curves (movie by Noguchi 2004) Prad = 2e2(F|| 2 g2F 2) /3c ... Currently the WG has ~ 30 international members on the. mailing list. High Energy. Astrophysics ...
Coordinate difference (comoving distance) is not the same as physical distance. Can rewrite conformal ... Affine parameter can be replaced by comoving distance ...
... the first. luminous structures. Dark Ages. Twilight Zone ... Reionization: the movie. 8Mpc comoving. Barkana and Loeb 2001. Constraint I: Gunn-Peterson Effect ...
Reionization: the movie. 8Mpc comoving. Constraint I: Gunn-Peterson Effect. Fan et al 2006 ... Twilight zone': study of first light limited to near-IR to radio l's ...
dP(t) = a(t) dr = a(t) r (dP is not a comoving distance) but we know for light emitted at ... fortunately at different times different components will dominate ...
Formation rate of galaxies per comoving volume ... scale clustering of galaxies within a single halo. large scale clustering of galaxies in different halos ...
These are necessary in order to transport the energy to the required distances, ... The time scales are given in units of the comoving blob crossing time. TEST ...
Note: comover dissociation as well as DDbar recombination can occure only if the ... Dissociation energy density: e(J/Y )=16 GeV/fm3, e(cc ) =2 GeV/fm3, e(Y ' ...
Use calculated tQ and measured f to find n ?(Lpeak) And you get. Simulation ... Getting Quasar Creation Rate n. ? f = the comoving number density of quasars in ?log L ...
Title: Galaxy Formation and Evolution Author: Kenneth M. Lanzetta Last modified by: Kenneth M. Lanzetta Created Date: 11/19/2002 6:57:14 PM Document presentation format
Universidade de Santiago de Compostela, Spain ... La Thuile, Aosta valley, Italy March 8th ... arXiv:0801.4949 E. G. Ferreiro, F. Fleuret, A. Rakotozafindrabe ...
Disentangling dynamic and geometric distortions Federico Marulli Dipartimento di Astronomia, Universit di Bologna Marulli, Bianchi, Branchini, Guzzo, Moscardini and ...
Galaxy Evolution and WFMOS History of Galaxies Present-day Universe: SDSS WFMOS Survey of z1 Universe K. Shimasaku (University of Tokyo) galaxy morphology galaxy ...
Title: PowerPoint Presentation Last modified by: Robert Jedicke Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles
Dark Ages: only probe! Spectral line: measure entire history ... The Dark Ages. Straightforward physics ... Dark Ages: 'clean' probe of cosmology and of exotic ...
(anti)shadowing. saturation, color glass condensate. suppression via ... Light systems and peripheral Pb-Pb collisions: J/? is absorpted by nuclear matter. ...
We calculated an Anisotropic Correlation Function, ?(s,s//), from SDSS LRG ... survey such as WFMOS (Wide-Field Multi-Object Spectrograph) gets available. ...
... Modeling the Universe BASIC COSMOLOGICAL ASSUMPTIONS Germany 1915: Einstein just completed theory of GR Explains anomalous orbit of Mercury perfectly ...
Panoramic Survey of the Deep Universe Observing Galaxy Formation at High Redshift Toru Yamada National Astronomical Observatory of Japan Opt/IR Div., Subaru Telescope
J/Y, Charm and intermediate mass dimuons in Indium-Indium collisions, not RHIC! Results from recent data (year 2003) from SPS Time is limited. I will focus on open ...
To catch the sign of proton acceleration. GLAST will be Launched May in this year. ... Proton acceleration efficiency. We need 6-8 1043 ergs/Mpc3/yr to explain UHECRs ...
35% of bulge-dominated galaxies experienced a merger with mass ratio 1:4 in the ... For both field and cluster galaxies, the merger events are dominated by Sp-Sp ...
DEPARTAMENTO DE ENSINO DOUTRIN RIO CURSO DE EXPOSITOR ESP RITA (Org. por S rgio Biagi Greg rio) 22/01/2002 Curso de Expositor Esp rita No plano da orat ria ...
Charmonia production in heavy ion collisions, from SPS to LHC * FR D RIC FLEURET LLR CNRS/IN2P3 cole polytechnique Palaiseau, France * F. Fleuret LLR-CNRS ...
It is concluded that J/Y suppression in nuclear collisions should provide an unambigous ... Absorption attendue RHIC. Rhic : shadowing des pdf. Etretat - Sept. ...
Distortion due to non-linear evolution, peculiar velocities and galaxy bias ... P(k) / Pref(Wbaryon=0) Also detected in SDSS LRG sample (Eisenstein etal 05) ...
Astrophysical Cosmology Andy Taylor Institute for Astronomy, University of Edinburgh, Royal Observatory Edinburgh The large-scale distribution of galaxies Temperature ...
based on dynamical models transport approaches and hydrodynamics ... 3D-fluid hydrodynamical model gives the right slope! Is the matter a parton liquid? ...
Constraints on Non-Acceleration Models A comment on extragalactic magnetic fields Top-down models Avoiding the GZK cut-off : The Z-burst and new physics
REW 0.3 Angstrom ... REW=1 Angstrom black absorption 107 ... Only have analyzed 243 MgII systems with kinematically extreme absorption (REW 2 Angstroms) ...
... is ionized, baryons and photons are coupled via. Thomson scattering: we refer to a 'photon-baryon fluid' ... Increasing the baryon density increases the density ...
Laboratoire de Physique des Lasers. Universit Paris Nord and CNRS. Villetaneuse, France ... m accumulates the phase mf with f = Final amplitude. a0 = cc' ss' cos f ...
Early dust in the galaxy structure formation opens up the possibility that ' ... Thanks for the practice of 16 strings and the 7 last words (Haydn) ...
Roberto Decarli Dark Matter Nature First evidences of Dark Matter in Universe Baryonic or non baryonic? Thermal or non thermal? Hot, Warm, Cold or other?
Cosmic Acceleration: Back-Reaction vs. Dark Energy (with: Rocky Kolb & Toni Riotto) ... Only about 4% of the cosmic energy budget is in the form of ordinary 'baryonic' ...
Assume that the Universe is homogenous and isotropic, and therefore described by ... where k = 1, -1 or 0 for a closed, open and flat universe, respectively, ...
Some people love hot girls: R. Snellings. Others prefer hot guys: C. Markert ... Production increases more quickly for hadrons with three instead of two quarks ...