Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Log inSign up
Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Blog
Job Board
Q3AS

© 2026 Aqora Quantum S.A.S.

TermsPrivacyLegal Notice

A Unified Theory of Characteristic Equations for Bose-Einstein Condensates: Dimensional Extension, Fractional Superfluidity and Generalized Quantum Statistics

shifa liu

Published Dec 31, 2025• 0 citations
Publisher

Abstract

This paper establishes and systematically develops the “Theory of Characteristic Equations” for Bose-Einstein condensates (BECs), revealing a profound correspondence between diverse types of equations – polynomial (partition functions), differential (Gross-Pitaevskii and Bogoliubov-de Gennes equations), integral (path integrals and dimensional regularization), difference (lattice BECs), sum (antidifferences), variational (energy functionals), inverse variational (effective actions), and transcendental (BKT transition and Efimov effect) – and geometric/topological structures of quantum degenerate Bose gases. This provides a complete geometric characteristic representation for BECs, thereby extending and upgrading classical mean-field theory, Bogoliubov theory, and the theory of quantum phase transitions to a unified framework. Starting from the observation that the partition function of an ideal Bose gas is a characteristic polynomial that reduces to the binomial theorem via the Euler- Maclaurin formula, we propose the Dimensional Extension Principle: integer parameters such as spatial dimension, particle number, and interaction range can be analytically continued via the Gamma function and generalized binomial coefficients, thereby generalizing integer-dimensional BEC theory to real and even complex dimensions. We rigorously construct negative-dimensional BEC models, compute their homology via Koszul complexes and BGG resolutions, and establish duality relations. We prove equivalence between dimensional regularization in quantum field theory and characteristic integral equations for BECs. We interpret the Bogoliubov excitation spectrum as a characteristic differential equation, extending it to fractional-dimensional lattices Zα whose heat kernel coefficients are polynomials in α with binomial structure. We incorporate variational principles (Gross-Pitaevskii functionals) and prove analytic dependence on dimension for condensate ground states. We extend difference equations to fractional-dimensional optical lattices via interpolation, with spectra depending continuously on the dimension. We develop sum equations (antidifferences) capturing the discrete partition function and its analytic continuation, leading to α-dimensional BEC models whose characteristic equation reduces to the Euler-binomial identity in the Abel sense for Re(α) > −1. We introduce modular and elliptic BEC networks (e.g., BECs in frustrated lattices and the BKT transition), whose characteristic equations reduce to modular equations. All major BEC invariants – partition functions, heat-kernel coefficients, and their fractional extensions – are unified under this framework. We prove a Strong Unification Theorem showing that all these invariants are manifestations of a single underlying structure: the binomial theorem and its analytic continuations. We establish a fractional-dimensional index theorem for Dirac operators on bipartite BEC networks and extend the Atiyah-Singer theorem to non-integer dimensions. The work demonstrates that characteristic equations provide a complete representation of BEC features, upgrading spectral, statistical, and hydrodynamic theories to a generalized geometry capable of handling non-integer and negative parameters, as well as various types of equations, offering a unified language for many branches of condensed matter physics, quantum field theory, and mathematical physics.

DOI
10.5281/zenodo.21138809

Related papers

A Note on the Resolvent Algebra and Functional Integral Approach to the Free Bose Einstein Condensation

Yoshitsugu Sekine

We present a systematic description of the structure of Bose-Einstein condensation (BEC) in the free Bose gas from the viewpoint of the correspondence between the operator-algebraic formulation based on the resolvent algebra and the functional integral representation. By clarifying the representation-theoretic structure of finite-temperature BEC states and rigorously analyzing the correspondence between their direct integral decomposition and the ergodic decomposition of the associated probability measures, we provide a framework in which general features of phase transitions-such as the emergence of order parameters, the decomposition of states, and clustering properties-are explicitly described using BEC in the free Bose gas as a concrete example. Furthermore, we construct in detail the correspondence between the decomposition of measures in the functional integral approach and that of operator-algebraic representations, thereby establishing the equivalence between the probabilistic and algebraic aspects, and providing a guiding principle for isolating the essential structures by disentangling the additional mathematical complications arising from the treatment of infrared singularities in interacting systems. These results lay a foundation for the rigorous analysis of phase transitions in non-relativistic constructive quantum field theory and quantum statistical mechanics, and serve as a starting point for extensions to interacting models.

arXiv:2604.01424•Apr 1, 2026•0 citations

Mathematical Models and Numerical Methods for Bose-Einstein Condensation

Weizhu Bao

The achievement of Bose-Einstein condensation (BEC) in ultracold vapors of alkali atoms has given enormous impulse to the theoretical and experimental study of dilute atomic gases in condensed quantum states inside magnetic traps and optical lattices. This article offers a short survey on mathematical models and theories as well as numerical methods for BEC based on the mean field theory. We start with the Gross-Pitaevskii equation (GPE) in three dimensions (3D) for modeling one-component BEC of the weakly interacting bosons, scale it to obtain a three-parameter model and show how to reduce it to two dimensions (2D) and one dimension (1D) GPEs in certain limiting regimes. Mathematical theories and numerical methods for ground states and dynamics of BEC are provided. Extensions to GPE with an angular momentum rotation term for a rotating BEC, to GPE with long-range anisotropic dipole-dipole interaction for a dipolar BEC and to coupled GPEs for spin-orbit coupled BECs are discussed. Finally, some conclusions are drawn and future research perspectives are discussed.

arXiv:1403.3884•Mar 16, 2014•10 citations

Termodinamica di bosoni confinati e interagenti

Matteo Ferraretto

The Bose-Einstein condensation (BEC) is a quantum phenomenon which was theorized in 1920s, but it was realized for the first time in the JILA Laboratory (University of Colorado, Boulder) by Eric Cornell and Carl Wieman only in 1995. Since 1995, lots of experiments on BEC have been realized using different gases and various conditions. One can give a correct interpretation of the results of these works only by considering the role of interaction between particles on relevant physical quantities, such as critical temperature and condensed fraction. The purpose of our work is deducing the main thermodynamic properties of trapped and interacting Bose gases using the tools of Quantum Mechanics, avoiding the introduction of (which often recurs in litterature). The first chapter shows a derivation of the famous Gross-Pitaevskii equation, starting from the many-bodies Dirac action and applying the principle of least action. Moreover, two approximate solutions of this equation are discussed as well: the gaussian variational ansatz for weakly interacting particles, and the Thomas-Fermi approximation, for strongly interacting particles. In chapter 2 we derive the Bogoliubov dispersion relation for excited states (or quasiparticle energy spectrum) with the tools of Hamiltonian Mechanics and semiclassical approximation. Furthermore, we discuss some approximations for this formula (especially the Hartree-Fock spectrum for weakly interacting bosons) and we use the Bose-Einstein distribution to find the thermal cloud density. In chapter 3 we use the previous results to calculate explicit expressions for critical temperature and condensed fraction (where possible) in four particular cases: ideal free and trapped Bose gas, interacting free and trapped Bose gas. We also discuss the main results obtained by Giorgini, Pitaevskii and Stringari, who managed to explain accurately Cornell and Wieman's experimental plots. Finally we conclude that traditional Quantum Mechanics is quite efficient to derive the main equations of BEC and that introducing second quantization is not essential. Nevertheless, some issues remain unresolved in this context: for example the phenomenon of quantum depletion and the generalisation of the Gross-Pitaevskii equation at non-zero temperature.

•Sep 1, 2016•0 citations

On the Bose-Einstein condensation

S.R. DE GROOT, G.J. Hooyman, Cornelis A. Ten Seldam

Abstract The Bose-Einstein condensation of a gas is investigated. Starting from the well-known formulae for Bose statistics, the problem has been generalized to include a variety of potential fields in which the particles of the gas move, and the number w of dimensions has not been restricted to three. The energy levels are taken to be εi≡εs1,....,s10=constanth2ms1α−1a12+...+swαaw2(1≤α≤2) the quantum numbers being s1 ,w= 1, 2, ..., and a1, ..., aw being certain characteristic lengths. (For α = 2, the potential field is that of the w-dimensional rectangular box; for α = 1, we obtain the w-dimensional harmonic oscillator field.) A direct rigorous method is used similar to that proposed by Fowler & Jones (1938). It is shown that the number q = w/α determines the appearance of an Einstein transition temperature T0·For q≤ 1 there is no such point, while for q > 1 a transition point exists. For 1 < q≤ 2, the mean energy ϵ- per particle and the specific heat dϵ-/dT are continuous at T = T0· For q > 2, the specific heat is discontinuous at T = T0, giving rise to a A λ-point. A well-defined transition point only appears for a very large (theoretically infinite) number N of particles. T0 is finite only if the quantity v = N/(a1 .... aw)2/ α¯is finite. For a rectangular box, v is equal to the mean density of the gas. If v tends to zero or infinity as N→ ∞, then T0 likewise tends to zero or infinity. In the case q > 1, and at temperatures T < T 0' there is a finite fraction N0 /N of the particles, given by N 0/N = 1-(T/T0)q, in the lowest state. London’s formula (1938 b) for the three-dimensional box is an example of this equation. Some further results are also compared with those given by London’s continuous spectrum approximation.

Proceedings of the Royal Society of London A Mathematical and Physical Sciences•Sep 22, 1950•138 citations

Mathematical theory and numerical methods for Bose-Einstein condensation

Weizhu Bao, Yongyong Cai

In this paper, we mainly review recent results on mathematical theory andnumerical methods for Bose-Einstein condensation (BEC),based on the Gross-Pitaevskii equation (GPE). Starting from the simplest case with one-component BEC of the weakly interacting bosons, we study the reduction of GPE to lower dimensions, the ground states of BEC including the existence and uniqueness as well as nonexistence results, and the dynamics of GPE including dynamical laws, well-posedness of the Cauchy problem as well as the finite time blow-up. To compute the ground state, the gradient flow with discrete normalization (or imaginary time) method is reviewed and various full discretization methods are presented and compared. To simulate the dynamics, both finite difference methods and time splitting spectral methods are reviewed, and their error estimates are briefly outlined. When the GPE has symmetric properties, we show how to simplify the numerical methods. Then we compare two widely used scalings, i.e. physical scaling (commonly used) and semiclassical scaling, for BEC in strong repulsive interaction regime (Thomas-Fermi regime), and discuss semiclassical limits of the GPE. Extensions of these results for one-component BEC are thencarried out for rotating BEC by GPE with an angular momentum rotation, dipolar BEC by GPE with long range dipole-dipole interaction, and two-component BEC by coupled GPEs. Finally, as a perspective, we show briefly the mathematical models forspin-1 BEC, Bogoliubov excitation and BEC at finite temperature.

arXiv:1212.5341•Kinetic and Related Models•Dec 11, 2012•591 citations

Mathematical analysis of Bose mixtures and related models: ground state theory and effective dynamics.

Alessandro Olgiati

This PhD thesis contains new results on the mathematical study of Bose-Einstein condensation and the main part of it is devoted to mixtures of condensates, i.e., systems composed of multiple bosonic species in interaction. We prove the validity of effective ground state theories for mixtures in the Gross-Pitaevskii and mean-field regime. We show that the ground state energy asymptotics, in the large-N limit, is captured by the minimum of a suitable one-body functional. Moreover, we prove that in the ground state all species exhibit Bose-Einstein condensation onto the minimizer of that functional. For mixtures in the mean-field regime, we provide a rigorous justification of Bogoliubov’s theory. This is done by computing the contribution to the ground state energy which is due to excited particles. We also prove a norm approximation for the ground state vector, in the Fock space norm. From the time-dependent viewpoint, we prove for the first time the validity of the effective equations that were previously known due to heuristic physical arguments, and that are confirmed by robust experimental evidence. Our results show that, for mixtures in the Gross-Pitaevskii and mean-field regime, the effective dynamics is governed by a system of non-linear Schrödinger equations, one for each species of the mixture. In the final part of the thesis we present additional results on problems and models related to the study on mixtures. We were able to derive the effective dynamics for spinor- and pseudo-spinor condensates. The equations that we obtain are precisely those of modern experiments with ultra-cold spin bosons. We also show that the mean-field model provide a time-dependent control of condensation that is very accurate for the typical duration times of experiments. A further result is the global well-posedness in the energy space of the singular Hartree equation. Last, we present new remarks on the adaptation of known techniques that one needs in order to prove the derivation of the magnetic Gross-Pitaevskii equation.

•Sep 25, 2018•0 citations
This paper establishes and systematically develops the “Theory of Characteristic Equations” for Bose-Einstein condensates (BECs), revealing a profound correspondence between diverse types of equations – polynomial (partition functions), differential (Gross-Pitaevskii and Bogoliubov-de Gennes equations), integral (path integrals and dimensional regularization), difference (lattice BECs), sum (antidifferences), variational (energy functionals), inverse variational (effective actions), and transcendental (BKT transition and Efimov effect) – and geometric/topological structures of quantum degenerate Bose gases. This provides a complete geometric characteristic representation for BECs, thereby extending and upgrading classical mean-field theory, Bogoliubov theory, and the theory of quantum phase transitions to a unified framework. Starting from the observation that the partition function of an ideal Bose gas is a characteristic polynomial that reduces to the binomial theorem via the Euler- Maclaurin formula, we propose the Dimensional Extension Principle: integer parameters such as spatial dimension, particle number, and interaction range can be analytically continued via the Gamma function and generalized binomial coefficients, thereby generalizing integer-dimensional BEC theory to real and even complex dimensions. We rigorously construct negative-dimensional BEC models, compute their homology via Koszul complexes and BGG resolutions, and establish duality relations. We prove equivalence between dimensional regularization in quantum field theory and characteristic integral equations for BECs. We interpret the Bogoliubov excitation spectrum as a characteristic differential equation, extending it to fractional-dimensional lattices Zα whose heat kernel coefficients are polynomials in α with binomial structure. We incorporate variational principles (Gross-Pitaevskii functionals) and prove analytic dependence on dimension for condensate ground states. We extend difference equations to fractional-dimensional optical lattices via interpolation, with spectra depending continuously on the dimension. We develop sum equations (antidifferences) capturing the discrete partition function and its analytic continuation, leading to α-dimensional BEC models whose characteristic equation reduces to the Euler-binomial identity in the Abel sense for Re(α) > −1. We introduce modular and elliptic BEC networks (e.g., BECs in frustrated lattices and the BKT transition), whose characteristic equations reduce to modular equations. All major BEC invariants – partition functions, heat-kernel coefficients, and their fractional extensions – are unified under this framework. We prove a Strong Unification Theorem showing that all these invariants are manifestations of a single underlying structure: the binomial theorem and its analytic continuations. We establish a fractional-dimensional index theorem for Dirac operators on bipartite BEC networks and extend the Atiyah-Singer theorem to non-integer dimensions. The work demonstrates that characteristic equations provide a complete representation of BEC features, upgrading spectral, statistical, and hydrodynamic theories to a generalized geometry capable of handling non-integer and negative parameters, as well as various types of equations, offering a unified language for many branches of condensed matter physics, quantum field theory, and mathematical physics.
We present a systematic description of the structure of Bose-Einstein condensation (BEC) in the free Bose gas from the viewpoint of the correspondence between the operator-algebraic formulation based on the resolvent algebra and the functional integral representation. By clarifying the representation-theoretic structure of finite-temperature BEC states and rigorously analyzing the correspondence between their direct integral decomposition and the ergodic decomposition of the associated probability measures, we provide a framework in which general features of phase transitions-such as the emergence of order parameters, the decomposition of states, and clustering properties-are explicitly described using BEC in the free Bose gas as a concrete example. Furthermore, we construct in detail the correspondence between the decomposition of measures in the functional integral approach and that of operator-algebraic representations, thereby establishing the equivalence between the probabilistic and algebraic aspects, and providing a guiding principle for isolating the essential structures by disentangling the additional mathematical complications arising from the treatment of infrared singularities in interacting systems. These results lay a foundation for the rigorous analysis of phase transitions in non-relativistic constructive quantum field theory and quantum statistical mechanics, and serve as a starting point for extensions to interacting models.
The achievement of Bose-Einstein condensation (BEC) in ultracold vapors of alkali atoms has given enormous impulse to the theoretical and experimental study of dilute atomic gases in condensed quantum states inside magnetic traps and optical lattices. This article offers a short survey on mathematical models and theories as well as numerical methods for BEC based on the mean field theory. We start with the Gross-Pitaevskii equation (GPE) in three dimensions (3D) for modeling one-component BEC of the weakly interacting bosons, scale it to obtain a three-parameter model and show how to reduce it to two dimensions (2D) and one dimension (1D) GPEs in certain limiting regimes. Mathematical theories and numerical methods for ground states and dynamics of BEC are provided. Extensions to GPE with an angular momentum rotation term for a rotating BEC, to GPE with long-range anisotropic dipole-dipole interaction for a dipolar BEC and to coupled GPEs for spin-orbit coupled BECs are discussed. Finally, some conclusions are drawn and future research perspectives are discussed.
The Bose-Einstein condensation (BEC) is a quantum phenomenon which was theorized in 1920s, but it was realized for the first time in the JILA Laboratory (University of Colorado, Boulder) by Eric Cornell and Carl Wieman only in 1995. Since 1995, lots of experiments on BEC have been realized using different gases and various conditions. One can give a correct interpretation of the results of these works only by considering the role of interaction between particles on relevant physical quantities, such as critical temperature and condensed fraction. The purpose of our work is deducing the main thermodynamic properties of trapped and interacting Bose gases using the tools of Quantum Mechanics, avoiding the introduction of (which often recurs in litterature). The first chapter shows a derivation of the famous Gross-Pitaevskii equation, starting from the many-bodies Dirac action and applying the principle of least action. Moreover, two approximate solutions of this equation are discussed as well: the gaussian variational ansatz for weakly interacting particles, and the Thomas-Fermi approximation, for strongly interacting particles. In chapter 2 we derive the Bogoliubov dispersion relation for excited states (or quasiparticle energy spectrum) with the tools of Hamiltonian Mechanics and semiclassical approximation. Furthermore, we discuss some approximations for this formula (especially the Hartree-Fock spectrum for weakly interacting bosons) and we use the Bose-Einstein distribution to find the thermal cloud density. In chapter 3 we use the previous results to calculate explicit expressions for critical temperature and condensed fraction (where possible) in four particular cases: ideal free and trapped Bose gas, interacting free and trapped Bose gas. We also discuss the main results obtained by Giorgini, Pitaevskii and Stringari, who managed to explain accurately Cornell and Wieman's experimental plots. Finally we conclude that traditional Quantum Mechanics is quite efficient to derive the main equations of BEC and that introducing second quantization is not essential. Nevertheless, some issues remain unresolved in this context: for example the phenomenon of quantum depletion and the generalisation of the Gross-Pitaevskii equation at non-zero temperature.
Abstract The Bose-Einstein condensation of a gas is investigated. Starting from the well-known formulae for Bose statistics, the problem has been generalized to include a variety of potential fields in which the particles of the gas move, and the number w of dimensions has not been restricted to three. The energy levels are taken to be εi≡εs1,....,s10=constanth2ms1α−1a12+...+swαaw2(1≤α≤2) the quantum numbers being s1 ,w= 1, 2, ..., and a1, ..., aw being certain characteristic lengths. (For α = 2, the potential field is that of the w-dimensional rectangular box; for α = 1, we obtain the w-dimensional harmonic oscillator field.) A direct rigorous method is used similar to that proposed by Fowler & Jones (1938). It is shown that the number q = w/α determines the appearance of an Einstein transition temperature T0·For q≤ 1 there is no such point, while for q > 1 a transition point exists. For 1 < q≤ 2, the mean energy ϵ- per particle and the specific heat dϵ-/dT are continuous at T = T0· For q > 2, the specific heat is discontinuous at T = T0, giving rise to a A λ-point. A well-defined transition point only appears for a very large (theoretically infinite) number N of particles. T0 is finite only if the quantity v = N/(a1 .... aw)2/ α¯is finite. For a rectangular box, v is equal to the mean density of the gas. If v tends to zero or infinity as N→ ∞, then T0 likewise tends to zero or infinity. In the case q > 1, and at temperatures T < T 0' there is a finite fraction N0 /N of the particles, given by N 0/N = 1-(T/T0)q, in the lowest state. London’s formula (1938 b) for the three-dimensional box is an example of this equation. Some further results are also compared with those given by London’s continuous spectrum approximation.
In this paper, we mainly review recent results on mathematical theory andnumerical methods for Bose-Einstein condensation (BEC),based on the Gross-Pitaevskii equation (GPE). Starting from the simplest case with one-component BEC of the weakly interacting bosons, we study the reduction of GPE to lower dimensions, the ground states of BEC including the existence and uniqueness as well as nonexistence results, and the dynamics of GPE including dynamical laws, well-posedness of the Cauchy problem as well as the finite time blow-up. To compute the ground state, the gradient flow with discrete normalization (or imaginary time) method is reviewed and various full discretization methods are presented and compared. To simulate the dynamics, both finite difference methods and time splitting spectral methods are reviewed, and their error estimates are briefly outlined. When the GPE has symmetric properties, we show how to simplify the numerical methods. Then we compare two widely used scalings, i.e. physical scaling (commonly used) and semiclassical scaling, for BEC in strong repulsive interaction regime (Thomas-Fermi regime), and discuss semiclassical limits of the GPE. Extensions of these results for one-component BEC are thencarried out for rotating BEC by GPE with an angular momentum rotation, dipolar BEC by GPE with long range dipole-dipole interaction, and two-component BEC by coupled GPEs. Finally, as a perspective, we show briefly the mathematical models forspin-1 BEC, Bogoliubov excitation and BEC at finite temperature.
This PhD thesis contains new results on the mathematical study of Bose-Einstein condensation and the main part of it is devoted to mixtures of condensates, i.e., systems composed of multiple bosonic species in interaction. We prove the validity of effective ground state theories for mixtures in the Gross-Pitaevskii and mean-field regime. We show that the ground state energy asymptotics, in the large-N limit, is captured by the minimum of a suitable one-body functional. Moreover, we prove that in the ground state all species exhibit Bose-Einstein condensation onto the minimizer of that functional. For mixtures in the mean-field regime, we provide a rigorous justification of Bogoliubov’s theory. This is done by computing the contribution to the ground state energy which is due to excited particles. We also prove a norm approximation for the ground state vector, in the Fock space norm. From the time-dependent viewpoint, we prove for the first time the validity of the effective equations that were previously known due to heuristic physical arguments, and that are confirmed by robust experimental evidence. Our results show that, for mixtures in the Gross-Pitaevskii and mean-field regime, the effective dynamics is governed by a system of non-linear Schrödinger equations, one for each species of the mixture. In the final part of the thesis we present additional results on problems and models related to the study on mixtures. We were able to derive the effective dynamics for spinor- and pseudo-spinor condensates. The equations that we obtain are precisely those of modern experiments with ultra-cold spin bosons. We also show that the mean-field model provide a time-dependent control of condensation that is very accurate for the typical duration times of experiments. A further result is the global well-posedness in the energy space of the singular Hartree equation. Last, we present new remarks on the adaptation of known techniques that one needs in order to prove the derivation of the magnetic Gross-Pitaevskii equation.