| 10401 |
|
The Boundary Value Problem for the Stationary and Axisymmetric Einstein Equations is Generically Solvable
|
Schaudt, U. M
|
American Physical Society
|
1980
|
|
|
|
| 10402 |
|
The Case against Scaling Defect Models of Cosmic Structure Formation
|
Albrecht, A
|
American Physical Society
|
1980
|
|
|
|
| 10403 |
|
The Central Density of Neutron Stars in Close Binaries
|
Wiseman, A. G
|
American Physical Society
|
1980
|
|
|
|
| 10404 |
|
The cosmological constant and dark energy/
|
Peebles, P. J. E
|
American Physical Society
|
2003
|
|
|
|
| 10405 |
|
The Critical Line of an Ising Antiferromagnet on Square and Honeycomb Lattices
|
Wang, X.-Z
|
American Physical Society
|
1980
|
|
|
|
| 10406 |
|
The discovery of the top quark
|
Franklin, M. Campagnari, C.
|
American Physical Society
|
1997
|
|
|
|
| 10407 |
|
The Dynamics of Curved Fronts: Beyond Geometry
|
Hagberg, A
|
American Physical Society
|
1980
|
|
|
|
| 10408 |
|
The Dynamics of Multidimensional Secession: Fixed Points and Ideological Condensation/
|
Soulier, A
|
American Physical Society
|
2003
|
|
|
|
| 10409 |
|
The eighteen arbitrary parameters of the standard model in your everydaylife
|
Cahn, R. N.
|
American Physical Society
|
1996
|
|
|
|
| 10410 |
|
The Energy Dependence of Flow in Ni Induced Collisions from 400A to 1970A MeV
|
Chance, J
|
American Physical Society
|
1980
|
|
|
|
| 10411 |
|
The extraordinary phases of liquid ^3He
|
Lee, D. M.
|
American Physical Society
|
1997
|
|
|
|
| 10412 |
|
The fundamental constants and their variation: observational and theoretical status/
|
Uzan, J.-P
|
American Physical Society
|
2003
|
|
|
|
| 10413 |
|
The Gravitational Constant, the Chandrasekhar Limit, and Neutron Star Masses
|
Thorsett, S. E
|
American Physical Society
|
1980
|
|
|
|
| 10414 |
|
The ground-state phase diagram of the one-dimensional Kondo lattice model
|
Ueda, K. Sigrist, M. Tsunetsugu, H.
|
American Physical Society
|
1997
|
|
|
|
| 10415 |
|
The Homologous Contraction of a Sonoluminescing Bubble
|
Chu, M.-C
|
American Physical Society
|
1980
|
|
|
|
| 10416 |
|
The interstellar environment of our galaxy - The interstellar medium has an ambient pressure of only 10-20 atmospheres, but its composition is quite rich, ranging from molecules and dust grains to cosmics rays, all in a magnetic field of a few hundred microT. The cycling of matter form stars to interstellar medium and back varies depending on the medium's characteristics. This article discusses the components of the medium, their interactions, and their relationships to the stars./
|
Ferri�re, Katia M
|
American Physical Society
|
2001
|
|
|
|
| 10417 |
|
The Kondo Screening Cloud: What Can We Learn from Perturbation Theory?
|
Barzykin, V
|
American Physical Society
|
1980
|
|
|
|
| 10418 |
|
The Light Quark Masses from Lattice Gauge Theory
|
Gough, B
|
American Physical Society
|
1980
|
|
|
|
| 10419 |
|
The low-Q^2, low-x region in electroproduction - an overview
|
Badelek, B. Kwiecinski, J.
|
American Physical Society
|
1996
|
|
|
|
| 10420 |
|
The microscopic magnetization: concept and application
|
Hirst, L. L.
|
American Physical Society
|
1997
|
|
|
|
