Quantum statistical canonical formalism to find ground state at T

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Discussion Overview

The discussion revolves around the computational approach to solving a spinless fermionic Hamiltonian using the Quantum Canonical Ensemble formalism. Participants explore the implications of temperature on the ground state energy and wave function, as well as the challenges faced in calculations at low temperatures.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant describes their algorithm for calculating ground state energy and wave function at temperature T, detailing the steps of diagonalizing the Hamiltonian and using the density matrix.
  • Concerns are raised about the relevance of temperature in defining ground state energy and wave function, with some participants asserting that the ground state is defined at T=0.
  • Another participant argues that while the ground state energy does not change with temperature, the probability of occupying the ground state versus other states does vary with temperature.
  • There is mention of the density matrix in the canonical ensemble and how it relates to the distribution of states at finite temperatures.
  • References to external resources are provided to illustrate examples of canonical ensembles and state distributions.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between temperature and ground state properties. While some assert that ground state energy is independent of temperature, others suggest that temperature influences the occupancy probabilities of states.

Contextual Notes

Participants discuss the computational difficulties encountered at low temperatures, particularly the large values of beta leading to infinite results. There is also a lack of consensus on how to approach the calculation of ground state properties at non-zero temperatures.

Luqman Saleem
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TL;DR
As an example, calculating the ground state energy and wave function using canonical formalism of a simple fermionic model.
For my own understanding, I am trying to computationally solve a simple spinless fermionic Hamiltonian in Quantum Canonical Ensemble formalism . The Hamiltonian is written in the second quantization as

$$H = \sum_{i=1}^L c_{i+1}^\dagger c_i + h.c.$$

In the canonical formalism, the density matrix is given as
$$\rho = \frac{e^{-\beta H}}{Tr [e^{-\beta H}]}$$
where ##\beta = 1/k_B T## and the expectation value of any operator ##A## is given as
$$\langle A \rangle = Tr[\rho A]$$

Things that I want to calculate:
1. ground state energy at temperature ##T##
2. ground state wave-function at ##T##

My attempt to solution:
1. I first write ##H## in matrix form by using particle number basis i.e. 1100, 1010 ##\cdots## for 4 sites and 2 particles
2. then I diagonalize ##H## and find energy eigenvalues ##E_i## and eigenvectors ##\psi_i##
3. then I write ##\rho## by using above given formula
4. finally, I try to calculate ground state energy using ##\langle H \rangle = Tr[\rho H]##

Problems I am facing:
As Boltzmann constant ##k_B## is ##1.36\times 10^{-23}##, so even at room room temperature ##\beta## is very large i.e. ~##10^{21}##. Due to which I can't calculate ground state energy at very low temperatures? Computer just give 'Infinity' values. And at very large temperatures, the energy seems to be decreasing with increasing ##T##. ... totally wrong

Questions:
1. Is my algorithm correct? How can we calculate ground state energy at ##T=0## and at small temperatures?
2. How to calculate ground state wave function at ##T##?
 
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Is the temperature relevant to defining the ground state energy and wave function? Isn't the ground state defined at T=0?
 
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atyy said:
Is the temperature relevant to defining the ground state energy and wave function? Isn't the ground state defined at T=0?
At T=0, ground state is defined. I was just wondering how does statistical mechanics' formalism deal with this case. And I got the answer, I mean at T=0, ##\rho = I##, which means ##\langle H \rangle = \langle I H \rangle = \langle H \rangle##.

And I would say that ground state energy is relevant to temperature. Does not ground state energy increase with the increase in temperature?
 
Luqman Saleem said:
And I would say that ground state energy is relevant to temperature. Does not ground state energy increase with the increase in temperature?

The ground state and the ground state energy do not change with temperature. The ground state is a property of the Hamiltonian, and is the state with the lowest energy.

The probability with which the ground state and other states are occupied changes with temperature.

In the canonical ensemble at finite T, each member of the notional canonical ensemble of systems is in a different state. The distribution of states across the members of the ensemble is given by the density matrix of the canonical ensemble. Roughly, one can think that the probability of a given state in the canonical ensemble is given by p(E) ∝ exp(-βE).

You can find an example in https://en.wikipedia.org/wiki/Canonical_ensemble. See the right side of the figure titled "Example of canonical ensemble for a quantum system consisting of one particle in a potential well."

You can also see section 6.5 of https://mcgreevy.physics.ucsd.edu/s12/lecture-notes/chapter06.pdf for an example of the distribution of states at finite T in the canonical ensemble for the quantum harmonic oscillator.
 
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