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Intro to Particle Physics Physics 165 Richard Seto I work at RHIC (PHENIX expt) I do far too much bureaucracy (money, people…) I like to think about all.

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Presentation on theme: "Intro to Particle Physics Physics 165 Richard Seto I work at RHIC (PHENIX expt) I do far too much bureaucracy (money, people…) I like to think about all."— Presentation transcript:

1 Intro to Particle Physics Physics 165 Richard Seto I work at RHIC (PHENIX expt) I do far too much bureaucracy (money, people…) I like to think about all kinds of stuff teaching 165 is part of the stuff I like

2 The course All relevant info on blackboard All relevant info on blackboard Book – Particle Physics – Martin/Shaw Book – Particle Physics – Martin/Shaw TA - Shih-Chuan Kao TA - Shih-Chuan Kao PS 1 is up due…. PS 1 is up due…. Problem sets ~ 1 every 1-2 weeks Problem sets ~ 1 every 1-2 weeks a late midterm a late midterm Presentation Presentation 5-10 page paper (actually there is not a page limit) 5-10 page paper (actually there is not a page limit)

3 Lectures – Scope of the course Lecture and PS – first 2/3 of course Lecture and PS – first 2/3 of course Leptons/quarks, forces (our corner of the universe) Leptons/quarks, forces (our corner of the universe) Particle Detection Particle Detection Field Theory and Symmetries (how we do it) Field Theory and Symmetries (how we do it) QED and Electo-weak theory QED and Electo-weak theory Quantum Chromodymamics Quantum Chromodymamics Grand Unification Grand Unification Dark Energy – The problem Dark Energy – The problem Strings and other things Strings and other things

4 Some possible topics (not exhaustive) The LHC or one of the LHC detectors and what they might see The LHC or one of the LHC detectors and what they might see Past experiments Past experiments Dark energy Dark energy Dark matter Dark matter Particle Detection techniques (e.g. gas drift chambers, calorimeters, Silicon detectors etc – pick one). Particle Detection techniques (e.g. gas drift chambers, calorimeters, Silicon detectors etc – pick one). RHIC and its experiments RHIC and its experiments FNAL/CDF/D0 FNAL/CDF/D0 Space based experiments (e.g. GLAST) Space based experiments (e.g. GLAST) Underground searches Underground searches Attempts at unification Attempts at unification For someone with a taste for something tough For someone with a taste for something tough a real analysis a real analysis a real theoretical calculation a real theoretical calculation Sources Sources Folks at UCR Folks at other universities Scientific American Journal articles The web Your brain Books at the library

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6 What is the world made of?

7 What is the world made of? 1 Ancient Greeks

8 What is the universe made of? 2 Mendelev But why? Fundamental?

9 n p e-e- Bohr Model Most of our existence is here electrons give us chemistry! people, elements protons and neutrons give us nuclear physics, energy, stars,…

10 In our class we will spend most of our time here Proton Is this all there is? Is it fundamental

11 Standard Model Probably best tested Theory of all time. Probably best tested Theory of all time. Drives physicists nuts Drives physicists nuts EVERYTHING WORKS EVERYTHING WORKS Are we done? Are we done? Why are the masses what they are Why are the masses what they are e.g. why don’t you weigh twice what you do? e.g. why don’t you weigh twice what you do? Why are the strengths of the interactions what they are Why are the strengths of the interactions what they are Why isn’t gravity 1% stronger? Why isn’t gravity 1% stronger?

12 Problems… problems… problems… velocity

13 Universe expansion is Accelerating!

14 Why? repulsive gravity (aka anti-gravity) vacuum energy Note – a quick calculation from what we know gets this wrong by ~ 120 orders of magnitude quintessence

15 What is the universe made of? Is that all there is?

16 Is that all there is? Wimp? Dark matter? Supersymmetry?

17 Is it fundamental?? In fact why do we want to work in only 4-D? Go to 11-D Go to 11-D THEORY of EVERYTHING?

18 Other questions why does time go forward? what defines forward in time? why does time go forward? what defines forward in time? Why do we think symmetries govern everything? Why do we think symmetries govern everything? can we understand field theory/QM? can we understand field theory/QM? Are the “fundamental” constants really fundamental or is it just like the direction of “down” Are the “fundamental” constants really fundamental or is it just like the direction of “down” Why are the fundamental constants where they are? Why are the fundamental constants where they are? Why are we here? Why are we here?

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22 The presentation and paper Pretend you are a researcher (actually – no need to pretend – you are!) Pretend you are a researcher (actually – no need to pretend – you are!) Give a talk, write it up Give a talk, write it up Purpose Purpose Learn deeply about a topic Learn deeply about a topic Teach your friends about it Teach your friends about it Learn to prepare a presentation/write a paper Learn to prepare a presentation/write a paper clarity clarity interest interest Format Format you choose a topic – you see me to discuss it you choose a topic – you see me to discuss it a practice talk in class (We all interrupt, criticize etc) a practice talk in class (We all interrupt, criticize etc) A real talk in class (I keep my mouth shut – Students can ask questions) A real talk in class (I keep my mouth shut – Students can ask questions) use last several weeks+exam date use last several weeks+exam date turn In paper during exam week turn In paper during exam week

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28 Hubble diagram: Redshift z m = - 2.5 log F + cst = 5 log (H 0 D L ) + M - 5 log H 0 + 25 H 0 D L cz z  0 measure of H 0 Large z : measure of  m,   Magnitude m older fainter 1+z = a(t obs )/a(t em ) At a given z Supernova Cosmology Project Accelerated expansion = smaller rate in the past = more time to reach a given z = larger distance of propagation of the photons = smaller flux 

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30 Redshift z Magnitude m older fainter 1+z = a(t obs )/a(t em ) At a given z Supernova Cosmology Project Accelerated expansion = smaller rate in the past = more time to reach a given z = larger distance of propagation of the photons = smaller flux  Older, receding faster further away


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