2. The Celebration of Undergraduate Research Valparaiso University Spring 2009 Expect Surprises! Donald D. Koetke Department of Physics and Astronomy

3. (Prof. Randy Fisk) Prof. David Grosnick Prof. Robert Manweiler Mr. Paul Nord Prof. Shrivel Stanislaus MANY students Expect Surprises! Donald D. Koetke Department of Physics and Astronomy

4. 1. Whatever you think you understand about your science today - be prepared to modify that as time goes on -- sometimes rather dramatically! Expect Surprises!

5. Bubble Chambers Detector Systems - then

6. Bubble Chambers Detector Systems - then First neutrino interaction with hydrogen First observations of the  -

7. Many discoveries & surprises! - The elementary particle zoo - And their antimatter twins! BaryonsMesons The fundamental building blocks of nature

8. The Standard Model of Particle Physics

9. antiMatter antiQuark antiLepton

10. The Standard Model of Particle Physics

11. Fundamental Interactions in Nature - The Standard Model - The good news: The SM is enormously successful - The SM is enormously successful - Essentially every experiment yields results that agree with the SM! Essentially every experiment yields results that agree with the SM! It postulates: the mechanism for particles acquiring mass is due to the Higgs particle/field as yet unfound. (Will FNAL-tevatron or CERN-LHC find the Higgs?) It postulates: the mechanism for particles acquiring mass is due to the Higgs particle/field as yet unfound. (Will FNAL-tevatron or CERN-LHC find the Higgs?)

12. Fundamental Interactions in Nature - The Standard Model - The bad news: The SM is not a fundamental theory - The SM is not a fundamental theory - - Over 20 numbers must be put in from experiment: particle masses, lifetimes, spins, etc. - Conservation laws are put in ad hoc - It does not explain the matter - antimatter asymmetry - It is “broken” by two fundamental measurements! - It does not include gravity, i.e., it is not a unified theory - And more… (stay tuned) - Over 20 numbers must be put in from experiment: particle masses, lifetimes, spins, etc. - Conservation laws are put in ad hoc - It does not explain the matter - antimatter asymmetry - It is “broken” by two fundamental measurements! - It does not include gravity, i.e., it is not a unified theory - And more… (stay tuned)

13. Homestake Mine Neutrino Observatory Dr. Ray Davis, Univ. of PA, BNL e 4,500 ft e e     Neutrino oscillations are discovered! Neutrinos must have mass!! Neutrino oscillations are discovered! Neutrinos must have mass!! Expect Surprises!

14. 2. The more you learn and know, the more questions you will discover beg for answers ! This is really good news! You are not ever going to get “there”. Expect Surprises! Here is my list of outstanding questions and upcoming surprises.

15. Expect Surprises! - Why do particles have mass? The Higgs mechanism? Will the Higgs be found at the LHC? - Why do particles have their specific masses? - What other surprises will come from the LHC? - What, causes the proton to have a specific intrinsic angular momentum (spin)? (Watch our spin experiment) (Watch our spin experiment) - What happened to all of the antimatter created in the Big Bang? (Watch our nEDM expt) STAR

16. Expect Surprises! - Why are some conservation laws followed? Will there be some allowed violation? - What will happen to the quark-gluon plasma at LHC energies? - What will be the next particle accelerator? Will we be able to afford it? Where will it be sited? - What will replace the present Standard Model? - What will be the near term impacts of global warming?

17. Expect Surprises! - What is the dark matter? WIMPs ? WIMPs ? Brown dwarfs? Brown dwarfs? Large black holes? Large black holes? A new form of matter? A new form of matter? - What is the dark energy? Antigravity? Antigravity? A new source of energy? A new source of energy? Completely new science? Completely new science? “Atoms” = 4.6% Free hydrogen & helium = 4% Stars = 0.5% Neutrinos = 0.3% Heavy Elements = 0.03% Dark Matter & Dark Energy - 95% we cannot see! And, we don’t know what it is!

18. That’s my list. What’s yours? Expect Surprises!

19. 3. Science is evermore a collaborative experience. You will meet and work with some extraordinary people: Very bright Often kind and helpful Critical but friendly There will be a few that are NOT! Choose how to deal with it … Expect Surprises!

20. 4.There is subjectivity in science. BUT - avoid injecting your own biases. There are powerful forces that want to corrupt your objectivity - - Previous results can distort your objectivity - “Get the right answer” : it’s been part of our experience. - When do you stop looking for problems in your work? Expect Surprises!

21. HistoryHistory

22. HistoryHistory

23. 4.There is subjectivity in science. BUT - avoid injecting your own biases. There are powerful forces that want to corrupt your objectivity - - Previous results can distort your objectivity - “Get the right answer” : it’s been part of our experience. - When do you stop looking for problems in your work? - Consider blind analysis! Expect Surprises!

24. 5. Aim high! You should expect surprises. Expect Surprises!

25. Concordia Valparaiso University

26. Concordia DOE Contract

27. Student film scanners Bubble Chambers Learned to recognize physics events of interest Student Research Students These events were then digitized and analyzed

28. DOE - ANL Contract DOE Medium Energy Nuclear Physics Grant Concordia Valparaiso University

29. 6.Not everyone will be as excited about what you do as you are. - Work at getting them interested if not excited. - Keep your own perspective There are other important things in life! 6.Not everyone will be as excited about what you do as you are. - Work at getting them interested if not excited. - Keep your own perspective There are other important things in life! Expect Surprises!

30. 7. Accept unpleasant surprises in your work and move on. Search for “neutral currents” with elastic scattering of neutrinos on hydrogen. The MEGA disaster… Expect Surprises!

31. Concordia Valparaiso University MEGA 10 14 0 500 MHz instantaneous decay rate Background ~ (beam rate) 8 Background ~ (beam rate)

32. 8. Don’t become jaded; step back and reflect on what has happened or developed or been learned. - Be amazed! - Marvel at what can be accomplished or learned. - Expect that more surprises will come. Expect Surprises!

33. 9. Research is hard work. - The ratio of hard work to great discoveries is very large! (Even small discoveries.) Draw strength from the work of others. - Enjoy being part of the larger enterprise! Expect Surprises!

34. 10.Enjoy what you do and share that joy and enthusiasm with others as much as possible. If you don’t, who will? If you don’t, who will? Expect Surprises! Thank you