Particle Fever Teacher Guide.Pdf
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The Higgs Boson!
MEET THE TIME MAGAZINE PARTICLE OF THE YEAR: THE HIGGS BOSON! Saptaparna Bhattacharya July 11th - 22nd, 2016 Lets start at the beginning! http://poy.time.com/2012/12/19/the-higgs-boson-particle-of-the-year/ Introduction • I am Saptaparna Bhattacharya, a post-doctoral scholar in the department of Physics and Astronomy at Northwestern University in Chicago. • My research is based on the data from the Large Hadron Collider at CERN. • I have worked on the first published result that uses the Higgs boson as a probe for New Physics. • My interest lies in various models of New Physics, ranging from SuperSymmetry to exploring the possibility of finding microscopic black holes. • I am also interested in exploring interesting techniques for data analysis. But, enough about me, where are you guys from? Current Enrollment We are a class of 17 students! Let me quickly check to see if you are all here! What we did last summer! Di-photon invariant mass h_InvariantMass_PhPh Higgs to ZZ invariant mass h_InvariantMass_HZZ Entries 85893 Entries 13235 30000 Mean 125.9 Mean 124.2 RMS 2.636 RMS 3.147 5000 25000 Events/2.0 GeV Events/2.0 GeV 20000 4000 Higgs boson mass distribution Higgs boson mass distribution 15000 3000 10000 2000 5000 1000 0 0 100 105 110 115 120 125 130 135 140 145 150 100 105 110 115 120 125 130 135 140 145 150 m [GeV] m [GeV] γγ µ µ µ µ Di-muon invariant mass h_InvariantMass_MuMu Tranverse Mass with Muons Entries 37122 h_TransverseMass_Mu Mean 90.66 Entries 37791 RMS 4.506 5000 4000 Mean 65.9 RMS 15.36 3500 4000 Events/GeV Events/1.0 GeV 3000 Z boson mass distribution 3000 2500 W boson transverse 2000 mass distribution 2000 1500 1000 1000 500 0 0 70 75 80 85 90 95 100 105 110 0 50 100 150 200 250 300 m [GeV] mµµ [GeV] T Outline • The course is roughly structured into two parts: • Laying down the fundamentals. -
Conceptual Investigations of a Trigger Extension for Muons from Pp Collisions in the CMS Experiment
Conceptual investigations of a trigger extension for muons from pp collisions in the CMS experiment Von der Fakult¨at fur¨ Mathematik, Informatik und Naturwissenschaften der RWTH Aachen University zur Erlangung des akademischen Grades eines Doktors der Naturwissenschaften genehmigte Dissertation vorgelegt von Diplom-Physiker Yusuf Erdogan aus Istanbul Berichter: Universit¨atsprofessor Dr. rer. nat. Achim Stahl Universit¨atsprofessor Dr. rer. nat. Thomas Hebbeker Tag der mundlic¨ hen Prufung¨ : 24. Februar 2015 Diese Dissertation ist auf den Internetseiten der Hochschulbibliothek online verfu¨gbar. Kurzfassung Der Large Hadron Collider wird ab 2023 an seine Experimente fun¨ f bis zehn mal mehr Lu- minosit¨at als der derzeitige Designwert von 1034 cm−2s−1 liefern k¨onnen. Diese Verbes- serung wird die Messung von physikalischen Prozessen mit sehr kleinen Wirkungsquer- schnitten erlauben. Jedoch wird bei diesen hohen Luminosit¨aten, aufgrund von Pile-up Wechselwirkungen, die Belegung des CMS-Detektors sehr hoch sein. Dies wird einer- seits einen systematischen Anstieg von Triggerraten fur¨ einzelne Myonen verursachen, Andererseits werden die Fehlmessungen von Myon-Transversalimpulsen, verst¨arkt durch die begrenzte Impulsaufl¨osung des Myon-Systems, fur¨ hohe Impulswerte dominant sein. In diesem Bereich flacht die Verteilung der Triggerrate ab, was die Beschr¨ankung der Triggerrate durch eine Schwelle der Transversalimpulse erschwert. Außerdem wird die Qualit¨at des Triggers fu¨r einzelne Myonen durch koinzidente Teilchendurchg¨ange ver- ringert, da diese zu Doppeldeutigkeiten in den innersten Myonkammern fuh¨ ren k¨onnen. Im Rahmen der Ver¨offentlichung [2] wurde im Jahr 2007 ein Muon Track fast Tag (MTT) genanntes Konzept vorgestellt, um diese Trigger-Herausforderungen zu adressieren. Die, in dieser Arbeit durchgefuh¨ rten Studien sind in drei Abschitte unterteilt. -
Inside the Perimeter Is Published by Perimeter Institute for Theoretical Physics
the Perimeter fall/winter 2014 Skateboarding Physicist Seeks a Unified Theory of Self The Black Hole that Birthed the Big Bang The Beauty of Truth: A Chat with Savas Dimopoulos Subir Sachdev's Superconductivity Puzzles Editor Natasha Waxman [email protected] Contributing Authors Graphic Design Niayesh Afshordi Gabriela Secara Erin Bow Mike Brown Photographers & Artists Phil Froklage Tibra Ali Colin Hunter Justin Bishop Robert B. Mann Amanda Ferneyhough Razieh Pourhasan Liz Goheen Natasha Waxman Alioscia Hamma Jim McDonnell Copy Editors Gabriela Secara Tenille Bonoguore Tegan Sitler Erin Bow Mike Brown Colin Hunter Inside the Perimeter is published by Perimeter Institute for Theoretical Physics. www.perimeterinstitute.ca To subscribe, email us at [email protected]. 31 Caroline Street North, Waterloo, Ontario, Canada p: 519.569.7600 f: 519.569.7611 02 IN THIS ISSUE 04/ Young at Heart, Neil Turok 06/ Skateboarding Physicist Seeks a Unified Theory of Self,Colin Hunter 10/ Inspired by the Beauty of Math: A Chat with Kevin Costello, Colin Hunter 12/ The Black Hole that Birthed the Big Bang, Niayesh Afshordi, Robert B. Mann, and Razieh Pourhasan 14/ Is the Universe a Bubble?, Colin Hunter 15/ Probing Nature’s Building Blocks, Phil Froklage 16/ The Beauty of Truth: A Chat with Savas Dimopoulos, Colin Hunter 18/ Conference Reports 22/ Back to the Classroom, Erin Bow 24/ Finding the Door, Erin Bow 26/ "Bright Minds in Their Life’s Prime", Colin Hunter 28/ Anthology: The Portraits of Alioscia Hamma, Natasha Waxman 34/ Superconductivity Puzzles, Colin Hunter 36/ Particles 39/ Donor Profile: Amy Doofenbaker, Colin Hunter 40/ From the Black Hole Bistro, Erin Bow 42/ PI Kids are Asking, Erin Bow 03 neil’s notes Young at Heart n the cover of this issue, on the initial singularity from which everything the lip of a halfpipe, teeters emerged. -
Curriculum Vitae
CURRICULUM VITAE Raman Sundrum July 26, 2019 CONTACT INFORMATION Physical Sciences Complex, University of Maryland, College Park, MD 20742 Office - (301) 405-6012 Email: [email protected] CAREER John S. Toll Chair, Director of the Maryland Center for Fundamental Physics, 2012 - present. Distinguished University Professor, University of Maryland, 2011-present. Elkins Chair, Professor of Physics, University of Maryland, 2010-2012. Alumni Centennial Chair, Johns Hopkins University, 2006- 2010. Full Professor at the Department of Physics and Astronomy, The Johns Hopkins University, 2001- 2010. Associate Professor at the Department of Physics and Astronomy, The Johns Hop- kins University, 2000- 2001. Research Associate at the Department of Physics, Stanford University, 1999- 2000. Advisor { Prof. Savas Dimopoulos. 1 Postdoctoral Fellow at the Department of Physics, Boston University. 1996- 1999. Postdoc advisor { Prof. Sekhar Chivukula. Postdoctoral Fellow in Theoretical Physics at Harvard University, 1993-1996. Post- doc advisor { Prof. Howard Georgi. Postdoctoral Fellow in Theoretical Physics at the University of California at Berke- ley, 1990-1993. Postdoc advisor { Prof. Stanley Mandelstam. EDUCATION Yale University, New-Haven, Connecticut Ph.D. in Elementary Particle Theory, May 1990 Thesis Title: `Theoretical and Phenomenological Aspects of Effective Gauge Theo- ries' Thesis advisor: Prof. Lawrence Krauss Brown University, Providence, Rhode Island Participant in the 1988 Theoretical Advanced Summer Institute University of Sydney, Australia B.Sc with First Class Honours in Mathematics and Physics, Dec. 1984 AWARDS, DISTINCTIONS J. J. Sakurai Prize in Theoretical Particle Physics, American Physical Society, 2019. Distinguished Visiting Research Chair, Perimeter Institute, 2012 - present. 2 Moore Fellow, Cal Tech, 2015. American Association for the Advancement of Science, Fellow, 2011. -
Outreach Activities, Web, Radio&TV, Non-Specialized Conferences And
1 Laboratoire de Physique des Hautes Energies (LPHE) Outreach activities, web, radio&TV, non-specialized conferences and publications April 2009 { March 2016 We list here activities aiming at making our research known to less specialized audiences, or more generally to the public at large. April 2015 { March 2016 1. C. Fitzpatrick, guide for visit at CERN of students from Campbell College Belfast, March 19, 2016. 2. O. Schneider, visit organized at CERN (at LHCb, CAST, and LHC magnets) for 60 Bachelor students of EPFL, November 17, 2015. 3. I. Komarov, \On the irreversibility of time and Einstein's theory", online lecture for children in the framework of the \Scientists to kids" project, Experimentarium Museum, Moscow, Russia, October 24, 2015. 4. CERN Courier: \LHCb improves trigger in Run 2", September 25, 2015. 5. O. Schneider, participation in an interdisciplinary podium discussion \Le boson de Higgs { architecte de l'Univers ?" after a public screening of the movie \Particle Fever" (flyer), Lyc´ee-Coll`egedes Creusets, Sion, Switzerland, September 25, 2015. 6. LHCb public web site: \First LHC run2 physics results: measurement of J= production cross- sections in pp collisions at 13 TeV", July 24, 2015. 7. EPFL news: \EPFL contributes to breakthrough experiment at CERN"(\L'EPFL contribue `aune d´ecouverte majeure au CERN", May 21, 2015. 8. EPFL news: \Tatsuya Nakada awarded Honorary Doctorate from University of Zurich"(\Tatsuya Nakada honor´epar l'Universit´ede Zurich"), May 4, 2015. 9. V. Battista, \LHCb: tra bellezza e asimmetrie", science popularization article published in \Quaderni di scienza e scienziati molisani", 2015. April 2014 { March 2015 1. -
Speed of Light and Rates of Clocks in the Space Generation Model of Gravitation, Part 1
GravitationLab.com Speed of Light and Rates of Clocks in the Space Generation Model of Gravitation, Part 1 1 R. BENISH( ) (1) Eugene, Oregon, USA, [email protected] Abstract. — General Relativity’s Schwarzschild solution describes a spherically symmetric gravi- tational field as an utterly static thing. The Space Generation Model (SGM) describes it as an absolutely moving thing. The SGM nevertheless agrees equally well with observations made in the fields of the Earth and Sun, because it predicts almost ex- actly the same spacetime curvature. This success of the SGM motivates deepening the context—especially with regard to the fundamental concepts of motion. The roots of Einstein’s relativity theories thus receive critical examination. A particularly illumi- nating and widely applicable example is that of uniform rotation, which was used to build General Relativity (GR). Comparing Einstein’s logic to that of the SGM, the most significant difference concerns the interpretation of the readings of accelerom- eters and the rates of clocks. Where Einstein infers relativity of motion and space- time symmetry, it is argued to be more logical to infer absoluteness of motion and spacetime asymmetry. This approach leads to reassessments of the essential nature of matter, time, and the dimensionality of space, which lead in turn to some novel cos- mological consequences. Special emphasis is given to the model’s deviations from standard predictions inside matter, which have never been tested, but could be tested by conducting a simple experiment. PACS 04.80.Cc – Experimental tests of gravitational theories. 1. – Introduction; Intended Audience Beware ye, all those bold of spirit who want to suggest new ideas. -
Curating the Collider: Using Place to Engage Museum Visitors with Particle Physics
Science Museum Group Journal Curating the collider: using place to engage museum visitors with particle physics Journal ISSN number: 2054-5770 This article was written by Alison Boyle, Harry Cliff 10-09-2014 Cite as 10.15180; 140207 Research Curating the collider: using place to engage museum visitors with particle physics Published in Autumn 2014, Issue 02 Article DOI: http://dx.doi.org/10.15180/140207 Abstract CERN’s Large Hadron Collider, the world’s largest particle physics facility, provides museological opportunities and challenges. Visitor interest in cutting-edge physics, with its high media profile, is tempered by anxiety about understanding complex content. The topic does not readily lend itself to traditional museum showcase-dominated displays: the technology of modern particle physics is overwhelmingly large, while the phenomena under investigation are invisible. For Collider, a major temporary exhibition, the Science Museum adopted a ‘visit to CERN’ approach, recreating several of the laboratory’s spaces. We explore the effectiveness of this approach, at a time when historical studies of scientific laboratories and museum reconstructions of spaces are subject to renewed interest. Component DOI: http://dx.doi.org/10.15180/140207/001 Keywords Science Museum, Collider, Large Hadron Collider, CERN, particle physics, place, space, re-creation, room set, museum Introduction Collider: step inside the world’s greatest experiment ran at the Science Museum from November 2013–May 2014 and is touring internationally until 2017. The exhibition covers the work of the Large Hadron Collider (LHC) at CERN, the world’s largest particle physics facility. Strategically, the subject matter had obvious appeal for the Science Museum, with its long term ambitions to tackle complex scientific topics, attract more adult visitors, and raise its international profile (Science Museum, 2012). -
The Higgs Boson and Big Science Sarah Eno, U. Maryland MASP Lectur
How many physicists does it take to discover a new particle? The Higgs Boson and Big Science Sarah Eno, U. Maryland MASP lecture 29 April 08 Sarah Eno 1 4 July 2012 CERN Auditorium: announcement of a new particle 8 October 2013 20 May 2014 Sarah Eno, MASP lecture 2 Two Experiments CMS ATLAS 20 May 2014 Sarah Eno, MASP lecture 3 Each with a paper Discoveries are made by people, not by detectors. 20 May 2014 Sarah Eno, MASP lecture 4 CMS: Discovery courtesy of: 20 May 2014 Sarah Eno, MASP lecture 5 20 May 2014 Sarah Eno, MASP lecture 6 20 May 2014 Sarah Eno, MASP lecture 7 20 May 2014 Sarah Eno, MASP lecture 8 20 May 2014 Sarah Eno, MASP lecture 9 20 May 2014 Sarah Eno, MASP lecture 10 20 May 2014 Sarah Eno, MASP lecture 11 2892 authors from 168 institutions This is just the CMS paper. There is a similar list for ATLAS. 20 May 2014 Sarah Eno, MASP lecture 12 Outline • What is the Higgs boson? • How do we know that it was created in proton-proton collisions at the Large Hadron Collider • What do all those people actually do? 20 May 2014 Sarah Eno, MASP lecture 13 Particle Fever Assistant Professor Alberto Belloni 20 May 2014 Sarah Eno, MASP lecture 14 What is a Higgs Boson? 20 May 2014 Sarah Eno, MASP lecture 15 Before we talk about the Higgs, let’s think about forces Is it this? Particle physicists think of it as this: Force boson Matter: Quarks (protons) leptons (electron) matter Some more force bosons 20 May 2014 Sarah Eno, MASP lecture 16 Only four of them, each with a “boson” Electricity and Magnetism (QED) photon Strong Force (QCD) gluon Weak Force 1H + 1H ® 2 H + e+ +n 1 1 1 W&Z bosons 20 May 2014 Sarah Eno, MASP lecturehttp://www.dreamstime.com/powerplant-infrastructure-stock-photo-imagefree242420 17 Fourth is gravity, but since its effects are negligible when considering particle collisions at accelerators, I’ll ignore it. -
T R U S T E D . V a L U E D . E S S E N T I A
Trusted. Valued. Essential. JUNE 2018 Helping Our People Helping People It’s a guiding principle at Silver State Schools Credit Community Union. Since 1951, we have been fully-vested in the Southern Nevada community we serve. Whether it’s setting up your child’s first savings account, finding a Through Life’s great rate on a loan, buying your first home or finding the best investment, our employees are available to Financial Journey put your best interests first. Become a member today and experience the SSSCU difference. 800.357.9654 silverstatecu.com Vegas PBS A Message from the Management Team General Manager General Manager Tom Axtell, Vegas PBS Educational Media Services Director Niki Bates Production Services Director Kareem Hatcher Communications and Brand Management Director Shauna Lemieux Business Manager Brandon Merrill Content Director In Remembrance of Cyndy Robbins Workforce Training & Economic Development Director Charlotte Hill Debra Solt Corporate Partnerships Director Bruce Spotleson n 1971, Charlotte Hill convened a group of community leaders who founded Director of Engineering, IT and Emergency Response “Friends of Channel 10” to provide financial support for KLVX, Nevada’s first John Turner educational public television station – and she never left us. Over the next 47 Southern Nevada Public Television Board of Directors years, she would dedicate untold hours of support to the station; raise millions of Executive Director dollars through auctions and wine tastings; recruit a virtual army of volunteers; Tom Axtell, Vegas PBS Iand troop through the marbled halls of Congress to secure support despite blizzards President Nancy Brune, Guinn Center for Policy Priorities and thunderstorms. -
CHIPP Roadmap for Research and Infrastructure 2025–2028 and Beyond by the Swiss Particle Physics Community IMPRINT
Vol. 16, No. 6, 2021 swiss-academies.ch CHIPP Roadmap for Research and Infrastructure 2025–2028 and beyond by the Swiss Particle Physics Community IMPRINT PUBLISHER Swiss Academy of Sciences (SCNAT) · Platform Mathematics, Astronomy and Physics (MAP) House of Academies · Laupenstrasse 7 · P.O. Box · 3001 Bern · Switzerland +41 31 306 93 25 · [email protected] · map.scnat.ch @scnatCH CONTACT Swiss Institute of Particle Physics (CHIPP) ETH Zürich · IPA · HPK E 26 · Otto-Stern-Weg 5 · 8093 Zürich Prof. Dr. Rainer Wallny · [email protected] · +41 44 633 40 09 · chipp.ch @CHIPP_news RECOMMENDED FORM OF CITATION Wallny R, Dissertori G, Durrer R, Isidori G, Müller K, Rivkin L, Seidel M, Sfyrla A, Weber M, Benelli A (2021) CHIPP Roadmap for Research and Infrastructure 2025–2028 and beyond by the Swiss Particle Physics Community Swiss Academies Reports 16 (6) SCNAT ROADMAPS COORDINATION Hans-Rudolf Ott (ETH Zürich) · Marc Türler (SCNAT) CHIPP ROADMAP EDITORIAL BOARD A. Benelli (secretary) · G. Dissertorib · R. Durrerd · G. Isidoric · K. Müllerc · L. Rivkina, g · M. Seidela, g · A. Sfyrlad R. Wallnyb (Chair) · M. Weberf CONTRIBUTING AUTHORS A. Antogninia, b · L. Baudisc · HP. Beckf · G. Bisona · A. Blondeld · C. Bottac · S. Braccinif · A. Bravard · L. Caminadaa, c F. Canellic · G. Colangelof · P. Crivellib · A. De Cosab · G. Dissertorib, M. Donegab · R. Durrerd · M. Gaberdielb · T. Gehrmannc T. Gollingd, C. Grabb · M. Grazzinic · M. Hildebrandta · M. Hoferichterf · B. Kilminstera · K. Kircha, b · A. Knechta · I. Kreslof B. Kruschee · G. Iacobuccid · G. Isidoric · M. Lainee · B. Laussa, M. Maggiored · F. Meiera · T. Montarulid · K. Müllerc A. Neronovd, 1 · A. -
Naturalness Under Stress Arxiv:1501.01035V2 [Hep-Ph]
hep-th/yymmnnn SCIPP 14/15 Naturalness Under Stress Michael Dine Santa Cruz Institute for Particle Physics and Department of Physics, Santa Cruz CA 95064 Abstract Naturalness has for many years been a guiding principle in the search for physics beyond the Standard Model, particularly for understanding the physics of elec- troweak symmetry breaking. However, the discovery of the Higgs particle at 125 GeV, accompanied by exclusion of many types of new physics expected in natural models has called the principle into question. In addition, apart from the scale of weak interactions, there are other quantities in nature which appear unnaturally small and for which we have no proposal for a natural explanation.We first review the principle, and then discuss some of the conjectures which it has spawned. We then turn to some of the challenges to the naturalness idea and consider alterna- tives. arXiv:1501.01035v2 [hep-ph] 8 Jan 2015 1 Naturalness: A Contemporary Implementation of Dimensional Analysis In our first science courses we learn about the importance of dimensional analysis. Often this is presented as a consistency requirement for calculations of physical quantities. But it shapes our understanding of physical systems in a fundamental way. For example, from the electron mass, me, the speed of light, c, and Plancks constant, ~ we can form a ~ −15 quantity with dimensions of length: a = mc ≈ 10 cm: supplemented with the insight that the strength of the force between the proton and the electron is proportional to e2, 2 ~ so the size should get larger as e , or a = mce2 : To know the exact coefficient { which is an order one number { we need to solve the Schrodinger equation completely. -
The Hierarchy Problem and New Dimensions at a Millimeter
18 June 1998 Physics Letters B 429Ž. 1998 263±272 The hierarchy problem and new dimensions at a millimeter Nima Arkani±Hamed a, Savas Dimopoulos b, Gia Dvali c a SLAC, Stanford UniÕersity, Stanford, CA 94309, USA b Physics Department, Stanford UniÕersity, Stanford, CA 94305, USA c ICTP, Trieste 34100, Italy Received 12 March 1998; revised 8 April 1998 Editor: H. Georgi Abstract We propose a new framework for solving the hierarchy problem which does not rely on either supersymmetry or technicolor. In this framework, the gravitational and gauge interactions become united at the weak scale, which we take as the only fundamental short distance scale in nature. The observed weakness of gravity on distances R 1 mm is due to the G ; y1r2 existence of n 2 new compact spatial dimensions large compared to the weak scale. The Planck scale MPl GN is not a fundamental scale; its enormity is simply a consequence of the large size of the new dimensions. While gravitons can freely propagate in the new dimensions, at sub-weak energies the Standard ModelŽ. SM fields must be localized to a 4-dimensional manifold of weak scale ``thickness'' in the extra dimensions. This picture leads to a number of striking signals for accelerator and laboratory experiments. For the case of ns2 new dimensions, planned sub-millimeter measurements of gravity may observe the transition from 1rr 2 ™1rr 4 Newtonian gravitation. For any number of new dimensions, the LHC and NLC could observe strong quantum gravitational interactions. Furthermore, SM particles can be kicked off our 4 dimensional manifold into the new dimensions, carrying away energy, and leading to an abrupt decrease in R events with high transverse momentum pT TeV.