Pairs-Production of Higgs in Association with Bottom Quarks Pairs at e+e−e^+e^- Colliders

In a previous paper, we studied the Higgs pair production in the standard model with the reaction $e^{+}e^{-}\to t \bar t HH$. Based on this, we study the Higgs pair production via $e^{+}e^{-}\to b \bar b HH$. We evaluate the total cross section of $b\bar bHH$ and calculate the number total of events considering the complete set of Feynman diagrams at tree-level, and compare this process with the process $e^{+}e^{-}\to t \bar t HH$. The numerical computation is done for the energy which is expected to be available at a possible Next Linear $e^{+}e^{-}$ Collider with a center-of-mass energy $800, 1000, 1600$ $GeV$ and luminosity 1000 $fb^{-1}$.Comment: 12 pages, 6 figure

Aspectos de los sistemas tributarios en los países andinos que preocupan a los inversionistas extranjeros

Estamos complacidos con la oportunidad que nos brinda el Banco Interamericano de Desarrollo de compartir, con los protagonistas del desarrollo e integración económica en los países de la Comunidad Andina de Naciones, algunos de los aspectos de sus sistemas tributarios que en nuestra experiencia generan ciertos problemas a las empresas multinacionales desarrollando negocios en estas jurisdicciones.Política fiscal, Sistemas tributarios, países Andinos, Inversionistas

Corporate governance facing corporate social responsability: solving challenges in the 21st century

17 páginasWithin the context of modern Corporate Governance and particularly in the aftermath of the financial scandals of the XXIst Century, companies, regulators, markets and the public in general claim for more transparency, accountability, shareholders and investor protection. There is also a trend towards reinforcing the Responsibility of Companies towards the Communities in which they develop their businesses. However, generally speaking shareholders do not have a direct control nor saying in management; and stakeholders possibility of influencing corporations’ decisions seems very rare. This article reviews some of the existing corporate cultural and legal systems and provides ideas for future development of corporate Governance in de field of Share- and Interest- -Holders’ protectionS

LCG Service Challenge 3 at the Spanish Tier-1 and Tier-2 sites

This note describes the participation of the Spanish centres PIC and CIEMAT in the LCG Service Challenge 3 as Tier-1 and Tier-2 sites respectively. Data transfer, job submission and data throughput from mass storage to the data processing jobs have been successfully exercised at the desired level. Very valuable experience has been gained running the complex computing system under realistic conditions at a signi cant scale

The Collimated Jet Source in IRAS 16547-4247: Time Variation, Possible Precession, and Upper Limits to the Proper Motions Along the Jet Axis

The triple radio source detected in association with the luminous infrared source IRAS 16547-4247 has previously been studied with high angular resolution and high sensitivity with the Very Large Array (VLA) at 3.6-cm wavelength. In this paper, we present new 3.6 cm observations taken 2.68 years after the first epoch that allow a search for variability and proper motions, as well as the detection of additional faint sources in the region. We do not detect proper motions along the axis of the outflow in the outer lobes of this source at a 4-$\sigma$ upper limit of $\sim$160 km s$^{-1}$. This suggests that these lobes are probably working surfaces where the jet is interacting with a denser medium. However, the brightest components of the lobes show evidence of precession, at a rate of $0\rlap.^\circ08$ yr$^{-1}$ clockwise in the plane of the sky. It may be possible to understand the distribution of almost all the identified sources as the result of ejecta from a precessing jet. The core of the thermal jet shows significant variations in flux density and morphology. We compare this source with other jets in low and high mass young stars and suggest that the former can be understood as a scaled-up version of the latter.Comment: 26 pages, 9 figure

The Rotating Molecular Structures and the Ionized Outflow Associated with IRAS 16547-4247

We present VLA 1.3 cm radio continuum and water maser observations as well as SMA SO$_2$ (226.300 GHz) and 1.3 mm dust continuum observations toward the massive star formation region IRAS 16547-4247. We find evidence of multiple sources in the central part of the region. There is evidence of a rotating structure associated with the most massive of these sources, traced at small scales (~50 AU) by the water masers. At large scales (~1000 AU) we find a velocity gradient in the SO2 molecular emission with a barely resolved structure that can be modeled as a rotating ring or two separate objects. The velocity gradients of the masers and of the molecular emission have the same sense and may trace the same structure at different size scales. The position angles of the structures associated with the velocity gradients are roughly perpendicular to the outflow axis observed in radio continuum and several molecular tracers. We estimate the mass of the most massive central source to be around 30 solar masses from the velocity gradient in the water maser emission. The main source of error in this estimate is the radius of the rotating structure. We also find water masers that are associated with the large scale molecular outflow of the system, as well as water masers that are associated with other sources in the region. Our results suggest that the formation of this source, one of the most luminous protostars or protostellar clusters known, is taking place with the presence of ionized jets and disk-like structures.Comment: 26 pages, 7 figure