124556579
Motivation and goals of ERL 2005
Various types of ERL sources are introduced, the relevant beam physics and accelerator technology issues noted, innovative areas of development identified and current and future goals of ERL research and development established.
9548066
ALL OPTICAL ACCELERATOR EXPERIMENTS AT LBNL
An overview is presented of the status of laser wakefield acceleration research at the l’OASIS laboratory of the Center for Beam Physics at LBNL. Experiments have been performed on laser driven production of relativistic electron beams from plasmas using a high repetition rate (10 Hz), high power (10 TW) Ti:sapphire (0.8 „m ) laser system. Large amplitude plasma waves have been excited in the self-modulated laser wakefield acceleration regime by tightly focusing (spot diameter 8 „m ) a single high power (up to 10 TW), ultra-short (‚ 50 fs) laser pulse onto a high density (> 1019 cmi 3) pulsed gasjet of length 1.2 mm. Nuclear activation measurements in lead and copper targets indicate the production of electrons with energy in excess of 25 MeV. This result was confirmed by electron distribution measurements using a bending magnet spectrometer. Progress on implementing the colliding pulse laser injection method is also presented. This method is expected to produce low emittance (< 1... mm-mrad), low energy spread (< 1% ), 40 MeV femtosecond duration electron bunches containing 107 electrons/bunch.
27302633
Advanced Accelerator Technologies - A Snowmass'96 Subgroup Summary
The authors address the collider physics issues, concepts and technologies of (e{sup +}e{sup -}{gamma}) colliders at a cm. energy of 5 TeV and a luminosity of 10{sup 35} cm{sup -2}s{sup -1}.
123445623
Free electron lasers for gamma-gamma colliders — a summary
119954902
Study of Thermodynamic Quantities in Horava-Lifshitz and f(R) gravity Theories
The present paper reports studies on thermodynamic quantities like temperature of the universe, heat capacity and squared speed of sound in f(R) and Horava-Lifshitz gravity theories. Considering the universe to be filled with dark matter and dark energy we have shown that in all cases the equation of state behaves like quintessence. The thermodynamic quantities have been studied graphically by plotting them against redshift z.
5875803
Tachyonic field interacting with scalar (phantom) field
In this letter, we have considered the universe is filled with the mixture of tachyonic field and scalar or phantom field. If the tachyonic field interacts with scalar or phantom field, the interaction term decays with time and the energy for scalar field is transferred to tachyonic field or the energy for phantom field is transferred to tachyonic field. The tachyonic field and scalar field potentials always decrease, but phantom field potential always increases.
120262865
On the various aspects of interacting Ricci dark energy and tachyonic field
In this letter we considered an interaction between Ricci dark energy and tachyonic field. We investigated the equation of state parameters in presence of the interaction and revealed a quintessence like behavior. Also, we investigated the validity of the generalized second law of thermodynamics in presence of this interaction and observed that it is broken down under this interaction.
120207132
New holographic dark energy in modified f(R) Horava-Lifshitz gravity
In this paper, we study the new holographic dark energy model in the framework of modified f(R) Horava-Lifshitz Gravity. We apply correspondence scheme to construct model the in underlying scenario using power-law form of scale factor. To explore accelerated expansion of the universe, some well-known cosmological parameters (equation of state parameter and squared speed of sound) and cosmological planes (ωΛ–$\omega'_{\varLambda}$ and statefinder) are discussed for reconstructed model. It is interesting to conclude that these parameters represent phantom behavior of the universe with stable configuration. also, the cosmological planes show compatible results with recent observations for accelerated expansion of the universe.
14838499
Density evolution in the new modified Chaplygin gas model
In this paper, we have considered a new modified Chaplygin gas (NMCG) model which interpolates between radiation at an early stage and ΛCDM at a late stage. This model is regarded a unification of dark energy and dark matter (with a general form of matter). We have derived the density parameters from the equation of motion for interaction between dark energy and dark matter. Also, we have studied the evolution of various components of the density parameters.