Particle Physics: a practical primer

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Particle Physics: a practical primer Having fun with common manifestations of fundamental particles and interactions Andrea Pocar, University Of Massachusetts, Amherst - Saturday February 2, 2013

Particle Physics: a practical primer Having fun with common manifestations of fundamental particles and interactions Andrea Pocar, University Of Massachusetts, Amherst - Saturday February 2, 2013

Outline and goals Highlight particle physics phenomena encountered in everyday life Interplay with quantum physics and relativity Introductory remarks and examples Three/Four hands-on demonstrations, a couple of calculations List of fun examples Laundry list of much more!

Fundamental Forces gravity electromagnetic nuclear forces: strong, weak examples of each, discussion

Elementary Particles mass charge spin H Higgs

Quantum mechanics and relativity very high velocities/energies -----> special relativity particles ------> quanta of fields (very small scale) particles are also waves -----> optical phenomena (diffraction, interference, scattering)

Radioactive decays alpha, beta, gamma mean life (or half life): exponential probability table of isotopes: http://ie.lbl.gov/toi/perchart.htm http://www.nndc.bnl.gov/chart/recenter.jsp?z=56&n=80

Demo 1: Geiger counter a few available sources mystery substance!

Muons muon production in cosmic rays ~200 per square meter every second hit the surface of Eart ~100 GeV average energy http://hyperphysics.phy-astr.gsu.edu/hbase/relativ/muon.html

the Muon: the electron s cousin

Muons and relativity mean life (!) = 2.2 microseconds produced in the upper atmosphere, up to tens km up time dilation: t = q t 0 1 v 2 c 2 = t 0 relativistic energy E = q mc2 = mc 2 1 v 2 c 2

Calculate muon survival at the Earth s surface 1 GeV muons, produced at 10 km altitude:

Particle detectors general properties ionizing radiation

Discovery of the positron

Discovery of the positron

Demo 2: build a cloud chamber http://www.youtube.com/watch?v=400xfgmslqq follow handout use supercooled region to form droplets along the trail of ionization what do you see? how could you improve it?

Quarks 6 quarks, 3 pairs strong interactions, 3 colors (i.e. charges) never seen bare, i.e. isolated; they always hadronize always form color-neutral particles: baryons and mesons how many combinations are there? how many possible protons are there?

Demo 3: build baryons and mesons cut out shapes and make the baryon of your choice!

Demo 3: Calculate the top quark mass! real data from the D0 experiment at Fermilab pencil and paper http://ed.fnal.gov/samplers/hsphys/activities/ top_quark_intro.html

Demo 4: Calculate the top quark mass!

Demo 4: D0 detector at Fermilab

Demo 4: Calculate the top quark mass!

Examples How the sun burns Heavy elements: we are stardust! Carbon dating Radio-isotope batteries (betacells) X-rays: inspection of welds Smoke detectors Muon tomography Analytics with neutrons Neutron doping of silicon Much more (list)

How the Sun burns p-p Solar Fusion Chain CNO Solar Fusion Cycle p + p 2 H + e + + ν e p + e + p 2 H + ν e 12 C + p 13 N + γ 2H + p 3 He + γ 13 N 13 C + e + + ν e 3He + 3 He 4 He + 2 p 3He + p 4 He + e + + ν e 13 C + p 14 N + γ 14 N + p 15 O + γ 3He + 4 He 7 Be + γ 15 O 15 N + e + + ν e 7Be + e 7 Li + γ + ν e 7Be + p 8 B + γ 15 N + p 12 C + 4 He 7Li + p α + α 8B 2 α + e + + ν e 4p He 4 +2e + +2 e + 26.7MeV Image: bbc.co.uk

Heavy elements: we are stardust! large stars, supernovae

Carbon dating C-14 dating (half life = 5730 years)

Radioactive space propulsion Pu-238 ("-decay of 5.6 MeV, rare spontaneous fission; 90 year half life) heat up fluid that is then exhausted through a nozzle

Radio-isotope batteries (betacells) relatively old idea (pacemakers), back in fashion based on beta decays on silicon devices: low power, long-lasting

X-rays: inspections of welds

Smoke detectors air ionization between electrodes ----> current Am-241 source (430 years)

Muon tomography hidden chambers in Egyptian and Mayan temples http://www.hep.utexas.edu/mayamuon/aboutus/ http://www.ph.utexas.edu/spw/schwitters_061111.pdf fight contraband

Analytics with neutrons neutron activation analysis to measure trace elements use in non-invasive sampling of works of art

Neutron doping of silicon

Much more dark matter gravitational waves the Higgs boson dark energy inflation and cosmological evolution...