Lepton Probes in Nuclear Physics
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How to Hack a Turned-Off Computer Or Running Unsigned
HOW TO HACK A TURNED-OFF COMPUTER, OR RUNNING UNSIGNED CODE IN INTEL ME Contents Contents ................................................................................................................................ 2 1. Introduction ...................................................................................................................... 3 1.1. Intel Management Engine 11 overview ............................................................................. 4 1.2. Published vulnerabilities in Intel ME .................................................................................. 5 1.2.1. Ring-3 rootkits.......................................................................................................... 5 1.2.2. Zero-Touch Provisioning ........................................................................................... 5 1.2.3. Silent Bob is Silent .................................................................................................... 5 2. Potential attack vectors ...................................................................................................... 6 2.1. HECI ............................................................................................................................... 6 2.2. Network (vPro only)......................................................................................................... 6 2.3. Hardware attack on SPI interface ..................................................................................... 6 2.4. Internal file system ......................................................................................................... -
Issue #63, July 2000 Starting Our SIXTH Year in Publishing!
Issue #63, July 2000 Starting our SIXTH year in publishing! 64a Page 1 Wed, Jul 2000 Cover by: Bill Perry [email protected] Published by My Mac Productions 110 Burr St., Battle Creek, MI 49015-2525 Production Staff Tim Robertson • [email protected] Publisher / Creator / Owner Editor-in-Chief Adam Karneboge • [email protected] Webmaster / Contributing Editor Roger Born • [email protected] Website Edior Barbara Bell • [email protected] Director, Public Relations •Jobs & Woz • Inspiration Artwork Created by: •Mike Gorman• [email protected] •Bill Perry• [email protected] •Tim Robertson• [email protected] •Adam Karneboge• [email protected] This Publication was created with: DOCMaker v4.8.4 http://www.hsv.tis.net/~greenmtn & Adobe Acrobat 4.0 http://www.adobe.com 64a Page 2 Wed, Jul 2000 Other Tools: Adobe Photoshop 5.5, 5.0.1 ColorIt! 4.0.1 BBEdit Lite ClarisWorks 5.0 Microsoft Word 98 GraphicConverter Snapz Pro 2.0 SimpleText Netscape Communicator 4.6.1 Internet Explorer 4.5 Eudora Pro 4.0.2 FileMaker Pro 4.0v3 QuickKeys 4.0 and the TitleTrack CD Player (To keep us sane!) Website hosted by Innovative Technologies Group Inc. http://www.inno-tech.com My Mac Magazine ® 1999-2000 My Mac Productions. All Rights Reserved. 64a Page 3 Wed, Jul 2000 http://www.inno-tech.com http://www.smalldog.com http://www.megamac.com 64a Page 4 Wed, Jul 2000 Advertising in My Mac = Good Business Sense! With over 500,000 website visits a month and thousands of email subscribers, You just can't go wrong! Send email to [email protected] for information. -
B2.IV Nuclear and Particle Physics
B2.IV Nuclear and Particle Physics A.J. Barr February 13, 2014 ii Contents 1 Introduction 1 2 Nuclear 3 2.1 Structure of matter and energy scales . 3 2.2 Binding Energy . 4 2.2.1 Semi-empirical mass formula . 4 2.3 Decays and reactions . 8 2.3.1 Alpha Decays . 10 2.3.2 Beta decays . 13 2.4 Nuclear Scattering . 18 2.4.1 Cross sections . 18 2.4.2 Resonances and the Breit-Wigner formula . 19 2.4.3 Nuclear scattering and form factors . 22 2.5 Key points . 24 Appendices 25 2.A Natural units . 25 2.B Tools . 26 2.B.1 Decays and the Fermi Golden Rule . 26 2.B.2 Density of states . 26 2.B.3 Fermi G.R. example . 27 2.B.4 Lifetimes and decays . 27 2.B.5 The flux factor . 28 2.B.6 Luminosity . 28 2.C Shell Model § ............................. 29 2.D Gamma decays § ............................ 29 3 Hadrons 33 3.1 Introduction . 33 3.1.1 Pions . 33 3.1.2 Baryon number conservation . 34 3.1.3 Delta baryons . 35 3.2 Linear Accelerators . 36 iii CONTENTS CONTENTS 3.3 Symmetries . 36 3.3.1 Baryons . 37 3.3.2 Mesons . 37 3.3.3 Quark flow diagrams . 38 3.3.4 Strangeness . 39 3.3.5 Pseudoscalar octet . 40 3.3.6 Baryon octet . 40 3.4 Colour . 41 3.5 Heavier quarks . 43 3.6 Charmonium . 45 3.7 Hadron decays . 47 Appendices 48 3.A Isospin § ................................ 49 3.B Discovery of the Omega § ...................... -
Pair Energy of Proton and Neutron in Atomic Nuclei
International Conference “Nuclear Science and its Application”, Samarkand, Uzbekistan, September 25-28, 2012 Fig. 1. Dependence of specific empiric function Wigner's a()/ A A from the mass number A. From the expression (4) it is evident that for nuclei with indefinitely high mass number ( A ~ ) a()/. A A a1 (6) The value a()/ A A is an effective mass of nucleon in nucleus [2]. Therefore coefficient a1 can be interpreted as effective mass of nucleon in indefinite nuclear matter. The parameter a1 is numerically very close to the universal atomic unit of mass u 931494.009(7) keV [4]. Difference could be even smaller (~1 MeV), if we take into account that for definition of u, used mass of neutral atom 12C. The value of a1 can be used as an empiric unit of nuclear mass that has natural origin. The translation coefficient between universal mass unit u and empiric nuclear mass unit a1 is equal to: u/ a1 1.004434(9). (7) 1. A.M. Nurmukhamedov, Physics of Atomic Nuclei, 72 (3), 401 (2009). 2. A.M. Nurmukhamedov, Physics of Atomic Nuclei, 72, 1435 (2009). 3. Yu.V. Gaponov, N.B. Shulgina, and D.M. Vladimirov, Nucl. Phys. A 391, 93 (1982). 4. G. Audi, A.H. Wapstra and C. Thibault, Nucl.Phys A 729, 129 (2003). PAIR ENERGY OF PROTON AND NEUTRON IN ATOMIC NUCLEI Nurmukhamedov A.M. Institute of Nuclear Physics, Tashkent, Uzbekistan The work [1] demonstrated that the structure of Wigner’s mass formula contains pairing of nucleons. Taking into account that the pair energy is playing significant role in nuclear events and in a view of new data we would like to review this issue again. -
Intel Management Engine Deep Dive
Intel Management Engine Deep Dive Peter Bosch About me Peter Bosch ● CS / Astronomy student at Leiden University ● Email : [email protected] ● Twitter: @peterbjornx ● GitHub: peterbjornx ● https://pbx.sh/ About me Previous work: ● CVE-2019-11098: Intel Boot Guard bypass through TOCTOU attack on the SPI bus (Co-discovered by @qrs) Outline 1. Introduction to the Management Engine Operating System 2. The Management Engine as part of the boot process 3. Possibilities for opening up development and security research on the ME Additional materials will be uploaded to https://pbx.sh/ in the days following the talk. About the ME About ME ● Full-featured embedded system within the PCH ○ 80486-derived core ○ 1.5MB SRAM ○ 128K mask ROM ○ Hardware cryptographic engine ○ Multiple sets of fuses. ○ Bus bridges to PCH global fabric ○ Access to host DRAM ○ Access to Ethernet, WLAN ● Responsible for ○ System bringup ○ Manageability ■ KVM ○ Security / DRM ■ Boot Guard ■ fTPM ■ Secure enclave About ME ● Only runs Intel signed firmware ● Sophisticated , custom OS ○ Stored mostly in SPI flash ○ Microkernel ○ Higher level code largely from MINIX ○ Custom filesystems ○ Custom binary format ● Configurable ○ Factory programmed fuses ○ Field programmable fuses ○ SPI Flash ● Extensible ○ Native modules ○ JVM (DAL) Scope of this talk Intel ME version 11 , specifically looking at version 11.0.0.1205 Platforms: ● Sunrise Point (Core 6th, 7th generation SoC, Intel 100, 200 series chipset) ● Lewisburg ( Intel C62x chipsets ) Disclaimer ● I am in no way affiliated with Intel Corporation. ● All information presented here was obtained from public documentation or by reverse engineering firmware extracted from hardware found “in the wild”. ● Because this presentation covers a very broad and scarcely documented subject I can not guarantee accuracy of the contents. -
The Strangeness Magnetic Moment of the Proton in the Chiral Quark Model
The Strangeness Magnetic Moment of the Proton in the Chiral Quark Model L. Hannelius, D.O. Riska Department of Physics, University of Helsinki, 00014 Finland and L. Ya. Glozman Institute for Theoretical Physics, University of Graz, A-8019 Graz, Austria Abstract The strangeness magnetic moment of the proton is shown to be small in the chiral quark model. The dominant loop contribution is due to kaons. The K∗ loop contributions are proportional to the difference between the strange and light constituent quark masses or −2 mK∗ and therefore small. The loop fluctuations that involve radiative transitions between K∗ mesons and kaons are small, when the cut-off scale in the loops is taken to be close to the chiral symmetry restoration scale. The net loop amplitude contribution to the strangeness magnetic moment of the proton is about −0.05, which falls within the uncertainty range of arXiv:hep-ph/9908393v2 24 Aug 1999 the experimental value. 0 1. Introduction The recent finding by the SAMPLE collaboration that the strangeness magnetic moment s 2 2 of the proton is small, and possibly even positive [1] (GM (Q = 0.1 GeV )=0.23 ± 0.37) was unexpected in view of the fact that the bulk of the many theoretical predictions for this quantity are negative, and outside of the experimental uncertainty range (summaries are given e.g. in refs. [2, 3, 4]). A recent lattice calculation gives −0.36 ± 0.20 for this quantity [5], thus reaffirming the typical theoretical expectation, while remaining outside of the uncertainty range of the empirical value. -
An Introduction to Morphos
An Introduction to MorphOS Updated to include features to version 1.4.5 May 14, 2005 MorphOS 1.4 This presentation gives an overview of MorphOS and the features that are present in the MorphOS 1.4 shipping product. For a fully comprehensive list please see the "Full Features list" which can be found at: www.PegasosPPC.com Why MorphOS? Modern Operating Systems are powerful, flexible and stable tools. For the most part, if you know how to look after them, they do their job reasonably well. But, they are just tools to do a job. They've lost their spark, they're boring. A long time ago computers were fun, it is this background that MorphOS came from and this is what MorphOS is for, making computers fun again. What is MorphOS? MorphOS is a fully featured desktop Operating System for PowerPC CPUs. It is small, highly responsive and has very low hardware requirements. The overall structure of MorphOS is based on a new modern kernel called Quark and a structure divided into a series of "boxes". This system allows different OS APIs to be used along side one another but isolates them so one cannot compromise the other. To make sure there is plenty of software to begin with the majority of development to date has been based on the A- BOX. In the future the more advanced Q-Box shall be added. Compatibility The A-Box is an entire PowerPC native OS layer which includes source and binary compatibility with software for the Commodore A500 / A1200 etc. -
Basics of Qcd Perturbation Theory
BASICS OF QCD PERTURBATION THEORY Davison E. Soper* Institute of Theoretical Science University of Oregon, Eugene, OR 97403 ABSTRACT (•• i This is an introduction to the use of QCD perturbation theory, em- I phasizing generic features of the theory that enable one to separate short-time and long-time effects. I also cover some important classes of applications: electron-positron annihilation to hadrons, deeply in- elastic scattering, and hard processes in hadron-hadron collisions. •Supported by DOE Contract DE-FG03-96ER40969. © 1996 by Davison E. Soper. -15- 1 Introduction 2 Electron-Positron Annihilation and Jets A prediction for experiment based on perturbative QCD combines a particular In this section, I explore the structure of the final state in QCD. I begin with the calculation of Feynman diagrams with the use of general features of the theory. kinematics of e+e~ —> 3 partons, then examine the behavior of the cross section The particular calculation is easy at leading order, not so easy at next-to-leading for e+e~ —i- 3 partons when two of the parton momenta become collinear or one order, and extremely difficult beyond the next-to-leading order. This calculation parton momentum becomes soft. In order to illustrate better what is going on, of Feynman diagrams would be a purely academic exercise if we did not use certain I introduce a theoretical tool, null-plane coordinates. Using this tool, I sketch general features of the theory that allow the Feynman diagrams to be related to a space-time picture of the singularities that we find in momentum space. -
Prospects for Measurements with Strange Hadrons at Lhcb
Prospects for measurements with strange hadrons at LHCb A. A. Alves Junior1, M. O. Bettler2, A. Brea Rodr´ıguez1, A. Casais Vidal1, V. Chobanova1, X. Cid Vidal1, A. Contu3, G. D'Ambrosio4, J. Dalseno1, F. Dettori5, V.V. Gligorov6, G. Graziani7, D. Guadagnoli8, T. Kitahara9;10, C. Lazzeroni11, M. Lucio Mart´ınez1, M. Moulson12, C. Mar´ınBenito13, J. Mart´ınCamalich14;15, D. Mart´ınezSantos1, J. Prisciandaro 1, A. Puig Navarro16, M. Ramos Pernas1, V. Renaudin13, A. Sergi11, K. A. Zarebski11 1Instituto Galego de F´ısica de Altas Enerx´ıas(IGFAE), Santiago de Compostela, Spain 2Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom 3INFN Sezione di Cagliari, Cagliari, Italy 4INFN Sezione di Napoli, Napoli, Italy 5Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom, now at Universit`adegli Studi di Cagliari, Cagliari, Italy 6LPNHE, Sorbonne Universit´e,Universit´eParis Diderot, CNRS/IN2P3, Paris, France 7INFN Sezione di Firenze, Firenze, Italy 8Laboratoire d'Annecy-le-Vieux de Physique Th´eorique , Annecy Cedex, France 9Institute for Theoretical Particle Physics (TTP), Karlsruhe Institute of Technology, Kalsruhe, Germany 10Institute for Nuclear Physics (IKP), Karlsruhe Institute of Technology, Kalsruhe, Germany 11School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom 12INFN Laboratori Nazionali di Frascati, Frascati, Italy 13Laboratoire de l'Accelerateur Lineaire (LAL), Orsay, France 14Instituto de Astrof´ısica de Canarias and Universidad de La Laguna, Departamento de Astrof´ısica, La Laguna, Tenerife, Spain 15CERN, CH-1211, Geneva 23, Switzerland 16Physik-Institut, Universit¨atZ¨urich,Z¨urich,Switzerland arXiv:1808.03477v2 [hep-ex] 31 Jul 2019 Abstract This report details the capabilities of LHCb and its upgrades towards the study of kaons and hyperons. -
Introduction to Storage and Software Systems for Data Analysis
INTRODUCTION TO STORAGE AND SOFTWARE SYSTEMS FOR DATA ANALYSIS Bob Jacobsen University of California, Berkeley, USA Abstract The Storage and Software Systems for Data Analysis track discusses how HEP physics data is taken, processed and analyzed, with emphasis on the problems that data size and CPU needs pose for people trying to do experimental physics. The role of software engineering is discussed in the context of building large, robust systems that must at the same time be accessible to physicists. We include some examples of existing systems for physics analysis, and raise some issues to consider when evaluating them. This lecture is the introduction to those topics. 1. INTRODUCTION Many modern high-energy physics (HEP) experiments are done by collaborations of hundreds of people. Together, these groups construct and operate complex detectors, recording billions of events and terabytes of data, all toward the goal of “doing physics”. In this note, we provide an introduction to how we currently do this, and raise a number of issues to be considered when thinking about the new systems that are now being built. 2. SCALE OF THE EXPERIMENTS BaBar, CDF and D0 are examples of the large experiments now taking or about to take data in a collider environment. The collaborations that have built these experiments contain 300 to 600 members with varying levels of activity. Almost everybody is considered “familiar” with using computing to do their work, but only a small fraction of the collaboration can be considered as computing professionals. Some of these can even be considered world-class experts in large scale computing. -
Quarkxpress 8.0 Readme Ii
QuarkXPress 8.0 ReadMe ii Contents QuarkXPress 8.0 ReadMe....................................................................................................3 System requirements.............................................................................................................4 Mac OS.....................................................................................................................................................4 Windows...................................................................................................................................................4 Installing: Mac OS................................................................................................................5 Performing a silent installation.................................................................................................................5 Preparing for silent installation....................................................................................................5 Installing.......................................................................................................................................5 Performing a drag installation..................................................................................................................5 Adding files after installation...................................................................................................................6 Installing: Windows..............................................................................................................7 -
Dark Matter in Nuclear Physics
Dark Matter in Nuclear Physics George Fuller (UCSD), Andrew Hime (LANL), Reyco Henning (UNC), Darin Kinion (LLNL), Spencer Klein (LBNL), Stefano Profumo (Caltech) Michael Ramsey-Musolf (Caltech/UW Madison), Robert Stokstad (LBNL) Introduction A transcendent accomplishment of nuclear physics and observational cosmology has been the definitive measurement of the baryon content of the universe. Big Bang Nucleosynthesis calculations, combined with measurements made with the largest new telescopes of the primordial deuterium abundance, have inferred the baryon density of the universe. This result has been confirmed by observations of the anisotropies in the Cosmic Microwave Background. The surprising upshot is that baryons account for only a small fraction of the observed mass and energy in the universe. It is now firmly established that most of the mass-energy in the Universe is comprised of non-luminous and unknown forms. One component of this is the so- called “dark energy”, believed to be responsible for the observed acceleration of the expansion rate of the universe. Another component appears to be composed of non-luminous material with non-relativistic kinematics at the current epoch. The relationship between the dark matter and the dark energy is unknown. Several national studies and task-force reports have found that the identification of the mysterious “dark matter” is one of the most important pursuits in modern science. It is now clear that an explanation for this phenomenon will require some sort of new physics, likely involving a new particle or particles, and in any case involving physics beyond the Standard Model. A large number of dark matter studies, from theory to direct dark matter particle detection, involve nuclear physics and nuclear physicists.