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Preprint servers and journal databases
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[astro-ph/0505266] Alternatives to Dark Matter and Dark Energy Philip D. Mannheim (University of Connecticut) + [gr-qc/9611038] Local and global gravity + [astro-ph/9602094] Linear potentials and galactic rotation curves - detailed fitting
Terms: second order Poisson equation (5), fourth order Poisson (20), modified newtonian dynamics (10000), higher order Poisson (10),
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Terms: galactic halos (11500), galactic dark matter (5090), galaxy halos (6450), flat rotation curve (2050), flat rotation curves (2710), galactic rotation curves (2630), galactic rotation (31700), rotation curve systematics (4),
Terms: annual modulation (3720), annual modulation signatures (9), annual modulation signature (778), cosmic astigmatism (), correlated galaxy ellipticities (),
Terms: photino (9780), neutralino (55300), weak scale gravitinos (19), heavy gaugino (14), dark energy (620000),
Terms: WIMP-nucleon (1920), WIMP nuclear (35), dark matter detectors (2680), dark matter particles (12700), dark matter particle (3650), search for dark matter particles (442), direct detection of dark matter (1320), WIMP dark matter (3520), elastic scattering of dark matter (12), terrestrial dark matter detectors (4),
Terms: phonons and ionization (37), ionization and phonons (12), phonon and ionization (18), thermal and ionization signals (13),
Berkeley - Cosmic Dark Matter Search (CDMS) Publications
McMaster Canada - Massive Compact Halo Objects
Terms: Massive Compact Halo Objects (8420), MACHO Project (9870), UK Dark Matter Collaboration (3000),
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Terms: dark matter distribution (8590), distribution of dark matter (13100), mass density fluctuations (), cosmic mass distributions (), gravitational distortions (), cosmological weak shear (), cosmic shear (),
[astro-ph/0212390] The Dark Matter Distribution in Galaxy Cluster Cores
CFHT Gives First Glimpse of Dark Matter Distribution Canada France Hawaii Telescope Corporation
Terapix - DESCART
[astro-ph/0409224] Constraints on higher-dimensional gravity from the cosmic shear three-point correlation function - In particular it is shown here that the behavior of the density field bi-spectrum is sensitive to departure from normal gravity ... The cosmic shear bispectrum appears to be particularly sensitive to changes in the Poisson equation: we show that the current cosmic shear data can already be used to infer constraints on the scale of a possible higher-dimensional gravity, above 2 h^{-1}Mpc