ,

where H0 is the unperturbed Hamiltonian of the electron.

Solving for Energy States

Under the dipole approximation, solutions can be obtained using:

  1. Time-Dependent Perturbation Theory: To calculate transition probabilities between energy levels.
  2. Rabi Oscillations: For resonant interactions between two levels.
  3. Floquet Theory: For periodic electric fields (e.g., in laser interactions).

 

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Electron interacts with a photon – Schrodinger equation and it’s solution https://stationarystates.com/quantum-field-theory/electron-interacts-with-a-photon-schrodinger-equation-and-its-solution/?utm_source=rss&utm_medium=rss&utm_campaign=electron-interacts-with-a-photon-schrodinger-equation-and-its-solution Wed, 27 Nov 2024 00:41:44 +0000 https://stationarystates.com/?p=670 Schrödinger Equation for Electron-Photon Interaction The system includes: An electron with wavefunction ψe(r, t), A photon field described by the vector potential A(r, t). The total Hamiltonian includes: The electron’s […]

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Schrödinger Equation for Electron-Photon Interaction

The system includes:

  • An electron with wavefunction ψe(r, t),
  • A photon field described by the vector potential A(r, t).

The total Hamiltonian includes:

  1. The electron’s kinetic energy, -ℏ2/2me2,
  2. The coupling between the electron and photon field through minimal coupling,
  3. The photon’s energy.

The Hamiltonian in SI units is:

H = (1/2me) [ -iℏ∇ - eA(r, t) ]2
    + eφ(r, t) 
    + (1/2)ε0 ∫ |E(r, t)|2 + (1/2μ0)|B(r, t)|2 d3r,

where:

  • φ(r, t) is the scalar potential,
  • E = -∂A/∂t - ∇φ is the electric field,
  • B = ∇×A is the magnetic field.

Simplifying for interaction only, the Schrödinger equation is:

iℏ∂ψe/∂t = Hψe.

Solving for Energy States

Solving the energy states requires quantizing the photon field. Using second quantization:

  • Represent the photon field as a superposition of modes:
        A(r, t) = Σk sqrt(ℏ/2ε0ωk) 
        [ akeik·r + ake-ik·r ].
    

Approach to Energy Levels:

  1. Electron in an Electromagnetic Field (Perturbation Theory): For weak coupling, perturbation theory gives corrections to the electron’s energy levels.
  2. Jaynes-Cummings Model: For resonant interactions (electron treated as a two-level system), one can use this model to calculate Rabi oscillations and energy splitting.
  3. Numerical Methods: For more general cases, computational methods are necessary.

 

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Trying to Understand Bell’s EPR Paper https://stationarystates.com/entanglement/trying-to-understand-bells-epr-paper/?utm_source=rss&utm_medium=rss&utm_campaign=trying-to-understand-bells-epr-paper Tue, 10 Sep 2024 18:15:55 +0000 https://stationarystates.com/?p=620 Sections 2 and 3 in the paper – I had some trouble deciphering. ### Section II: Formulation In this section, Bell formulates the Einstein-Podolsky-Rosen (EPR) paradox mathematically. He uses the […]

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Sections 2 and 3 in the paper – I had some trouble deciphering.

### Section II: Formulation

In this section, Bell formulates the Einstein-Podolsky-Rosen (EPR) paradox mathematically. He uses the example of two spin-½ particles in a singlet state, moving in opposite directions. According to quantum mechanics, if a measurement of one particle’s spin component along some axis a yields +1, the measurement of the other particle’s spin component along the same axis must yield -1.

Bell then introduces the hypothesis of *locality*, which means that the result of a measurement on one particle should not be influenced by a distant measurement of the other particle. In other words, if two measurements are made on these separated particles, the outcome of one should not depend on the setting of the other. This leads to the idea that the results of measurements must be predetermined by some additional “hidden” variables denoted by \lambda. These hidden variables allow for a more complete specification of the state than quantum mechanics provides.

The results of measurements on the two particles are denoted by A(a, \lambda) and B(b, \lambda), where a and b are the directions along which measurements are made, and \lambda represents the hidden variables. Bell then writes the product of the measurement results as A(a, \lambda) B(b, \lambda) and considers the expectation value of this product, denoted by P(a, b), which is expressed as an integral over the probability distribution p(\lambda) of the hidden variables.

Bell shows that if locality holds, the expectation value P(a, b) should be equal to the quantum mechanical prediction for the singlet state. However, the crux of Bell’s theorem lies in proving that no hidden variable theory that satisfies locality can reproduce the quantum mechanical predictions.

### Section III: Illustration

Before proving the main result, Bell provides a few examples to clarify the mathematical framework. He first shows that a hidden variable theory can easily explain the measurement outcomes of a single spin-½ particle in a pure state. By introducing a hidden variable that determines the outcome of any spin measurement, Bell demonstrates that the expectation value of the spin measurement along a given direction matches the quantum mechanical prediction.

Next, Bell attempts to construct a hidden variable model for two-particle systems that reproduces some of the essential features of quantum mechanics. However, he finds that while such models can approximate quantum mechanical results for some measurement settings, they fail to fully capture the quantum mechanical correlation functions, particularly for the singlet state. Specifically, the models tend to deviate from the quantum mechanical predictions for certain angles between the measurement settings.

In the final example, Bell shows that if the measurement results A(a, \lambda) and B(b, \lambda) are allowed to depend on both measurement settings a and b, it is possible to reproduce the quantum mechanical correlation functions. However, this comes at the cost of violating locality, which contradicts the key requirement that the measurement results at one location should not depend on the measurement setting at a distant location.

In conclusion, Section III illustrates that reproducing the quantum mechanical predictions is possible only by giving up locality, thus paving the way for Bell’s proof in the next section.

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Feynman’s paths and bohm’s paths in quantum theory https://stationarystates.com/basic-quantum-theory/feynmans-paths-and-bohms-paths-in-quantum-theory/?utm_source=rss&utm_medium=rss&utm_campaign=feynmans-paths-and-bohms-paths-in-quantum-theory Mon, 29 Jul 2024 14:19:39 +0000 https://stationarystates.com/?p=549 A recap of the Article – Bohm and Feynman Path Integrals – author – Marius Oltean, U Waterloo. Feynman’s Path Integral Feynman’s approach to quantum mechanics involves the concept of […]

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A recap of the Article – Bohm and Feynman Path Integrals – author – Marius Oltean, U Waterloo.

Feynman’s Path Integral

Feynman’s approach to quantum mechanics involves the concept of path integrals, where the probability amplitude for a particle to move from one point to another is computed by summing over all possible paths that the particle can take between these points. Each path contributes an amplitude, which is an integral of the classical action. This method provides a reformulation of the Schrödinger equation and is particularly useful in quantum field theory.

  • Mathematical Tool: Feynman’s paths are not real paths along which particles move. They are mathematical constructs used to calculate the evolution of the wavefunction.
  • Sum Over Histories: The method involves summing the contributions from all possible paths, weighted by the exponential of the classical action.
  • Wavefunction Propagation: The Feynman path integral provides a way to compute the propagator, which describes how the wavefunction evolves over time.

Bohm’s Path Integral

In contrast, Bohm’s approach, also known as the de Broglie-Bohm theory or Bohmian mechanics, posits that particles have definite trajectories guided by the wavefunction. This theory incorporates both the wave and particle nature of quantum entities.

  • Real Trajectories: In Bohm’s theory, particles follow actual paths determined by a guiding equation derived from the wavefunction.
  • Quantum Potential: The particle’s motion is influenced by a quantum potential, which is derived from the wavefunction and affects the trajectory.
  • Single Path: Unlike Feynman’s sum over all paths, Bohm’s formulation involves integrating the quantum Lagrangian along a single, real path—the actual trajectory of the particle.

Distinguishing Between Feynman’s and Bohm’s Paths

  1. Conceptual Basis:
    • Feynman: Paths are mathematical constructs without physical reality.
    • Bohm: Paths are real trajectories that particles actually follow.
  2. Mathematical Formulation:
    • Feynman: Involves summing over an infinite number of possible paths.
    • Bohm: Involves a single path determined by the guiding equation and quantum potential.
  3. Interpretation of Paths:
    • Feynman: The paths represent all possible histories of the particle.
    • Bohm: The path represents the actual history of the particle as it moves according to the guiding equation.
  4. Wavefunction Propagation:
    • Feynman: Uses the path integral to compute the propagator and describe the evolution of the wavefunction.
    • Bohm: Uses the de Broglie-Bohm trajectory to directly integrate the quantum Lagrangian for the wavefunction’s evolution.
  5. Physical Reality:
    • Feynman: No single path is real; all paths contribute probabilistically.
    • Bohm: The particle’s path is real and unique, influenced by the quantum potential.

The article demonstrates that while these two approaches originate from different conceptual bases, they can be connected. The Feynman method of summing over all paths can be derived from the de Broglie-Bohm theory by considering the contributions of all possible trajectories​

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Quantum vs. Classical States of a Combined System https://stationarystates.com/basic-quantum-theory/mixed-states-combined-states-quantum-vs-classical/?utm_source=rss&utm_medium=rss&utm_campaign=mixed-states-combined-states-quantum-vs-classical Wed, 24 Jul 2024 18:13:17 +0000 https://stationarystates.com/?p=539 A classical state doesn’t require basis vectors – since it is a simple POINT in phase space. This is true even of combined states in classical physics. In QM, every […]

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A classical state doesn’t require basis vectors – since it is a simple POINT in phase space. This is true even of combined states in classical physics.

In QM, every state requires basis vectors to represent. Mixed states (combined states) require special basis vectors. This post discusses some of these topics.

Combined State of a Quantum System

Quantum Combined State

In quantum mechanics, the combined state of a composite system, such as a system composed of subsystems A and B, is described by the tensor product of the individual states of the subsystems. If subsystem A is in state ∣ψA⟩|\psi_A\rangle and subsystem B is in state ∣ψB⟩|\psi_B\rangle, the combined state of the system is given by:

∣Ψ⟩=∣ψA⟩⊗∣ψB⟩|\Psi\rangle = |\psi_A\rangle \otimes |\psi_B\rangle

The basis vectors for the combined state are formed by the tensor products of the basis vectors of the subsystems. If {∣ai⟩}\{|a_i\rangle\} and {∣bj⟩}\{|b_j\rangle\} are basis vectors for subsystems A and B, respectively, the basis vectors for the combined system are {∣ai⟩⊗∣bj⟩}\{|a_i\rangle \otimes |b_j\rangle\}.

For example, if subsystem A has basis vectors ∣a1⟩|a_1\rangle and ∣a2⟩|a_2\rangle, and subsystem B has basis vectors ∣b1⟩|b_1\rangle, ∣b2⟩|b_2\rangle, and ∣b3⟩|b_3\rangle, the combined system will have the following basis vectors:

∣a1⟩⊗∣b1⟩, ∣a1⟩⊗∣b2⟩, ∣a1⟩⊗∣b3⟩, ∣a2⟩⊗∣b1⟩, ∣a2⟩⊗∣b2⟩, ∣a2⟩⊗∣b3⟩|a_1\rangle \otimes |b_1\rangle, \ |a_1\rangle \otimes |b_2\rangle, \ |a_1\rangle \otimes |b_3\rangle, \ |a_2\rangle \otimes |b_1\rangle, \ |a_2\rangle \otimes |b_2\rangle, \ |a_2\rangle \otimes |b_3\rangle

In general, if subsystem A has nn basis states and subsystem B has mm basis states, the combined system will have n×mn \times m basis states.

Classical Combined State

In classical mechanics, the combined state of a system is described by the Cartesian product of the states of the subsystems. If subsystem A is described by coordinates (x1,p1)(x_1, p_1) and subsystem B by coordinates (x2,p2)(x_2, p_2), the state of the combined system is described by the tuple (x1,p1,x2,p2)(x_1, p_1, x_2, p_2).

A classical pure state is a point in the phase space, and a classical mixed state is described by a probability density function ρ(x1,p1,x2,p2)\rho(x_1, p_1, x_2, p_2) over the phase space.

Comparison

  • Quantum Basis Vectors: In quantum mechanics, the basis vectors for the combined state are formed by the tensor product of the basis vectors of the subsystems. These basis vectors can represent entangled states where the subsystems are not independent.
  • Classical Basis Vectors: In classical mechanics, the state of the combined system is described by the Cartesian product of the states of the subsystems. The concept of basis vectors is not typically used in the same way as in quantum mechanics. Instead, the state of the system is described by a point or a probability density function in phase space.
  • Independence of Subsystems: In a classical combined state, knowledge of the state of the entire system implies complete knowledge of each subsystem. However, in a quantum combined state, especially when entanglement is involved, the state of each subsystem can be mixed even if the state of the combined system is pure

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Experimental Measurement of Planck’s Constant https://stationarystates.com/basic-quantum-theory/experimental-measurement-of-plancks-constant/?utm_source=rss&utm_medium=rss&utm_campaign=experimental-measurement-of-plancks-constant Wed, 03 Jul 2024 17:54:23 +0000 https://stationarystates.com/?p=501 Experimental Measurement of Planck’s Constant Apparatus: Light source with known wavelength Photoelectric cell Variable voltage power supply Ammeter and voltmeter Procedure: Illuminate the photoelectric cell with light of a known […]

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Experimental Measurement of Planck’s Constant
  • Apparatus:
    • Light source with known wavelength
    • Photoelectric cell
    • Variable voltage power supply
    • Ammeter and voltmeter
  • Procedure:
    • Illuminate the photoelectric cell with light of a known wavelength.
    • Adjust the voltage to stop the emitted photoelectrons (stopping potential).
    • Measure the stopping potential using the voltmeter.
    • Repeat the experiment with different wavelengths of light.
  • Calculations:
    • Use the equation eV=hf−ϕeV = hf – \phi, where ee is the electron charge, VV is the stopping potential, ff is the frequency of the light, and ϕ\phi is the work function of the material.
    • Plot stopping potential VV against frequency ff and determine the slope, which is he\frac{h}{e}.
  • Error Minimization:
    • Use monochromatic light sources with precise wavelengths.
    • Calibrate the voltage measurement equipment accurately.
    • Perform the experiment in a dark environment to avoid interference from ambient light.

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Bohm’s Quantum Potential Approach https://stationarystates.com/basic-quantum-theory/bohms-quantum-potential-approach/?utm_source=rss&utm_medium=rss&utm_campaign=bohms-quantum-potential-approach Mon, 10 Jun 2024 18:34:32 +0000 https://stationarystates.com/?p=436 Bohm’s quantum potential approach, also known as the de Broglie-Bohm interpretation or Bohmian mechanics, is an alternative formulation of quantum mechanics that provides a deterministic framework. Here are the key […]

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Bohm’s quantum potential approach, also known as the de Broglie-Bohm interpretation or Bohmian mechanics, is an alternative formulation of quantum mechanics that provides a deterministic framework. Here are the key aspects of Bohm’s quantum potential approach:

Key Concepts of Bohmian Mechanics

  1. Pilot Wave and Particle Trajectories:
    • In Bohmian mechanics, particles have definite trajectories, guided by a “pilot wave”.
    • The wave function ψ\psi evolves according to the Schrödinger equation, and particles follow deterministic paths influenced by this wave function.
  2. Quantum Potential:
    • The quantum potential QQ is a central element in Bohm’s approach, derived from the wave function <katex> ψ\psi.</katex>
    • It is given by: <katex>Q=−ℏ22m∇2RRQ = -\frac{\hbar^2}{2m} \frac{\nabla^2 R}{R}[\katex][katex] where RR is the amplitude of the wave function [katex]ψ=ReiS/ℏ\psi = Re^{iS/\hbar}, with R=∣ψ∣R = |\psi| and SS being the phase of the wave function.</katex>
    • The quantum potential affects the motion of particles, introducing quantum effects into the classical-like trajectories.
  3. Guidance Equation:
    • The velocity of a particle is determined by the gradient of the phase SS of the wave function: <katex> v=∇Sm\mathbf{v} = \frac{\nabla S}{m}
    • This equation shows that the particle’s motion is guided by the wave function’s phase.
  4. Deterministic Nature:
    • Unlike the standard Copenhagen interpretation, which involves inherent randomness in measurements, Bohmian mechanics is fully deterministic.
    • Given the initial positions and wave function, the future positions of particles can be precisely determined.
  5. Schrödinger Equation and Continuity Equation:
    • The wave function ψ\psi evolves according to the Schrödinger equation: <katex> iℏ∂ψ∂t=−ℏ22m∇2ψ+Vψi\hbar \frac{\partial \psi}{\partial t} = -\frac{\hbar^2}{2m} \nabla^2 \psi + V \psi
    • The probability density ρ=∣ψ∣2\rho = |\psi|^2 satisfies the continuity equation, ensuring the conservation of probability.

Quantum Potential and Non-locality

  1. Quantum Potential Characteristics:
    • The quantum potential QQ depends on the form of the wave function and not directly on the distance between particles, leading to non-local interactions.
    • This non-locality means that changes in the wave function in one region can instantaneously affect the quantum potential and hence the motion of particles elsewhere.
  2. Non-local Effects:
    • Bohm’s approach naturally incorporates non-locality, a feature highlighted by the famous EPR paradox and Bell’s theorem.
    • The quantum potential allows for instantaneous correlations between entangled particles, consistent with quantum mechanical predictions.

Implications and Interpretational Aspects

  1. Wave Function as a Real Field:
    • In Bohmian mechanics, the wave function ψ\psi is considered a real physical field that exists in configuration space.
    • This field guides the particles, similar to how a classical field influences particles.
  2. Measurement in Bohmian Mechanics:
    • Measurements do not collapse the wave function; instead, they reveal the pre-existing positions of particles.
    • The wave function continues to evolve smoothly, maintaining the deterministic nature of the theory.
  3. Classical Limit:
    • In the classical limit, where the quantum potential becomes negligible, Bohmian mechanics reduces to classical mechanics.
    • This correspondence principle ensures consistency with classical physics in the appropriate regime.

Summary

Bohm’s quantum potential approach offers a deterministic and non-local interpretation of quantum mechanics, where particles have well-defined trajectories guided by a pilot wave. The quantum potential, derived from the wave function, plays a crucial role in shaping these trajectories. This framework provides an alternative perspective to the standard Copenhagen interpretation, emphasizing realism and determinism while still accounting for quantum phenomena

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