Superkekb Background Simulations, Including Issues for Detector
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BABAR Studies Matter-Antimatter Asymmetry in Τ Lepton Decays
BABAR studies matter-antimatter asymmetry in τττ lepton decays Humans have wondered about the origin of matter since the dawn of history. Physicists address this age-old question by using particle accelerators to recreate the conditions that existed shortly after the Big Bang. At an accelerator, energy is converted into matter according to Einstein’s famous energy-mass relation, E = mc 2 , which offers an explanation for the origin of matter. However, matter is always created in conjunction with the same amount of antimatter. Therefore, the existence of matter – and no antimatter – in the universe indicates that there must be some difference, or asymmetry, between the properties of matter and antimatter. Since 1999, physicists from the BABAR experiment at SLAC National Accelerator Laboratory have been studying such asymmetries. Their results have solidified our understanding of the underlying micro-world theory known as the Standard Model. Despite its great success in correctly predicting the results of laboratory experiments, the Standard Model is not the ultimate theory. One indication for this is that the matter-antimatter asymmetry allowed by the Standard Model is about a billion times too small to account for the amount of matter seen in the universe. Therefore, a primary quest in particle physics is to search for hard evidence for “new physics”, evidence that will point the way to the more complete theory beyond the Standard Model. As part of this quest, BABAR physicists also search for cracks in the Standard Model. In particular, they study matter-antimatter asymmetries in processes where the Standard Model predicts that asymmetries should be very small or nonexistent. -
The Belle-II Experiment at Superkekb
Gary S. Varner, Hawai’i The Belle-II Experiment at SuperKEKB Gary S. Varner University of Hawai’i at Manoa Boston (Cambridge), July 26, 2011 Luminosity at the B Factories Gary S. Varner, Hawai’i Fantastic performance much beyond design values! Need O(100x) more data Next generation B-factories Gary S. Varner, Hawai’i SuperKEKB + SuperB 40 times higher luminosity KEKB PEP-II Asymmetric B factories Gary S. Varner, Hawai’i √s=10.58 GeV + - B e e z ~ c Υ(4s) B Υ(4s) B ~ 200m BaBar p(e-)=9 GeV p(e+)=3.1 GeV =0.56 Belle p(e-)=8 GeV p(e+)=3.5 GeV =0.42 Belle II p(e-)=7 GeV p(e+)=4 GeV =0.28 Full Reconstruction Method Gary S. Varner, Hawai’i • Fully reconstruct one of the B’s to – Tag B flavor/charge – Determine B momentum – Exclude decay products of one B from further analysis Decays of interest B BXu l , BK e e+(3.5GeV) (8GeV) BD, Υ(4S) B full reconstruction BD etc. (~0.5%) Offline B meson beam! Powerful tool for B decays with neutrinos “Super” B Factory motivation Gary S. Varner, Hawai’i For details on physics opportunities: See Kay Kinoshita talk 17:20 B factories is SM with CKM right? Thursday, July 28 – Section 5I Super B factories How is the SM wrong? Need much more data (two orders!) because the SM worked so well until now Super B factory e+e- machines running at (or near) Y(4s) will have considerable advantages in several classes of measurements, and will be complementary in many more to LHCb and BESIII Recent update of the physics reach with 50 ab-1 (75 ab-1): Physics at Super B Factory (Belle II authors + guests) hep-ex > arXiv:1002 .5012 SuperB Progress Reports: Physics (SuperB authors + guests) hep-ex > arXiv:1008.1541 TSUKUBA Area (Belle) High Energy Ring (HER) for Electron HER LER How to do it? Interaction Region Low Energy Ring (LER) for Positron Gary S. -
Superkekb VACUUM SYSTEM K
SuperKEKB VACUUM SYSTEM K. Shibata#, KEK, Tsukuba, Japan Abstract size in the horizontal and vertical directions at the IP, I is SuperKEKB, which is an upgrade of the KEKB B- the beam current, y is the vertical beam-beam * factory (KEKB), is a next-generation high-luminosity parameter, y is the vertical beta function at the IP, RL electron-positron collider. Its design luminosity is 8.0× and Ry are the reduction factors for the luminosity and 1035 cm-2s-1, which is about 40 times than the KEKB’s vertical beam-beam tune-shift parameter, respectively, record. To achieve this challenging goal, bunches of both owing to the crossing angle and the hourglass effect. The beams are squeezed extremely to the nanometer scale and subscripts + and – indicate a positron or electron, the beam currents are doubled. To realize this, many respectively. At the SuperKEKB, crossing the beams by upgrades must be performed including the replacement of using the “nanobeam scheme” [3] makes it possible to * th beam pipes mainly in the positron ring (LER). The beam squeeze y to about 1/20 of KEKB’s size. In the pipes in the LER arc section are being replaced with new nanobeam scheme, bunches of both beams are squeezed aluminium-alloy pipes with antechambers to cope with extremely to the nanometer scale (0.3 mm across and 100 the electron cloud issue and heating problem. nm high) and intersect only in the highly focused region Additionally, several types of countermeasures will be of each bunch at a large crossing angle (4.8 degrees). -
Commissioning of the KEKB B-Factoryinvited
Proceedings of the 1999 Particle Accelerator Conference, New York, 1999 COMMISSIONING OF THE KEKB B–FACTORY K. Akai, N. Akasaka, A. Enomoto, J. Flanagan, H. Fukuma, Y. Funakoshi, K. Furukawa, J. Haba, S. Hiramatsu, K. Hosoyama, N. Huang∗, T. Ieiri, N. Iida, T. Kamitani, S. Kato, M. Kikuchi, E. Kikutani, H. Koiso, S.–I. Kurokawa, M. Masuzawa, S. Michizono, T. Mimashi, T. Nakamura, Y. Ogawa, K. Ohmi, Y. Ohnishi, S. Ohsawa, N. Ohuchi, K. Oide,D.Pestrikov†,K.Satoh, M. Suetake, Y. Suetsugu, T. Suwada, M. Tawada, M. Tejima, M. Tobiyama, N. Yamamoto, M. Yoshida, S. Yoshimoto, M. Yoshioka, KEK, Oho, Tsukuba, Ibaraki 305-0801, Japan, T. Browder, Univ. of Hawaii, 2505 Correa Road, Honolulu, HI 96822, U.S.A. Abstract The commissioning of the KEKB B–Factory storage rings started on Dec. 1, 1998. The two rings both achieved a stored current of over 0.5 A after operating for four months. The two beams were successfully collided several times. The commissioning stopped on Apr. 19, taking a 5-week break to install the Belle detector. 1 BRIEF HISTORY OF THE COMMISSIONING The KEKB B–Factory[1] consists of two storage rings, the LER (3.5 GeV, e+) and the HER (8 GeV, e−), and the in- jector Linac/beam-transport (BT) system. The Linac was upgraded from the injector for TRISTAN, and was com- missioned starting in June 1997, including part of the BT line. The injector complex was ready before the start of commissioning of the rings.[2] Figure 1 shows the growth of the stored currents in the two rings through the period of commissioning. -
Superb Report Intensity Frontier Workshop 1 Introduction
SuperB Report Intensity Frontier Workshop 1 Introduction The Standard Model (SM) has been very successful in explaining a wide range of electroweak and strong processes with high precision. In the flavor sector, observation of CP violation in B decays at BABAR and Belle, and the extraordinary consistency between the CKM matrix elements, established the SM as the primary source of CP violation in nature (leading to the 2008 Nobel Prize in physics). However, the remarkable success of the SM in describing all known flavor-physics measurements presents a puzzle to the search for New Physics (NP) at the LHC. New particles below the TeV scale should contribute to low-energy processes through virtual loop diagrams and cause observable effects in the flavor sector. The lack of any such effects suggests that either the NP mass scale is much higher than the TeV scale, or that NP flavor-violating operators are suppressed. In either scenario, flavor physics at the intensity frontier is poised to remain a central element of particle physics research in the coming decades. The INFN-sponsored SuperB project [1–3] in Italy is an asymmetric-energy electron- positron collider in the 10 GeV energy region with an initial design average luminosity of 1036 cm−2s−1, which will deliver up to 75 ab−1 in five years of operation (see Fig. 1 for details) to a new SuperB detector derived from the existing BABAR. A new innovative concept in accelerator design, employing very low-emittance beams and a “crab waist” final focus, makes possible this large increase (100-fold) in instantaneous luminosity over present B Factory colliders with no corresponding increase in power consumption, and similar backgrounds for the detector. -
Present Status of Kekb Project
PRESENT STATUS OF KEKB PROJECT Shin-ichi Kurokawa KEK, High Energy Accelerator Research Organization 1-1 Oho, Tsukuba-shi, Ibaraki-ken, 305-0801, Japan Abstract GeV electron and a 5.3-GeV positron collide and produce a pair of B meson and anti-B meson at rest at the Υ(4S) The KEK B-Factory, KEKB, is an asymmetric-energy, resonance. In the laboratory frame where an 8-GeV two-ring, electron-positron collider for B physics. Eight- electron and a 3.5-GeV positron collide, the B and anti-B GeV electrons stored in a high-energy ring (HER) and mesons move along the direction of the incoming 3.5- GeV positrons in a low-energy ring (LER) collide at electron, travel over a few hundred µm, and decay at an interaction point (IP), which BELLE detector different positions. By detecting the decay products, we surrounds. In order to facilitate detection of CP-violation can identify the B and anti-B mesons. This identification effect at the bottom-quark sector, the machine is designed is essential for studying CP-violation, which is a subtle to reach a luminosity of 1034cm-2s-1. Even with a high difference in behavior between particles and anti- beam-beam tuneshift of 0.052 and a small βy* of 1 cm at particles. IP, necessary currents in the rings amount to 1.1 A at HER and 2.6 A at LER. KEKB adopts new schemes to reach TSUKUBA IP the goal, such as ±11 mrad finite-angle collision at IP, non-interleaved-sextupole chromaticity correction to have HER LER HER large dynamic apertures, higher-order-mode-free normal LER conducting cavity called ARES and single-cell, single- mode, superconducting cavities to prevent coupled-bunch instabilities and combat heavy beam-loading, among others. -
First New Particle-‐Smasher Since the LHC Comes
www.coepp.org.au Media release for immediate release Thursday 3 March 2016 First new particle-smasher since the LHC comes online A new particle collider, SuperKEKB, located at the KEK laboratory in Tsukuba, Japan has achieved “First Turns” and is now in the test operation stage. This is the newest “particle-smasher” to go online since the LHC at CERN in Geneva. SuperKEKB will be the world’s highest-luminosity collider and, in association with the Belle II experiment, it will collide electrons with their antiparticles – positrons – in the search for new physics. Designed and built at KEK by a team of Japanese accelerator physicists, SuperKEKB, along with the Belle II detector at the interaction point, will search for new physics beyond the Standard Model by measuring rare decays of elementary particles such as beauty quarks, charm quarks and tau leptons. In contrast to the LHC, which is the world's highest energy machine, SuperKEKB/Belle II is designed to have the world’s highest luminosity or rate of collisions (40 times higher than its predecessor KEKB). This will make SuperKEKB the world’s “highest luminosity” machine and the leading accelerator on the “luminosity frontier”. Key milestones: • 10 February, 2016: SuperKEKB succeeded in circulating and storing a positron beam moving close to the speed of light around the 3.0 kilometre circumference of its main ring. • 26 February, 2016: SuperKEKB electron-positron collider succeeded in circulating and storing a seven billion electron-volt energy (7 GeV) electron beam around its ring of magnets in the opposite direction. The achievement of these “first turns” – i.e. -
Status of Super-Kekb and Belle Ii∗
Vol. 41 (2010) ACTA PHYSICA POLONICA B No 12 STATUS OF SUPER-KEKB AND BELLE II∗ Henryk Pałka The H. Niewodniczański Institute of Nuclear Physics Polish Academy of Sciences Radzikowskiego 152, 31-342 Kraków, Poland (Received November 29, 2010) The status of preparations to Belle II experiment at the SuperKEKB collider is reviewed in this article. PACS numbers: 11.30.Er, 12.15.Hh, 13.20.He, 29.20.db 1. Introduction The Belle detector [1] has stopped data taking in June 2010. A decade- long operation of the experiment at the asymmetric beam energy electron- positron collider KEKB [2] resulted in a data sample of an integrated lumi- nosity exceeding 1 ab−1. This would not be possible without the excellent performance of the KEKB. The collider has reached the world record in- stantaneous luminosity of 2:2 × 1034 cm−2s−1 (Fig. 1), more than twice the design luminosity. Several technological innovations contributed to this achievement, among them crab cavities developed at KEK and successful implementation of continuous injection. Fig. 1. Time-line of KEKB peak luminosity. ∗ Lecture presented at the L Cracow School of Theoretical Physics “Particle Physics at the Dawn of the LHC”, Zakopane, Poland, June 9–19, 2010. (2595) 2596 H. Pałka By the precise measurement of the CKM angle φ1 by Belle and BaBar, its companion B-meson factory experiment at SLAC [3], the Kobayashi– Maskawa mechanism of CP violation [4] has been confirmed. Following the experimental confirmation M. Kobayashi and T. Maskawa were awarded the 2008 Nobel Prize in Physics. Numerous other physics results of B-meson factory experiments further support the hypothesis that the matrix of three- generation quark mixing is the dominant source of CP violation in B- and K-meson decays. -
Overview of the KEKB Accelerators
Nuclear Instruments and Methods in Physics Research A 499 (2003) 1–7 Overview of the KEKB accelerators S. Kurokawa, E. Kikutani* KEK, National High Energy Accelerator Organization, Oho 1-1, Tsukuba-shi, Ibaraki 305-0801, Japan Abstract An overview of the KEKB accelerators is given as an introduction of the following articles in this issue, first by summarizing the basic features of the machines, and then describing the improvements of the performance since the start of the physics experiment. r 2002 Elsevier Science B.V. All rights reserved. PACS: 29.20. Keywords: Colliding machine; Storage ring 1. Introduction osity by Belle from the start of the physics experiment in June 1999 up to November 2001. We have witnessed a steady improvement in the This steady improvement in the performance of performance of KEKB from the start of the KEKB and the achievement of unprecedented physics experiment in June 1999 to the present luminosity of 5:47 Â 1033 cmÀ2 sÀ1 are the culmi- time. To review this improvement, we list here nation of almost a 10-year effort by KEKB staff milestone dates of the peak luminosity: the peak members. There still remain many things to be luminosity of KEKB exceeded 1:0 Â 1033 cmÀ2 sÀ1 improved in KEKB, to first reach the design in April 2000, reached 2:0 Â 1033 cmÀ2 sÀ1 in July luminosity of 1 Â 1034 cmÀ2 sÀ1; and then to 2000, surpassed 3:0 Â 1033 and 4:0 Â 1033 cmÀ2 sÀ1 eventually exceed it. The papers compiled here in March and June 2001, and finally reached 5:47 Â summarize our efforts made for KEKB and were 1033 cmÀ2 sÀ1 in November 2001. -
KEKB Accelerator Control System
Nuclear Instruments and Methods in Physics Research A 499 (2003) 138–166 KEKB accelerator control system Nobumasa Akasaka, Atsuyoshi Akiyama, Sakae Araki, Kazuro Furukawa, Tadahiko Katoh*, Takashi Kawamoto, Ichitaka Komada, Kikuo Kudo, Takashi Naito, Tatsuro Nakamura, Jun-ichi Odagiri, Yukiyoshi Ohnishi, Masayuki Sato, Masaaki Suetake, Shigeru Takeda, Yasunori Takeuchi, Noboru Yamamoto, Masakazu Yoshioka, Eji Kikutani KEK, High Energy Accelerator Research Organization, Oho 1-1, Tsukuba Ibaraki 305-0801, Japan Abstract The KEKB accelerator control system including a control computer system, a timing distribution system, and a safety control system are described. KEKB accelerators were installed in the same tunnel where the TRISTAN accelerator was. There were some constraints due to the reused equipment. The control system is based on Experimental Physics and Industrial Control System (EPICS). In order to reduce the cost and labor for constructing the KEKB control system, as many CAMAC modules as possible are used again. The guiding principles of the KEKB control computer system are as follows: use EPICS as the controls environment, provide a two-language system for developing application programs, use VMEbus as frontend computers as a consequence of EPICS, use standard buses, such as CAMAC, GPIB, VXIbus, ARCNET, RS-232 as field buses and use ergonomic equipment for operators and scientists. On the software side, interpretive Python and SAD languages are used for coding application programs. The purpose of the radiation safety system is to protect personnel from radiation hazards. It consists of an access control system and a beam interlock system. The access control system protects people from strong radiation inside the accelerator tunnel due to an intense beam, by controlling access to the beamline area. -
Discovery at the Large Hadron Collider
Discovery at the Large Hadron Collider Michel Lefebvre University of Victoria ATLAS Canada Collaboration CAP Congress 27 May 2013 Abstract Discovery at the Large Hadron Collider The recent discovery of a new particle is a historic event in our exploration of the fundamental constituents of matter and the interactions between them. To date, the Standard Model of particle physics is extremely successful and accounts for all measured subatomic phenomena. However the postulated Higgs mechanism, from which fundamental particles acquire mass, remains to be verified experimentally. Research at the energy frontier is being carried out at the Large Hadron Collider (LHC), operating at CERN near Geneva since 2010. From 2010 to 2012, the LHC provided proton-proton collisions at a centre of mass energy of 7 to 8 TeV, allowing the exploration of distance scales smaller than a tenth of an attometer. The products of these collisions were successfully recorded by the ATLAS detector, which will be introduced in this lecture, with emphasis on Canadian contributions. The ATLAS physics programme features Standard Model measurements and a rich array of searches for new physics phenomena. The discovery of a new Higgs-like particle and other important results will be presented. The future increase in energy and intensity at the LHC, and the associated ATLAS plans, will also be discussed. These are exciting times indeed for particle physics! Michel Lefebvre, UVic and ATLAS Canada CAP Congress, 27 May 2013 2 Scattering experiment We see through the scatter of -
Introduction to Flavour Physics
Introduction to flavour physics Y. Grossman Cornell University, Ithaca, NY 14853, USA Abstract In this set of lectures we cover the very basics of flavour physics. The lec- tures are aimed to be an entry point to the subject of flavour physics. A lot of problems are provided in the hope of making the manuscript a self-study guide. 1 Welcome statement My plan for these lectures is to introduce you to the very basics of flavour physics. After the lectures I hope you will have enough knowledge and, more importantly, enough curiosity, and you will go on and learn more about the subject. These are lecture notes and are not meant to be a review. In the lectures, I try to talk about the basic ideas, hoping to give a clear picture of the physics. Thus many details are omitted, implicit assumptions are made, and no references are given. Yet details are important: after you go over the current lecture notes once or twice, I hope you will feel the need for more. Then it will be the time to turn to the many reviews [1–10] and books [11, 12] on the subject. I try to include many homework problems for the reader to solve, much more than what I gave in the actual lectures. If you would like to learn the material, I think that the problems provided are the way to start. They force you to fully understand the issues and apply your knowledge to new situations. The problems are given at the end of each section.