Simon problems

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Template:Short description Template:Distinguish Template:Multiple issues In mathematics, the Simon problems (or Simon's problems) are a series of fifteen questions posed in the year 2000 by Barry Simon, an American mathematical physicist.[1][2] Inspired by other collections of mathematical problems and open conjectures, such as the famous list by David Hilbert, the Simon problems concern quantum operators.[3] Eight of the problems pertain to the anomalous spectral behavior of Schrödinger operators, and five concern operators that incorporate the Coulomb potential.[1][4]

In 2014, Artur Avila won a Fields Medal for work including the solution of three Simon problems.[5][6] Among these was the problem of proving the set of energy levels of one particular abstract quantum system was, in fact, the Cantor set, a challenge known as the "Ten Martini Problem" after the reward Mark Kac offered for solving it.[6][7]

The 2000 list was a refinement of a similar set of problems Simon had posed in 1984.[8][9]

Context

Background definitions for the "Coulomb energies" problems (N non-relativistic particles (electrons) in ℝ3 with spin 1/2 and an infinitely heavy nucleus with charge Z and Coulombic mutual interaction):

  • ℋf(N) is the space of functions on L2(ℝ3N;ℂ2N) which are asymmetrical under exchange of the N spin and space coordinates.[1] Equivalently, the subspace of (L2(ℝ3)⊗ℂ2)⊗N which is asymmetrical under the exchange of the N factors.
  • The Hamiltonian is H(N,Z):=∑i=1N(−Δi−Z|xi|)+∑i<j1|xi−xj|. Here xi∈ℝ3 is the coordinate of the i-th particle, Δi is the Laplacian with respect to the coordinate xi. Even if the Hamiltonian does not explicitly depend on the state of the spin sector, the presence of spin has an effect due to the asymmetry condition on the total wave-function.
  • We define E(N,Z):=minℋfH(N,Z), that is, the ground state energy of the (N,Z) system.
  • We define N0(Z) to be the smallest value of N such that E(N+j,Z)=E(N,Z) for all positive integers j; it is known such a number always exists and is always between Z and 2Z, inclusive.[1]

The 1984 list

Simon listed the following problems in 1984:[8]

No. Short name Statement Status Year solved
1st (a) Almost always global existence for Newtonian gravitating particles (a) Prove that the set of initial conditions for which Newton's equations fail to have global solutions has measure zero. Open as of 1984.[8]Template:Update inline In 1977, Donald Saari showed this is true for 4-body problems.[10] ?
(b) Existence of non-collisional singularities in the Newtonian N-body problem Show that there are non-collisional singularities in the Newtonian N-body problem for some N and suitable masses. In 1988, Xia gave an example of a 5-body configuration which undergoes a non-collisional singularity.[11][12]

In 1991, Gerver showed 3n-body problems in the plane for some sufficiently large value of n also undergo non-collisional singularities.[13]

1989
2nd (a) Ergodicity of gases with soft cores Find repulsive smooth potentials for which the dynamics of N particles in a box (with, e.g., smooth wall potentials) is ergodic. Open as of 1984.Template:Update inline

Yakov Sinai once proved the hard sphere gas is ergodic, but no complete proof has appeared except for the case of two particles, and a sketch for three, four, and five particles.[8]

?
(b) Approach to equilibrium Use the scenario above to justify that large systems with forces that are attractive at suitable distances approach equilibrium, or find an alternate scenario that does not rely on strict ergodicity in finite volume. Open as of 1984.Template:Update inline ?
(c) Asymptotic abelianness for the quantum Heisenberg dynamics Prove or disprove that the multidimensional quantum Heisenberg model is asymptotically abelian. Open as of 1984.Template:Update inline ?
3rd Turbulence and all that Develop a comprehensive theory of long-time behavior of dynamical systems, including a theory of the onset of and of fully developed turbulence. Open as of 1984.Template:Update inline ?
4th (a) Fourier's heat law Find a mechanical model in which a system of size L with temperature difference ΔT between its ends has a rate of heat temperature that goes as L−1 in the limit L→∞. Open as of 1984.Template:Update inline ?
(b) Kubo's formula Justify Kubo's formula in a quantum model or find an alternate theory of conductivity. Open as of 1984.Template:Update inline ?
5th (a) Exponential decay of v=2 classical Heisenberg correlations Consider the two-dimensional classical Heisenberg model. Prove that for any beta, correlations decay exponentially as distance approaches infinity. Open as of 1984.Template:Update inline ?
(b) Pure phases and low temperatures for the v≥3 classical Heisenberg model Prove that, in the D=3 model at large beta and at dimension v≥3, the equilibrium states form a single orbit under SO(3): the sphere.
(c) GKS for classical Heisenberg models Let f and g be finite products of the form (σα⋅σγ) in the D=3 model. Is it true that <fg>Λ,β≥<f>Λ,β<g>Λ,β ?Template:Clarification needed
(d) Phase transitions in the quantum Heisenberg model Prove that for v≥3 and large beta, the quantum Heisenberg model has long range order.
6th Explanation of ferromagnetism Verify the Heisenberg picture of the origin of ferromagnetism (or an alternative) in a suitable model of a realistic quantum system. Open as of 1984.Template:Update inline ?
7th Existence of continuum phase transitions Show that for suitable choices of pair potential and density, the free energy is non-C1 at some beta. Open as of 1984.Template:Update inline ?
8th (a) Formulation of the renormalization group Develop mathematically precise renormalization transformations for v-dimensional Ising-type systems. Open as of 1984.Template:Update inline ?
(b) Proof of universality Show that critical exponents for Ising-type systems with nearest neighbor coupling but different bond strengths in the three directions are independent of ratios of bond strengths.
9th (a) Asymptotic completeness for short-range N-body quantum systems Prove asymptotic completeness for N-body Schrödinger operators with short-range potentials (⊕RanΩa+=L2(X)).Template:Clarify Proved for generic N-body systems in 1987 by I. M. Sigal and A. Soffer;[14] and later by Jan Derezinski and C. Gérard.[15][16] 1987
(b) Asymptotic completeness for Coulomb potentials Suppose v=3,Vij(x)=eij|x|−1. Prove that ⊕RanΩaD,+=L2(X).Template:Clarify Open as of 1984.[8] ?
10th (a) Monotonicity of ionization energy (a) Prove that (ΔE)(N−1,Z)≥(ΔE)(N,Z).Template:Clarify Open as of 2026. ?
(b) The Scott correction Prove that the ground state energy of a heavy atom of atomic number Z follows the predicted asymptotic expansion, rigorously justifying the "Scott Correction" (c2Z2) to the Thomas-Fermi model. Proved by H. Siedentop and R. Weikard,[17][18] and later by C. Fefferman and L. Seco.[19] 1987
(c) Asymptotic ionization Find the leading asymptotics of (ΔE)(Z,Z).

Prove that the maximum number of electrons Nmax an atom can bind cannot exceed Z by more than a small amount.

Proved by Elliott H. Lieb and Michael Loss.[20] 2003
(d) Asymptotics of maximal ionized charge Prove that limZ→∞N(Z)/Z=1.Template:Clarify Proved by Fefferman and Seco.[21] 1997
(e) Rate of collapse of Bose matter Find suitable C1,C2,α such that −C1Nα≤E~B(N,N;1)≤C2Nα.Template:Clarify Open as of 2026. ?
11th Existence of crystals Prove a suitable version of the existence of crystals (e.g. there is a choice of minimizing configurations that converge to some infinite lattice configuration). Open as of 1984.Template:Update inline ?
12th (a) Existence of extended states in the Anderson model Prove that in v≥3 and for small λ that there is a region of absolutely continuous spectrum of the Anderson model, and determine whether this is false for v=2.Template:Clarify Open as of 1984.Template:Update inline ?
(b) Diffusive bound on "transport" in random potentials Prove that Exp(δ0,(eitHN→e−itH)2δ0)≤c(1+|t|) for the Anderson model, and more general random potentials.Template:Clarify
(c) Smoothness of k(E) through the mobility edge in the Anderson model Is k(E), the integrated density of states,Template:Clarify a C∞ function in the Anderson model at all couplings?
(d) Analysis of the almost Mathieu equation Verify the following for the almost Mathieu equation:
  • If α is a Liouville number and λ≠0, then the spectrum is purely singular continuous for almost all θ.
  • If α is a Roth number and |λ|<2, then the spectrum is purely absolutely continuous for almost all θ.
  • If α is a Roth number and |λ|>2, then the spectrum is purely dense pure point.
  • If α is a Roth number and |λ|=2, then σ(h) has Lebesgue measure zero and the spectrum is purely singular continuous.Template:Clarify
(e) Point spectrum in a continuous almost periodic model Show that −d2dx2+λcos⁡(2πx)+μcos⁡(2παx+θ) has some point spectrum for suitable α,λ,μ and almost all θ.
13th Critical exponent for self-avoiding walks Let D(n) be the mean displacement of a random self-avoiding walk of length n. Show that v:=limn→∞n−1ln⁡D(n) is 12 for dimension at least four and is greater otherwise. Open as of 1984.Template:Update inline ?
14th (a) Construct QCD Give a precise mathematical construction of quantum chromodynamics. Open as of 1984.Template:Update inline ?
(b) Renormalizable QFT Construct a nontrivial quantum field theory that is renormalizable but not superrenormalizable.
(c) Inconsistency of QED Prove that QED is not a consistent theory.
(d) Inconsistency of φ44 Prove that a nontrivial φ44 theory does not exist.
15th Cosmic censorship Formulate and then prove or disprove a suitable version of cosmic censorship. Open as of 1984.Template:Update inline ?

In 2000, Simon claimed five of the problems he listed (namely 1B, 9A, 10B, 10C and 10D, 12D) were solved.[1]

The 2000 list

The Simon problems as listed in 2000 (with original categorizations), are:[1][22]

No. Short name Statement Status Year solved
Quantum transport and anomalous spectral behavior
1st Extended states Prove that the Anderson model has purely absolutely continuous spectrum for v≥3 and suitable values of b−a in some energy range. ? ?
2nd Localization in 2 dimensions Prove that the spectrum of the Anderson model for v=2 is dense pure point. ? ?
3rd Quantum diffusion Prove that, for v≥3 and values of |b−a| where there is absolutely continuous spectrum, that ∑n∈ℤνn2|eitH(n,0)|2 grows like ct as t→∞. ? ?
4th Ten Martini problem Prove that the spectrum of hα,λ,θ is a Cantor set (that is, nowhere dense) for all λ≠0 and all irrational α. Solved by Puig (2003).[22][23] 2003
5th Prove that the spectrum of hα,λ,θ has measure zero for λ=2 and all irrational α. Solved by Avila and Krikorian (2003).[22][24] 2003
6th Prove that the spectrum of hα,λ,θ is absolutely continuous for λ=2 and all irrational α. ? ?
7th Do there exist potentials V(x) on [0,∞) such that |V(x)|≤C|x|12+ε for some ε and such that −d2dx2+V has some singular continuous spectrum? Essentially solved by Denisov (2003) with only L2 decay.

Solved entirely by Kiselev (2005).[22][25][26]

2003, 2005
8th Suppose that V(x) is a function on ℝν such that ∫|x|−ν+1|V(x)|2dνx<∞, where ν≥2. Prove that −Δ+V has absolutely continuous spectrum of infinite multiplicity on [0,∞). ? ?
Coulomb energies
9th Prove that N0(Z)−Z is bounded for Z→∞. ? ?
10th What are the asymptotics of (δE)(Z):=E(Z,Z−1)−E(Z,Z) for Z→∞? ? ?
11th Make mathematical sense of the nuclear shell model. ? ?
12th Is there a mathematical sense in which one can justify current techniques for determining molecular configurations from first principles? ? ?
13th Prove that, as the number of nuclei approaches infinity, the ground state of some neutral system of molecules and electrons approaches a periodic limit (i.e. that crystals exist based on quantum principles). ? ?
Other problems
14th Prove that the integrated density of states k(E) is continuous in the energy. | k(E1 + ΔE) − k(E1) | < ε ?
15th Lieb-Thirring conjecture Prove the Lieb-Thirring conjecture on the constants Lγ,ν where ν=1,12<γ<32. ? ?

See also

References

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