The mass of the Higgs boson

Similar documents
Scale symmetry a link from quantum gravity to cosmology

Where are we heading? Nathan Seiberg IAS 2016

German physicist stops Universe

Where are we heading?

Gauge coupling unification without leptoquarks Mikhail Shaposhnikov

Where are we heading? Nathan Seiberg IAS 2014

Lecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM

STANDARD MODEL and BEYOND: SUCCESSES and FAILURES of QFT. (Two lectures)

The Standard Model and Beyond

Quintessence - a fifth force from variation of the fundamental scale

Coupled Dark Energy and Dark Matter from dilatation symmetry

The Scale-Symmetric Theory as the Origin of the Standard Model

Little Higgs Models Theory & Phenomenology

PHYSICS BEYOND SM AND LHC. (Corfu 2010)

Critical lines and points. in the. QCD phase diagram

Scale invariance and the electroweak symmetry breaking

Supersymmetry, Dark Matter, and Neutrinos

Kiwoon Choi (KAIST) 3 rd GCOE Symposium Feb (Tohoku Univ.)

A model of the basic interactions between elementary particles is defined by the following three ingredients:

Lecture 18 - Beyond the Standard Model

November 24, Scalar Dark Matter from Grand Unified Theories. T. Daniel Brennan. Standard Model. Dark Matter. GUTs. Babu- Mohapatra Model

Higgs Signals and Implications for MSSM

Beyond the Standard Model

Outlook Post-Higgs. Fermilab. UCLA Higgs Workshop March 22, 2013

Particle Physics Today, Tomorrow and Beyond. John Ellis

Strongly coupled gauge theories: What can lattice calculations teach us?

The Higgs discovery - a portal to new physics

+ µ 2 ) H (m 2 H 2

The Why, What, and How? of the Higgs Boson

May 7, Physics Beyond the Standard Model. Francesco Fucito. Introduction. Standard. Model- Boson Sector. Standard. Model- Fermion Sector

The Higgs Boson and Electroweak Symmetry Breaking

Solutions to gauge hierarchy problem. SS 10, Uli Haisch

The Standard Model of particle physics and beyond

Hot Big Bang model: early Universe and history of matter

Origin of the Universe - 2 ASTR 2120 Sarazin. What does it all mean?

Dark Energy a cosmic mystery. Dunkle Energie Ein kosmisches Raetsel

Introduction to Elementary Particles

Lecture III: Higgs Mechanism

Who is afraid of quadratic divergences? (Hierarchy problem) & Why is the Higgs mass 125 GeV? (Stability of Higgs potential)

The God particle at last? Astronomy Ireland, Oct 8 th, 2012

The Standard Model of Electroweak Physics. Christopher T. Hill Head of Theoretical Physics Fermilab

solving the hierarchy problem Joseph Lykken Fermilab/U. Chicago

Potential Discoveries at the Large Hadron Collider. Chris Quigg

The God particle at last? Science Week, Nov 15 th, 2012

Lecture 23. November 16, Developing the SM s electroweak theory. Fermion mass generation using a Higgs weak doublet

Unsolved Problems in Theoretical Physics V. BASHIRY CYPRUS INTRNATIONAL UNIVERSITY

Lecture 03. The Standard Model of Particle Physics. Part III Extensions of the Standard Model

Twin Higgs Theories. Z. Chacko, University of Arizona. H.S Goh & R. Harnik; Y. Nomura, M. Papucci & G. Perez

The Large Hadron Collider, and New Avenues in Elementary Particle Physics. Gerard t Hooft, Public Lecture, IPMU Tokyo, April 16, 2015

Introduction to the Standard Model New Horizons in Lattice Field Theory IIP Natal, March 2013

The Standard Model and Beyond

Directions for BSM physics from Asymptotic Safety

Electroweak and Higgs Physics

An Introduction to Particle Physics

Astronomy 182: Origin and Evolution of the Universe

Mass (Energy) in the Universe:

Zhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016

Non-perturbative Study of Chiral Phase Transition

Done Naturalness Desert Discovery Summary. Open Problems. Sourendu Gupta. Special Talk SERC School, Bhubaneshwar November 13, 2017

A first trip to the world of particle physics

Going beyond the Standard Model of Elementary Particle Physics

Particle Physics. Tommy Ohlsson. Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden

An Introduction to the Standard Model of Particle Physics

Particles and Strings Probing the Structure of Matter and Space-Time

The Strong Interaction and LHC phenomenology

Large Hadron Collider

The cosmological constant puzzle

Electroweak Symmetry Breaking

Discovery of the Higgs Boson

FYS3510 Subatomic Physics. Exam 2016

Versatility of the Abelian Higgs Model

Astronomy, Astrophysics, and Cosmology

Higgs Physics and Cosmology

The first one second of the early universe and physics beyond the Standard Model

The Electro-Strong Interaction

Composite Higgs, Quarks and Leptons, a contemporary view

Physics 662. Particle Physics Phenomenology. February 21, Physics 662, lecture 13 1

The Standard Model Part. II

Composite Higgs Overview

Cosmology and particle physics

Beyond Standard Models Higgsless Models. Zahra Sheikhbahaee

Lecture 39, 40 Supplement: Particle physics in the LHC era

Cosmological Relaxation of the Electroweak Scale

Fundamental Particles

New Physics from Vector-Like Technicolor: Roman Pasechnik Lund University, THEP group

Particle Physics. All science is either physics or stamp collecting and this from a 1908 Nobel laureate in Chemistry

Hunting New Physics in the Higgs Sector

SFB 676 selected theory issues (with a broad brush)

EDMs from the QCD θ term

Le Modèle Standard et ses extensions

First some Introductory Stuff => On The Web.

Introduction to Particle Physics. HST July 2016 Luis Alvarez Gaume 1

Physics at e + e - Linear Colliders. 4. Supersymmetric particles. M. E. Peskin March, 2002

FYS3510 Subatomic Physics. Exam 2016

Chapter 46. Particle Physics and Cosmology

Speculations on extensions of symmetry and interctions to GUT energies Lecture 16

SUPERSYMETRY FOR ASTROPHYSICISTS

Physics 4213/5213 Lecture 1

The Strong Interaction and LHC phenomenology

The Higgs Mechanism and the Higgs Particle

Transcription:

The mass of the Higgs boson

LHC : Higgs particle observation CMS 2011/12 ATLAS 2011/12

a prediction

Higgs boson found

standard model Higgs boson T.Plehn, M.Rauch

Spontaneous symmetry breaking confirmed at the LHC

Higgs mechanism verified Higgs Brout Englert

Spontaneous symmetry breaking

Physics only describes probabilities Gott würfelt

Physics only describes probabilities Gott würfelt Gott würfelt nicht

Physics only describes probabilities Gott würfelt Gott würfelt nicht humans can only deal with probabilities

Spontaneous symmetry breaking Fermi scale

Scalar potential

Radial mode and Goldstone mode expand around minimum of potential mass term for radial mode

massless Goldstone mode

Abelian Higgs mechanism supraconductivity coupling of complex scalar field to photon

Abelian Higgs mechanism supraconductivity massive photon!

Gauge symmetry Goldstone boson is gauge degree of freedom no physical particle can be eliminated by gauge transformation in favor of longitudinal component of massive photon

Photon mass m=e φ

Standard Model of electroweak interactions : Higgs - mechanism The masses of all fermions and gauge bosons are proportional to the ( vacuum expectation ) value of a scalar field φ H ( Higgs scalar ) For electron, quarks, W- and Z- bosons : etc. m electron = h electron * φ H

lessons

1 Vacuum is complicated

mass generated by vacuum properties particles: excitations of vacuum Their properties depend on properties of vacuum

vacuum is not empty!

2 Fundamental constants are not constant

Have coupling constants in the early Universe other values than today? Yes!

Fundamental couplings in quantum field theory Masses and coupling constants are determined by properties of vacuum! Similar to Maxwell equations in matter

Condensed matter physics : laws depend on state of the system Ground state, thermal equilibrium state Example : Laws of electromagnetism in superconductor are different from Maxwells laws

Standard model of particle physics : Electroweak gauge symmetry is spontaneously broken by expectation value of Higgs scalar

Cosmology : Universe is not in one fixed state Dynamical evolution Laws are expected to depend on time

Restoration of symmetry at high temperature in the early Universe Low T SSB <φ>=φ 0 0 High T SYM <φ>=0 high T : Less order More symmetry Example: Magnets

Standard Model of electroweak interactions : Higgs - mechanism The masses of all fermions and gauge bosons are proportional to the ( vacuum expectation ) value of a scalar field φ H ( Higgs scalar ) For electron, quarks, W- and Z- bosons : etc. m electron = h electron * φ H

In hot plasma of early Universe : masses of electron und muon not different! similar strength of electromagnetic and weak interaction

electromagnetic phase transition in early universe 10-12 s after big bang most likely smooth crossover could also be more violent first order transition

Varying couplings How strong is present variation of couplings?

Can variation of fundamental constants be observed? Fine structure constant α (electric charge) Ratio electron mass to proton mass Ratio nucleon mass to Planck mass

Time evolution of couplings and scalar fields Fine structure constant depends on value of cosmon field : α(φ) in standard model: couplings depend on value of Higgs scalar field Time evolution of φ Time evolution of α Jordan,

Static scalar fields In Standard Model of particle physics : Higgs scalar has settled to its present value around 10-12 seconds after big bang. Chiral condensate of QCD has settled at present value after quark-hadron phase transition around 10-6 seconds after big bang. No scalar with mass below pion mass. No substantial change of couplings after QCD phase transition. Coupling constants are frozen.

Observation of time- or space- variation of couplings Physics beyond Standard Model

Particle masses in quintessence cosmology can depend on value of cosmon field similar to dependence on value of Higgs field

3 Standard model of particle physics could be valid down to the Planck length

The mass of the Higgs boson, the great desert, and asymptotic safety of gravity

a prediction

key points great desert solution of hierarchy problem at high scale high scale fixed point vanishing scalar coupling at fixed point

Planck scale, gravity no technicolor no multi-higgs model no low scale higher dimensions no supersymmetry

Quartic scalar coupling prediction of mass of Higgs boson = prediction of value of quartic scalar coupling λ at Fermi scale

Radial mode = Higgs scalar expansion around minimum of potential Fermi scale mass term for radial mode

Running couplings, Infrared interval, UV-IR mapping

renormalization couplings depend on length scale, or mass scale k

Running quartic scalar coupling λ and Yukawa coupling of top quark h neglect gauge couplings g

running SM couplings Degrassi et al

Partial infrared fixed point

infrared interval allowed values of λ or λ/h 2 at UV-scale Λ : between zero and infinity are mapped to finite infrared interval of values of λ/h 2 at Fermi scale

infrared interval

realistic mass of top quark (2010), ultraviolet cutoff: reduced Planck mass

ultraviolet- infrared map Whole range of small λ at ultraviolet scale is mapped by renormalization flow to lower bound of infrared interval! Prediction of Higgs boson mass close to 126 GeV

high scale fixed point

high scale fixed point with small λ predicts Higgs boson mass close to 126 GeV

key points great desert solution of hierarchy problem at high scale high scale fixed point vanishing scalar coupling at fixed point

fixed point in short-distance theory short-distance theory extends SM minimal: SM + gravity higher dimensional theory? grand unification? ( almost) second order electroweak phase transition guarantees ( approximate ) fixed point of flow needed : deviation from fixed point is an irrelevant parameter (A>2)

asymptotic safety for gravity Weinberg, Reuter

running Planck mass infrared cutoff scale k, for k=0 :

fixed point for dimensionless ratio M/k

scaling at short distances

infrared unstable fixed point: transition from scaling to constant Planck mass

modified running of quartic scalar coupling in presence of metric fluctuations + for a > 0 and small h : λ is driven fast too very small values! e.g. a=3 found in gravity computations

short distance fixed point at λ=0 interesting speculation top quark mass predicted to be close to minimal value, as found in experiment

running quartic scalar coupling Degrassi et al

Sensitivity to Higgs boson mass for given top quark mass

top prediction for known Higgs boson mass for m H =126 Gev : m t = 171.5 GeV

conclusions observed value of Higgs boson mass is compatible with great desert short distance fixed point with small λ predicts Higgs boson mass close to 126 GeV prediction in SM+gravity, but also wider class of models desert: no new physics at LHC and future colliders relevant scale for neutrino physics may be low or intermediate ( say 10 11 GeV ) - oasis in desert?

end

gauge hierarchy problem and fine tuning problem

quantum effective potential scalar field χ with high expectation value M, say Planck mass

anomalous mass dimension one loop, neglect gauge couplings g

fixed point for γ = 0 zero temperature electroweak phase transition (as function of γ ) is essentially second order fixed point with effective dilatation symmetry no flow of γ at fixed point naturalness due to enhanced symmetry small deviations from fixed point due to running couplings: leading effect is lower bound on Fermi scale by quark-antiquark condensates

critical physics second order phase transition corresponds to critical surface in general space of couplings flow of couplings remains within critical surface once couplings are near critical surface at one scale, they remain in the vicinity of critical surface gauge hierarchy problem : explain why world is near critical surface for electroweak phase transition explanation can be at arbitrary scale!

critical physics in statistical physics use of naïve perturbation theory ( without RG improvement ) would make the existence of critical temperature look unnatural artefact of badly converging expansion

self-tuned criticality deviation from fixed point is an irrelevant parameter (A>2) critical behavior realized for wide range of parameters in statistical physics : models of this type are known for d=2 d=4: second order phase transitions found, self-tuned criticality found in models of scalars coupled to gauge fields (QCD), Gies realistic electroweak model not yet found

SUSY vs Standard Model natural predictions baryon and lepton number conservation SM flavor and CP violation described by CKM matrix SM absence of strangeness violating neutral currents SM g-2 etc. SM dark matter particle (WIMP) SUSY

gravitational running a < 0 for gauge and Yukawa couplings asymptotic freedom

bound on top quark mass quartic scalar coupling has to remain positive during flow ( otherwise Coleman-Weinberg symmetry breaking at high scale) ~170 GeV