• WordNet 3.6
    • n Riemann pioneer of non-Euclidean geometry (1826-1866)
    • ***


In literature:

The twenty-seven studies of Chopin have been separately edited by Riemann and Von Bulow.
"Chopin: The Man and His Music" by James Huneker
Riemann, H. Dictionary of music.
"A Library Primer" by John Cotton Dana
Riemann Dr. H. 27 (note), 185, 238.
"The Pianoforte Sonata" by J.S. Shedlock
Benoist, O. Riemann and C. Graux; (in archaeology) A.C. Quatremere de Quincy, P. le Bas, C.F.M.
"Encyclopaedia Britannica, 11th Edition, Volume 6, Slice 4" by Various
Weber, G.F. Riemann and S.D.
"Encyclopaedia Britannica, 11th Edition, Volume 3, Slice 6" by Various
Riemann proceeds to specialize the manifold by considerations as to measurement.
"Encyclopaedia Britannica, 11th Edition, Volume 11, Slice 6" by Various

In news:

Riemann Family Funeral Home of Gulfport is in charge of arrangements.
Riemann conjectured that these key signposts—"zeros" of the function—all lie on a single straight line out to infinity, that none are flung off in strange places.
Thoughts on the Riemann Hypothesis .
The simultaneous appearance in May 2003 of four books on the Riemann hypothesis (RH) provoked these reflections.
Manu Ginobili celebrates after solving the Riemann Hypothesis.
As I write, they have calculated "935.7 billion nontrivial zeros of the Riemann zeta function in 1146 days".

In science:

In the holomorphic case, these functions are CR functions; i.e., they satisfy the tangential Cauchy-Riemann equations ∂b ˆs = 0.
Universality and scaling of zeros on symplectic manifolds
Deift, Orthogonal polynomials and random matrices: a Riemann-Hilbert approach.
Universality and scaling of zeros on symplectic manifolds
Hence, at least in this case, which is related to the zeroes of the Riemann zeta function [KeaSn], the study of eigenvalues is the same as the study of conjugacy classes.
Random matrix theory over finite fields: a survey
F (z) so as to make the Riemann-tensor to vanish.
Quantum Theory within the Framework of General Relativity
Lg is the gravitational Lagrangian density, R is the scalar curvature of the Riemann-Cartan space-time.
Angular momentum conservation law in Einstein-Cartan space-time