Chair : Cédric DEFFAYET

نویسنده

  • Cédric DEFFAYET
چکیده

“standard model” of particles physics, which describes with great success all the known most intimate building block of nature. More concretely, it gives a unified description of all the known particles and of three of the four fundamental interactions at work in nature: the electromagnetic interaction, the so-called “strong” interaction and the so-called “weak” interaction. This standard model is expressed in the framework of a so-called “quantum theory of fields”, that is to say a theory which follows the principle of quantum mechanics but also those of special relativity, which were both enunciated in the first half of the last century. This remarkable achievement was made possible and has been tested with great precisions during many years thanks to particle accelerators such as the ones operating at CERN, in Geneva, the European Organization for Nuclear Research (an unfortunate name, since the last and this will also be true for the next generation of CERN accelerators was in fact able to explore sizes much smaller that the one of an atomic nucleus). The standard model is believed to describe at the most intimate level known today all the known phenomena of nature, hence for example, it is in principle possible (but can be very hard in practice) to use the standard model not only to describe what is going on inside a proton, one of the constituent of the atomic nucleus, but also to compute say the physical properties of liquid water or those of reinforced concrete. The standard model has been tested with great precision in particle accelerator, it also enables to give a successful description of an early period of the history of the Universe. However, one of the major piece of the standard model has still to be discovered, the so-called Higgs boson which is associated with the way particle masses are described. Moreover various arguments make one believe that the model has to be modified to describe phenomena occurring at energy slightly higher than those reached in the last generation of accelerators. It is the goal of the future CERN accelerator, named LHC (standing for “Large Hadron Collider”) to explore those INTRODUCTION

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Accelerated Universe from Gravity Leaking to Extra Dimensions

We discuss the idea that the accelerated Universe could be the result of the gravitational leakage into extra dimensions on Hubble distances rather than the consequence of non-zero cosmological constant. e-mail [email protected]

متن کامل

Non-conventional cosmology from a brane-universe

We consider “brane-universes”, where matter is confined to four-dimensional hypersurfaces (three-branes) whereas one extra compact dimension is felt by gravity only. We show that the cosmology of such branes is definitely different from standard cosmology and identify the reasons behind this difference. We give a new class of exact solutions with a constant five-dimensional radius and cosmologi...

متن کامل

Supernovae, CMB, and Gravitational Leakage into Extra Dimensions

We discuss observational constraints coming from CMB and type Ia supernovae, for the model of accelerated universe produced by gravitational leakage into extra dimensions. Our fits indicate that the model is currently in agreement with the data. We also give the equations governing the evolution of cosmological perturbations. Future observations will be able to severely constrain the model.

متن کامل

The radion in brane cosmology

We consider the homogeneous cosmological radion, which we define as the interbrane distance in a two-brane and Z2 symmetrical configuration. In a coordinate system where one of the brane is at rest, the junction conditions for the second (moving) brane give directly the (non-linear) equations of motion for the radion. We analyse the radion fluctuations and solve the non-linear dynamics in some ...

متن کامل

A note on the wellposedness of scalar brane world cosmological perturbations

We discuss scalar brane world cosmological perturbations for a 3-brane world in a maximally symmetric 5D bulk. We show that Mukoyama’s master equations leads, for adiabatic perturbations of a perfect fluid on the brane and for scalar field matter on the brane, to a well posed problem despite the non local aspect of the boundary condition on the brane. We discuss in relation to the wellposedness...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2008