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Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

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Presentation on theme: "Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)"— Presentation transcript:

1 Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

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3 Feynman rules: If energy E flows through the transmitted “virtual” particle (photon; Z) it costs 1/(E^2+M^2) If E >> M the cost is 1/E^2….like the case of the photon Only appears weak at low energy. Unified at high energy

4 WEAK STRONG

5 WEAK STRONG  why sun has shone for 5 Byr…  Intelligent life developed

6 The weak force is feeble in the Sun…..because 10,000,000K ~ 1 keV << 80 GeV The weak force is feeble in the Sun …this is why the sun has stayed active long enough for us to have evolved and be having this conversation.  We exist because m(W) is not zero  Mass matters

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8 Mc^2 >0 Gravity PE <0 Total E =0 (?!)

9 Mc^2 >0 Gravity PE <0 Total E =0 (?!)

10 Heisenberg: E ->0 t ->infinity “Universe erupted as quantum fluctuation out of nothing” (what/where/how encoded Heisenberg in “nothing”? Mc^2 >0 Gravity PE <0 Total E =0 (?!)

11 Heisenberg: E ->0 t ->infinity “Universe erupted as quantum fluctuation out of nothing” (what/where/how encoded Heisenberg in “nothing”? Mc^2 >0 Gravity PE <0 Total E =0 (?!)

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13 Quarks “freeze” into protons/neutrons

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19 Nuclear Physics

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21 symmetry pattern symmetry pattern

22 symmetry pattern symmetry pattern

23 symmetry pattern symmetry pattern Atoms

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25 3K microwave bgnd now seen to have structure COBE 2000 WMAP 2003

26 5byr ago accelerated expansion = Dark Energy. What? Why?......

27 One further symmetry??

28 Whole new families to be found

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30 Finale: A glimpse of the future recall from lecture 1….. Temperature Energy and Time The Universe in

31 …and the nature of matter

32 …and patterns (that change)

33 symmetry pattern Temperature and symmetry in the universe

34 The Idea (I will tell you when to be cautious about inhaling)

35 Symmetry when warm (high energy) patterns and structures when cold (low energy)

36 GrandUnified Force Electromagnetic Weak Strong ElectroWeak Strong (QCD) FORCES 1955-2005 COLD WARM HOT

37 Standard Model of Quarks Leptons and forces = pattern based on mass “cold” =“low” energy = below 1 TeV

38 superSymmetry when “warm” (= high energy > 1TeV ) Higgs Boson Supersymmetry Nature of Reality Standard Model of Quarks Leptons and forces = pattern based on mass “cold” =“low” energy = below 1 TeV

39 symmetry pattern symmetry pattern

40 5. symmetries can disappear or change

41 We like symmetry and when its absent we want to know why ?

42 Buridan’s Ass

43 The problem of the symmetric dinner party

44 symmetry Broken symmetry

45 Why is this a peak and not a trough? Broken symmetry Answer: random chance But given it’s a peak here it dictates where the other peaks are

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47 Symmetry when warm (high energy) patterns and structures when cold (low energy)

48 … “froze” into structures …. And patterns Such as Atoms ……. Mendeleev’s periodic table, And particles …. Quarks, forces and the Standard Model As the universe cooled after the hot big bang….. We think that an elegant symmetry…….. … which is a pattern based on MASS 2008: heat up to energies above 1000 GeV = “1 TeV” and discover the origin of MASS (= Higgs?)

49 Next ….

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51 More in Vsi And particle odyssey A Very Short Introduction

52 The Particle Odyssey A Journey to the Heart of matter Frank Close, Michael Marten, Christine Sutton

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