Finite-frequency noise in a non-interacting quantum dot

summary

Video file (mp4)

The gist

The gist The calculation of non-symmetrized finite-frequency NS-FF noise for a single-level quantum dot connected to reservoirs in the spinless non-interacting case establishes a general formula and

In short

This study calculates non-symmetrized finite-frequency noise for a single-level quantum dot connected to two reservoirs in a spinless, non-interacting system using Keldysh Green's functions. The results establish a general formula applicable across various temperatures and bias voltages. Numerical analysis shows the noise spectrum evolves significantly with changes in temperature, dot energy level, and coupling strength.

Key concepts

Keldysh Green’s function formalism
This is a mathematical framework used to describe quantum transport in non-equilibrium systems. It allows researchers to calculate how particles move between different parts of the system (like the dot and reservoirs) when they are not in equilibrium, which is essential for finding noise characteristics.
Non-symmetrized Finite-Frequency Noise (NS-FF noise)
This refers to a specific type of noise calculated for the quantum dot. It measures fluctuations in current at different frequencies. The 'non-symmetrized' aspect means it doesn't account for all possible symmetries, providing a detailed look at the system's response under specific conditions.
Büttiker Formula
This is a known expression from scattering theory that describes finite-frequency noise in quantum transport. The paper shows that their calculated non-symmetrized noise matches the Büttiker formula when symmetrized, confirming the consistency of their method with established scattering theory results.
Excess Noise ($\Delta S_{LL}(\omega, V)$)
This quantity is the difference between the total finite-frequency noise and the zero-voltage noise. Analyzing how this excess noise changes with frequency reveals how different physical parameters like temperature and coupling affect the fluctuations in current as a function of energy.

Terminology used across episodes

This episode discusses

The paper

Finite-frequency noise in a non-interacting quantum dot · Read on arXiv

Redouane Zamoum, Mireille Lavagna, Adeline Crépieux

Facultພ des sciences et des sciences appliquພes, Universitພe de Bouira · Univ. Grenoble Alpes, INAC-SPSMS · Aix Marseille Universitພe, Universitພe de Toulon

DOI: 10.1088/1742-5468/2016/05/054013

Transcript

Introduction to the show: ident: Quantum Radio. Generated commentary on the latest quantum physics and condensed matter papers.

Kai: I'm Kai.

Mira: And I'm Mira, here with Lev.

Kai: We're looking at the paper: "Finite-frequency noise in a non-interacting quantum dot".

Mira: Here's the gist of the paper. The gist The calculation of non-symmetrized finite-frequency NS-FF noise for a single-level quantum dot connected to reservoirs in the spinless non-interacting case establishes a general formula and reveals complex behaviors when varying temperature, dot energy level, and coupling strength.

Kai: Model and Formalism The study considers a single-level quantum dot connected to two reservoirs in the spinless non-interacting case <ref:1510.00762#pg3>.

Mira: The Hamiltonian is defined as the sum of four contributions: H = HL + HR + HT + Hdot <ref:1510.00762#pg3>.

Kai: The calculation employs the Keldysh Green’s function formalism in the wide band approximation limit <ref:1510.00762#pg3>.

Paper summary: Kai: So we’ve seen they established this general formula for non-symmetrized finite-frequency NS-FF noise for a single quantum dot. Mira They also showed that by taking the symmetrized version of that expression, their result coincides with the expression for finite frequency noise obtained by Büttiker using scattering theory.

Lev: It's interesting because it gives us a way to calculate this specific type of noise without having to rely solely on complex many-body techniques like full interacting Green's functions immediately. Kai Right, so they set up the model first, defining the Hamiltonian as a sum of four parts: H = HL + HR + HT + Hdot.

Mira: They use the Keldysh Green’s function formalism in the wide band approximation limit to do this calculation. Lev And then they define the noise in the left reservoir using that current-current correlation function, SLL(ω).

Kai: The core of their derivation involves expressing this noise SLL(τ, τ′) in terms of full two-particle Green's functions Gddi(τ, τ′, τ1, τ2) <ref:1510.00762#pg2>. Mira In the non-interacting case, they use the Hartree-Fock approximation to factorize those two-particle Green's functions into a product of one-particle Green's functions.

Lev: That factorization is important because it simplifies things immensely for calculations that would otherwise be intractable with interacting systems. Kai They then break down the noise SLL(τ, τ′) into two parts: a disconnected part, Sdis(τ, τ′), and a connected part that has fifteen contributions.

Mira: After Fourier transforming those fifteen contributions, they get an expression for P1(ω). Lev So they move from time-domain correlators to frequency-domain noise spectral density, which is what we usually care about when looking at noise.

Kai: The resulting finite-frequency noise spectrum SLL(ω) is given by equation thirty in the paper. Mira In the wide flat band limit with symmetric couplings, this expression simplifies down to a specific form involving T(ε - ω), T(ε), and some functions fLR and fRR.

Lev: That simplified form is what ties it back to Büttiker’s formula for the symmetrized finite frequency noise that they found using scattering matrix theory. Kai And they also provide an explicit analytical expression for the non-interacting case at zero temperature, which matches results from Hammer and Belzig.

Mira: What this means for us is they give us a general tool to calculate this specific kind of noise across different conditions—temperature, frequency, and bias voltage. Lev It sets a benchmark for how we can approach the noise calculation when interactions are ignored in a quantum dot system like this.

Conclusion: Kai: So, looking at the paper "Finite-frequency noise in a non-interacting quantum dot," it really boils down to them proving they have a general formula for the non-symmetrized finite-frequency NS-FF noise. Mira And they showed this isn't just some isolated calculation; it connects their result to established scattering theory results through symmetrization.

Lev: The real implication is that we have a systematic way to predict how noise behaves in these simple, non-interacting quantum dot systems across various external conditions like temperature and voltage. Kai It confirms that the non-interacting case gives us a solid theoretical foundation before we even start adding more complex interactions back into the picture.

Mira: And they also gave us that zero temperature result, which is a specific analytical expression for SLL(ω) involving the theta function and some terms dependent on eV and ω. Lev So what this means for someone who only listens to this show is that you have a mathematical tool to calculate how noisy these tiny quantum dots are under specific conditions.

Kai: It’s about establishing a baseline calculation, which is pretty crucial because it shows the underlying structure of the noise before we complicate things with Coulomb interactions. Mira And for future work, they mentioned numerical calculations exploring how varying temperature, dot energy level, and coupling strength changes the spectrum. Lev That numerical exploration seems to reveal a lot about symmetry properties in how this noise evolves under different conditions.

Kai: So the title is pretty descriptive of what they did: finite-frequency noise in a non-interacting quantum dot. Mira And the authors are showing that their formalism, based on nonequilibrium Green's functions, is a valid way to tackle this kind of problem.

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