The most unexpected at LHC and the status of high energy frontier : proceedings of the International School of Subnuclear Physics / edited by Antonino Zichichi.

Format:

Book

Conference/Event

Author/Creator:

International School of Subnuclear Physics, Corporate Author.

Contributor:

Zichichi, Antonino.

Conference Name:

International School of Subnuclear Physics.

International School of Subnuclear Physics

Series:

Subnuclear series ; v. 47.

Subnuclear series ; v. 47

Language:

English

Subjects (All):

Large Hadron Collider (France and Switzerland)--Congresses.

Large Hadron Collider (France and Switzerland).

Nuclear physics--Congresses.

Nuclear physics.

Physical Description:

1 online resource (530 p.)

Place of Publication:

Singapore : World Scientific Pub. Co., 2012.

Language Note:

English

Summary:

Contents: Hot Theoretical Topics: Ultraviolet Behavior of N=8 Supergravity (L J Dixon); Is the Best Superstring Model NP Complete? (M R Douglas); Erice Lecture on Microscopic Gravity (G Dvali); Supergravity: Foundations and Applications (S Ferrara); Orienfold String Vacua and Strings at the LHC (D Luest); Seminar on Specialized Topics: Status of Dark Matter and Neutrino Physics (A Bettini); Experimental Evidence for Pointlike Baryons at q2 = 4MB2 (S Pacetti); Neutrino Masses, Dark Matter, Baryon Asymmetry and Inflation can be Explained at Once (M Shaposhnikov); Results from RHIC with Implicati

Contents:

PREFACE; CONTENTS; HOT THEORETICAL TOPICS; SEMINARS ON SPECIALIZED TOPICS; HIGHLIGHTS FROM LABORATORIES; SPECIAL SESSIONS FOR NEW TALENTS; CLOSING CEREMONY; Ultraviolet Behaviour of N = 8 Supergravity L. J. Dixon; 1 Introduction; 2 Divergences in quantum gravity; 3 Computational tools; 3.1 KLT relations; 3.2 Unitarity method; 3.3 Multi-loop generalized unitarity and maximal cuts; 3.4 Supersymmetric Ward identities and the rung rule; 4 KLT copying and rung-rule behavior; 5 N = 8 supergravity at three loops; 6 N = 8 supergravity at four loops; 7 Conclusions and Outlook; Acknowledgments

ReferencesDISCUSSION I; DISCUSSION II; Is the Best Superstring Model NP Complete? M. R. Douglas; 1 Introduction; 2 Spaces of quantum field theories; 2.1 Renormalization group; 2.2 General results; 2.3 Sigma models; 2.4 Space of manifolds with metric; 2.5 Ricci flow; 3 Linear sigma models; 3.1 Why is the linear sigma model good?; References; DISCUSSION I; DISCUSSION II; Erice Lecture on Microscopic Gravity G. Dvali; 1 The Hierarchy Problem; 2 The Role of Gravity; 3 Generalized Planck Length; 4 Gravity and Species; 4.1 Bound on the UV-Scale From Black Hole Evaporation

4.2 Species Scale from the Black Hole Barrier of Information Storage4.3 Kaluza-Klein Species; 4.4 Non-Gravitational Species and Hierarchy Problem; Acknowledgments; References; DISCUSSION I; DISCUSSION II; Supergravity: Foundations and Applications S. Ferrara; 1 Foundations; 1.1 Mathematical Structure; 1.2 Super gravity lagrangians and susy rules in N-extended supergravities; 2 Applications; 2.1 Spontaneous Supersymmetry Breaking; 2.2 Extremal Black Holes; References; DISCUSSION I; DISCUSSION II; Orientifold String Vacua and Strings at the LHC D. Luest; 1 Introduction

2 Length scales and string excitations in D-brane orientifold com pactifications2.1 Various choices for the string scale; 2.2 Several generic particles in brane compactifications and their associated length scales; 3 Production of heavy string Regge excitations and KK/winding states at the LHC; 3.1 Two gluon, two quark scattering amplitudes; 3.2 Four quark scattering amplitudes; 3.3 Signals for lowest mass strings at the LHC; 4 Conclusions; Acknowledgements; References; DISCUSSION I; DISCUSSION II; Status of Dark Matter and Neutrino Physics A. Bettini; 1. Status of the ACDM cosmological model

2. The present status of neutrino physics3. Neutrino nature and masses; 4. Direct search for dark matter; 5. Conclusions; References; DISCUSSION; Experimental Evidence for Pointlike Baryons at q2 = 4M2B S. Pacetti; 1 Introduction; 2 Baryon cross section and form factors; 3 (e+e + pp) at threshold; 4 Other charged baryon form factors at threshold; 4.1 The AE+ E; channel; 4.2 The p (1440)+c.c. channel; 5 The neutral baryons puzzle; 6 Conclusions; References; DISCUSSION; Neutrino Masses, Dark Matter, Baryon Asymmetry and Inflation can be Explained at Once M. Shaposhnikov; 1 Introduction

2 Construction of the Minimal Model

Notes:

Description based upon print version of record.

Includes bibliographical references.

ISBN:

981-4374-12-1

OCLC:

794328362