On Future High-Energy Colliders
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News from the Precision Frontier at the LHC
News from the Precision Frontier at the LHC Doreen Wackeroth [email protected]ffalo.edu Colloquium @ McMaster University Hamilton, Ontario, January 25, 2017 HEPCOS@UB is a member of the LHC CMS collaboration and gratefully acknowledges funding by the U.S. National Science Foundation The Standard Model in a nutshell The physical world at the very fundamental level follows a symmetry principle: the strong and electroweak interactions of matter particles (leptons and quarks) are prescribed by gauge symmetries, i. e. the Lagrangian L = LQCD + LEW is form-invariant, L!L, under SU(3)color and SU(2)I =isospin × U(1)Y =hypercharge transformations of the matter and gauge fields. 1 a µν;a LQCD = − 4 Gµν G Pf j µ a λa j + j=1 q¯ (x)iγ (@µ + igs Gµ(x) 2 )q (x) P ¯ µ Yf b b LEW = f ΨL;f γ (i@µ − g1 2 Bµ + g2I Wµ )ΨL;f P µ (±1+yf ) + f a¯R;f γ (i@µ + g1 2 Bµ)aR;f 1 µν 1 b µν;b − 4 Bµν B − 4 Wµν W Glashow (1961) b Bµ : U(1) gauge field, Wµ; b = 1; 2; 3 : SU(2) gauge fields ΨL;f (aR;f ): SU(2) doublet(singlet) for left(right)-handed fermions Electroweak symmetry breaking in the Standard Model The mediators of the weak interaction, the W and Z bosons, are massive, but 2 b µ,b naively introducing mass terms in L such as M Wµ W breaks the electroweak symmetry of LEW . The mechanism of spontaneous symmetry breaking allows for simultaneously generating W and Z boson masses and preserving the gauge symmetry of LEW . -
Search for New Physics in Dijet Resonant Signatures and Recent Results from Run 2 with the CMS Experiment
138 Proceedings of the LHCP2015 Conference, St. Petersburg, Russia, August 31 - September 5, 2015 Editors: V.T. Kim and D.E. Sosnov Search for new physics in dijet resonant signatures and recent results from Run 2 with the CMS experiment GIULIA D’IMPERIO Universit`aLa Sapienza and INFN Roma On behalf of the CMS Collaboration Abstract. A search for narrow resonances in proton-proton collisions at a center-of-mass energy of √s = 13 TeV is presented. The dijet invariant mass distribution of the two leading jets is measured with the CMS detector using early data from Run 2 of the Large Hadron Collider. The dataset presented here was collected in July 2015 and corresponds to an integrated luminosity of 42 1 pb− . The highest observed dijet mass is 5.4 TeV. The spectrum is well described by a smooth parameterization and no evidence for new particle production is observed. Upper limits at a 95% confidence level are set on the cross section of narrow resonances with masses above 1.3 TeV. When interpreted in the context of specific models the limits exclude: string resonances with masses below 5.1 TeV; scalar diquarks below 2.7 TeV; axigluons and colorons below 2.7 TeV; excited quarks below 2.7 TeV; and color octet scalars below 2.3 TeV. Introduction Deep inelastic proton-proton (pp) collisions often produce two or more energetic jets when the constituent partons are scattered with large transverse momenta (pT ). The invariant mass of the two jets with the largest pT in the event (the dijet) has a spectrum that is predicted by quantum chromodynamics (QCD) to fall steeply and smoothly with increasing dijet mass (m jj) [1]. -
Introduction to Jet Finding and Jetography (1)
Introduction to Jet Finding and Jetography (1) Gavin Salam CERN, Princeton University and LPTHE/Paris (CNRS) 2011 IPMU-YITP School and Workshop on Monte Carlo Tools for LHC Yukawa Institute for Theoretical Physics, Kyoto University, Japan September 2011 [Introduction] [Background knowledge] Jets Jets are everywhere in QCD But not the same as partons: Our window on partons Partons ill-defined; jets well-definable Jets lecture 1 (Gavin Salam) MC tools for LHC school September 2011 2 / 30 [Introduction] [Background knowledge] Why do we see jets? Parton fragmentation Gluon emission: dE dθ α ≫ 1 quark Z s E θ At low scales: αs → 1 Jets lecture 1 (Gavin Salam) MC tools for LHC school September 2011 3 / 30 [Introduction] [Background knowledge] Why do we see jets? Parton fragmentation Gluon emission: dE dθ α ≫ 1 quark Z s E θ θ At low scales: gluon αs → 1 Jets lecture 1 (Gavin Salam) MC tools for LHC school September 2011 3 / 30 [Introduction] [Background knowledge] Why do we see jets? Parton fragmentation Gluon emission: dE dθ α ≫ 1 quark Z s E θ At low scales: αs → 1 Jets lecture 1 (Gavin Salam) MC tools for LHC school September 2011 3 / 30 [Introduction] [Background knowledge] Why do we see jets? Parton fragmentation Gluon emission: dE dθ α ≫ 1 quark Z s E θ At low scales: αs → 1 hadronisation non−perturbative Jets lecture 1 (Gavin Salam) MC tools for LHC school September 2011 3 / 30 [Introduction] [Background knowledge] Why do we see jets? Parton fragmentation Gluon emission: π+ dE dθ α ≫ 1 quark Z s E θ KL π0 At low scales: K+ − αs → 1 hadronisation -
Theoretical Aspects of Jet Substructure
Theoretical aspects of jet substructure Mrinal Dasgupta University of Manchester Karlsruhe, July 6th 2017 Based mainly on work with Gavin Salam, Simone Marzani, Alessandro Fregoso, Andrzej Siodmok, Gregory Soyez, Lais Schunk and Alexander Powling Outline • Introduction to boosted particle searches and jet substructure • Theoretical issues in substructure studies • Jet substructure from theory first principles • Some recent progress and developments • Conclusions Boosted object hadronic decays X AT REST BOOSTED X Boosted regime implies studying particles with pT >> MX. Important at the LHC with access to TeV scales in pT. Decay products are collimated. M 2 ✓2 = p2 z(1 z) T − Hadronic two-body decays often reconstructed in single jet. Jets from QCD vs boosted heavy particles What jet do we have here? Jets from QCD vs boosted heavy particles A gluon jet ? Jets from QCD vs boosted heavy particles A quark jet ? Jets from QCD vs boosted heavy particles A W/Z/H ? Jets from QCD vs boosted heavy particles A top quark? Source: An ATLAS boosted top candidate The boosted regime implies a change in paradigm in that jets can be more than quarks and gluons. Isn’t the jet mass a clue? Looking at jet mass is not enough! Jet substructure for LHC searches Since 2008 a vibrant research field emerged based on developing and exploiting jet substructure. Butterworth, Davison Rubin, Salam 2008. Published in PRL. Builds on work by Seymour 1993. BDRS paper has over 600 citations. “Jet substructure” title search on arXiv gives > 100 papers post BDRS. BDRS method results Mass drop method + filtering Signal significance of 4 . -
Disentangling Heavy Flavor at Colliders
MIT-CTP/4880 Disentangling Heavy Flavor at Colliders Philip Ilten,1, ∗ Nicholas L. Rodd,2, y Jesse Thaler,2, z and Mike Williams1, x 1Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, MA 02139, U.S.A. 2Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, U.S.A. We propose two new analysis strategies for studying charm and beauty quarks at colliders. The first strategy is aimed at testing the kinematics of heavy-flavor quarks within an identified jet. Here, we use the SoftDrop jet-declustering algorithm to identify two subjets within a large-radius jet, using subjet flavor tagging to test the heavy-quark splitting functions of QCD. For subjets containing a J= or Υ, this declustering technique can also help probe the mechanism for quarkonium production. The second strategy is aimed at isolating heavy-flavor production from gluon splitting. Here, we introduce a new FlavorCone algorithm, which smoothly interpolates from well-separated heavy- quark jets to the gluon-splitting regime where jets overlap. Because of its excellent ability to identify charm and beauty hadrons, the LHCb detector is ideally suited to pursue these strategies, though similar measurements should also be possible at ATLAS and CMS. Together, these SoftDrop and FlavorCone studies should clarify a number of aspects of heavy-flavor physics at colliders, and provide crucial information needed to improve heavy-flavor modeling in parton-shower generators. I. INTRODUCTION The production of charm and beauty quarks at the Large Hadron Collider (LHC) is studied both as a fun- damental probe of Standard Model (SM) phenomenology, and as an important component of searches for physics beyond the SM. -
Two Notions of Naturalness
For almost 40 years, the requirement that models of BSM physics be natural has heavily inuenced model-building in high-energy physics. Porter Williams (University of Pittsburgh) Two notions of naturalness February 28, 2018 1 / 60 The expectation of a natural solution to the hierarchy problem was probably the most popular argument for expecting new particles at the LHC. Porter Williams (University of Pittsburgh) Two notions of naturalness February 28, 2018 2 / 60 The Standard Model reigns supreme. As of today, the LHC has discovered no evidence for SUSY or any other mechanism for naturally stabilizing the weak scale. Porter Williams (University of Pittsburgh) Two notions of naturalness February 28, 2018 4 / 60 As of today, the LHC has discovered no evidence for SUSY or any other mechanism for naturally stabilizing the weak scale. The Standard Model reigns supreme. Porter Williams (University of Pittsburgh) Two notions of naturalness February 28, 2018 4 / 60 This has left many people in the HEP community unsure about how to proceed. Porter Williams (University of Pittsburgh) Two notions of naturalness February 28, 2018 5 / 60 Now What? Aspen 2013 - Higgs Quo Vadis Nathan Seiberg IAS TexPoint fonts used in EMF. Read the TexPoint manual before you delete this box.: AAAAAA AA If neither supersymmetry nor any other sort of natural solution...appears in the data...[t]his would...give theorists a strong incentive to take the ideas of the multiverse more seriously. – Nima Arkani-Hamed (2012) Porter Williams (University of Pittsburgh) Two notions of naturalness February 28, 2018 8 / 60 If the electroweak symmetry breaking scale is anthropically xed, then we can give up the decades long search for a natural solution to the hierarchy problem. -
Cern Quick Facts 2017
BUDGET Total Member States’ and additional contributions 1141.7 million CHF COUNCIL CERN QUICK FACTS 2017 Normalized contributions from the Member States (%) Austria 2.17 Belgium 2.76 Bulgaria 0.29 Czech Republic 0.94 Denmark 1.77 Finland 1.35 MANAGEMENT France 14.32 Directorate Germany 20.44 Greece 1.20 Director-General Fabiola Gianotti Hungary 0.60 Director for Accelerators and Technology Frédérick Bordry Israel 1.49 Director for Finance and Human Resources Martin Steinacher Italy 10.62 Director for International Relations Charlotte Warakaulle Netherlands 4.77 Director for Research and Computing Eckhard Elsen Norway 2.90 Poland 2.82 Council Support John Pym Portugal 1.11 Internal Audit John Steel Romania 0.99 Legal Service Eva-Maria Gröniger-Voss Slovakia 0.48 Occupational Health & Safety and Environmental Protection Simon Baird Spain 7.22 Ombuds Sudeshna Datta Cockerill Sweden 2.73 Switzerland 3.92 Scientific Information Services Jens Vigen United Kingdom 15.10 Education, Communications and Outreach Ana Godinho Associate Member States in the pre-stage Host States Relations Friedemann Eder to Membership Media and Press Relations Arnaud Marsollier Cyprus 0.01 Member State Relations Pippa Wells Serbia 0.17 Non-Member State Relations Emmanuel Tsesmelis Slovenia 0.03 Protocol Service Wendy Korda Relations with International Organizations Olivier Martin Associate Member States India 1.03 Departments Pakistan 0.13 Beams (BE) Paul Collier Turkey 0.43 Engineering (EN) Roberto Losito Ukraine 0.09 Experimental Physics (EP) Manfred Krammer Finance -
Higgs Collider Phenomenology: Important Backgrounds, Naturalness Probes and the Electroweak Phase Transition
Higgs collider phenomenology: important backgrounds, naturalness probes and the electroweak phase transition. A Dissertation presented by Harikrishnan Ramani to The Graduate School in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy in Physics and Astronomy Stony Brook University August 2017 (include this copyright page only if you are selecting copyright through ProQuest, which is optional) Copyright by Harikrishnan Ramani 2017 Stony Brook University The Graduate School Harikrishnan Ramani We, the dissertation committee for the above candidate for the Doctor of Philosophy degree, hereby recommend acceptance of this dissertation Patrick Meade - Dissertation Advisor Associate Professor, Department of Physics and Astronomy George Sterman - Chairperson of Defense Distinguished Professor, Department of Physics and Astronomy Dmitri Tsybychev - Committee Member Associate Professor, Department of Physics and Astronomy Eder Izaguirre - Outside Member Assistant Physicist, Department of Physics, Brookhaven National Laboratory This dissertation is accepted by the Graduate School Charles Taber Dean of the Graduate School ii Abstract of the Dissertation Higgs collider phenomenology: important backgrounds, naturalness probes and the electroweak phase transition. by Harikrishnan Ramani Doctor of Philosophy in Physics and Astronomy Stony Brook University 2017 The Higgs boson discovered in 2012, might be the portal to new physics. With the Higgs as the common theme we present the following research arcs. In order to study the Higgs, it is important to have a very good handle on Standard model(SM) backgrounds. One such background process is SM WW production, which reported routine 3 sigma excesses in early run 1 of the LHC. However, experiments use Parton Showers for theoreti- cal prediction and this might be inadequate for exclusive cross-sections. -
Largest Temperature of the Radiation Era and Its Cosmological
View metadata, citation and similar papers at core.ac.ukLargest temperature of the radiation era brought to you by CORE and its cosmological implications provided by CERN Document Server Gian Francesco Giudice∗ CERN Theory Division, CH-1211 Geneva 23, Switzerland Edward W. Kolb NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500, and Department of Astronomy and Astrophysics, Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637-1433 Antonio Riotto Scuola Normale Superiore, Piazza dei Cavalieri 7, I-56126 Pisa, Italy, and INFN, Sezione di Pisa, I-56127 Pisa, Italy (May 2000) The thermal history of the universe before the epoch of nucleosynthesis is unknown. The maxi- mum temperature in the radiation-dominated era, which we will refer to as the reheat temperature, may have been as low as 0.7 MeV. In this paper we show that a low reheat temperature has impor- tant implications for many topics in cosmology. We show that weakly interacting massive particles (WIMPs) may be produced even if the reheat temperature is much smaller than the freeze-out temperature of the WIMP, and that the dependence of the present abundance on the mass and the annihilation cross section of the WIMP differs drastically from familiar results. We revisit predic- tions of the relic abundance and resulting model constraints of supersymmetric dark matter, axions, massive neutrinos, and other dark matter candidates, nucleosynthesis constraints on decaying parti- cles, and leptogenesis by decay of superheavy -
The Dawn of the Post-Naturalness Era Arxiv:1710.07663V1 [Physics.Hist-Ph]
CERN-TH-2017-205 The Dawn of the Post-Naturalness Era Gian Francesco Giudice CERN, Theoretical Physics Department, Geneva, Switzerland Abstract In an imaginary conversation with Guido Altarelli, I express my views on the status of particle physics beyond the Standard Model and its future prospects. Contribution to the volume \From My Vast Repertoire" { The Legacy of Guido Altarelli. 1 A Master and a Friend Honour a king in his own land; honour a wise man everywhere. | Tibetan proverb [1] Guido Altarelli was an extraordinary theoretical physicist. Not only was Guido one of the heroes of the Standard Model, but he incarnated the very essence of that theory: a perfect synthesis of pure elegance and brilliance. With his unique charisma, he had a great influence on CERN and contributed much in promoting the role of theoretical physics in the life of the laboratory. With the right mixture of vision, authority, and practical common sense, he led the Theory Division from 2000 to 2004. I have always admired Guido for his brilliance, humour, knowledge, leadership, and intellectual integrity. I learned much from his qualities and his example is a precious legacy for me and for all of his colleagues. Guido had a very pragmatic attitude towards scientific theories. He was not attracted arXiv:1710.07663v1 [physics.hist-ph] 18 Oct 2017 by elaborate mathematical constructions, but wanted to understand the essence behind the formalism and get straight to the concept. In physics, I would define him as a conservative revolutionary or as an optimistic skeptical. One episode illustrates the meaning of this definition. -
Arxiv:0801.2562V2 [Hep-Ph]
NATURALLY SPEAKING: The Naturalness Criterion and Physics at the LHC Gian Francesco GIUDICE CERN, Theoretical Physics Division Geneva, Switzerland 1 Naturalness in Scientific Thought Everything is natural: if it weren’t, it wouldn’t be. Mary Catherine Bateson [1] Almost every branch of science has its own version of the “naturalness criterion”. In environmental sciences, it refers to the degree to which an area is pristine, free from human influence, and characterized by native species [2]. In mathematics, its meaning is associated with the intuitiveness of certain fundamental concepts, viewed as an intrinsic part of our thinking [3]. One can find the use of naturalness criterions in computer science (as a measure of adaptability), in agriculture (as an acceptable level of product manipulation), in linguistics (as translation quality assessment of sentences that do not reflect the natural and idiomatic forms of the receptor language). But certainly nowhere else but in particle physics has the mutable concept of naturalness taken a form which has become so influential in the development of the field. The role of naturalness in the sense of “æsthetic beauty” is a powerful guiding principle for physicists as they try to construct new theories. This may appear surprising since the final product is often a mathematically sophisticated theory based on deep fundamental principles, arXiv:0801.2562v2 [hep-ph] 30 Mar 2008 and one could believe that subjective æsthetic arguments have no place in it. Nevertheless, this is not true and often theoretical physicists formulate their theories inspired by criteria of simplicity and beauty, i.e. by what Nelson [4] defines as “structural naturalness”. -
Basics of QCD Lecture 1: the Core Ingredients
Basics of QCD Lecture 1: the core ingredients Gavin Salam CERN Theory Unit ICTP{SAIFR school on QCD and LHC physics July 2015, S~aoPaulo, Brazil [What is QCD] QCD QUANTUM CHROMODYNAMICS The theory of quarks, gluons and their interactions It's central to all modern colliders. (And QCD is what we're made of) Gavin Salam (CERN) QCD Basics 1 2 / 24 [What is QCD] QCD predictions v. data for many processes Status: March 2015 dt Standard Model Production Cross Section Measurements L 1 Reference R[fb− ] pp 8 8 10− Nucl. Phys. B, 486-548 (2014) total ATLAS Preliminary × Jets R=0.4 0.1 < pT < 2 TeV arXiv:1410.8857 [hep-ex] y <3.0 4.5 | | Dijets R=0.4 0.3 < mjj < 5 TeV JHEP 05, 059 (2014) y <3.0, y <3.0 Run 1 √s = 7, 8 TeV 4.5 | | ∗ W PRD 85, 072004 (2012) total 0.035 Z 0.035 PRD 85, 072004 (2012) total t¯t 4.6 Eur. Phys. J. C 74: 3109 (2014) fiducial 20.3 Eur. Phys. J. C 74: 3109 (2014) PRD 90, 112006 (2014) tt chan 4.6 −total 20.3 ATLAS-CONF-2014-007 WW 4.6 PRD 87, 112001 (2013) total 20.3 ATLAS-CONF-2014-033 γγ JHEP 01, 086 (2013) fiducial 4.9 Wt 2.0 PLB 716, 142-159 (2012) total 20.3 ATLAS-CONF-2013-100 WZ 4.6 EPJC 72, 2173 (2012) total 13.0 ATLAS-CONF-2013-021 ZZ 4.6 JHEP 03, 128 (2013) total LHC pp √s = 7 TeV 20.3 ATLAS-CONF-2013-020 Wγ 4.6 PRD 87, 112003 (2013) fiducial Theory arXiv:1407.1618 [hep-ph] WW+WZ JHEP 01, 049 (2015) fiducial Observed 4.6 stat Zγ stat+syst 4.6 PRD 87, 112003 (2013) fiducial arXiv:1407.1618 [hep-ph] t¯tW 20.3 ATLAS-CONF-2014-038 total 95% CL upper limit LHC pp √s = 8 TeV t¯tZ 4.7 ATLAS-CONF-2012-126 total 20.3 ATLAS-CONF-2014-038