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Theoretical physicists working at a blackboard collaboration pod in the Beecroft building.
Credit: Jack Hobhouse

Professor James Binney FRS

Emeritus Professor

Sub department

  • Rudolf Peierls Centre for Theoretical Physics

Research groups

  • Theoretical astrophysics and plasma physics at RPC
James.Binney@physics.ox.ac.uk
Telephone: 01865 (2)73979
Rudolf Peierls Centre for Theoretical Physics, room 50.3
  • About
  • Publications

The shape of the disk: Clues from the kinematics of disk stars

UNSOLVED PROBLEMS OF THE MILKY WAY (1996) 11-21

Authors:

MD Weinberg, P Schechter, J Binney, T deZeeuw

The stellar-dynamical oeuvre

JOURNAL OF ASTROPHYSICS AND ASTRONOMY 17:3-4 (1996) 81-94

EVOLVING COOLING FLOWS

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 276:2 (1995) 663-678

Authors:

J BINNEY, G TABOR

Probing non-axisymmetry with proper motions

ASTRONOMICAL AND ASTROPHYSICAL OBJECTIVES OF SUB-MILLIARCSECOND OPTICAL ASTROMETRY (1995) 239-246

The Principle of Least Action and Clustering in Cosmology

Mon.Not.Roy.Astron.Soc. 271 (1994) 719-719

Authors:

M Susperregi, J Binney

Abstract:

A scheme is developed which enables one to trace backwards in time the cosmic density and velocity fields, and to determine accurately the current-epoch velocity field from the current-epoch density field, or vice versa. The scheme implements the idea of Giavalisco \etal\ (1993) that the principle of least action should be used to formulate gravitational instability as a two-point boundary-value problem. We argue that the Eulerian formulation of the problem is to be preferred to the Lagrangian one, on grounds of computational simplicity, of ease of interfacing with observational data, and of internal consistency at early times. The scheme is successfully tested on an exact solution in one dimension, and on currently Gaussian fields in one and two dimensions. The application of the scheme to real observational data appears to be eminently feasible, though computationally costly.

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