
Roman Scoccimarro
Professor
Probing Newton's constant on vast scales: DGP gravity, cosmic acceleration, and large scale structure. A. Lue, R.S. & G. Starkman, Phys. Rev. D69, 124015 (2004).
Redshift-space distortions, pairwise velocities, and nonlinearities. R.S., Phys. Rev. D70, 083007 (2004).
Differentiating between modified gravity and dark energy. A. Lue, R.S. & G. Starkman, Phys. Rev. D69, 044005 (2004).
PTHalos: A fast method for generating mock galaxy distributions. R.S. & Ravi Sheth, MNRAS, 329, 629 (2002).
Constraints on Galaxy Bias, Omega_m, and Primordial Non-Gaussianity from the PSCz Survey Bispectrum. H. Feldman, J. Frieman, J.N. Fry, & R.S., Phys.Rev.Lett 86, 1434 (2001).
How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering. R.S., R. Sheth, L. Hui, B. Jain, ApJ 546, 20 (2001).
Power Spectrum Correlations Induced by Non-Linear Clustering. R.S., M. Zaldarriaga & L. Hui, Ap.J. 527, 1 (1999).
The Impact of Inhomogeneous Reionization on Cosmic Microwave Background Anisotropy. L. Knox, R.S., & S. Dodelson, Phys.Rev.Lett., 81, 2004 (1998).
Contact Information
Roman Scoccimarro
Professor scoccima@physics.nyu.edu 726 Broadway, Room 952New York, NY 10003
Phone: (212) 992-8786