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Science Seminar Winter week 9, Monday.6.March.2006 Finishing up Physics of Star Trek Next week: eval conferences  sign up today  Friday: self-eval survey.

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Presentation on theme: "Science Seminar Winter week 9, Monday.6.March.2006 Finishing up Physics of Star Trek Next week: eval conferences  sign up today  Friday: self-eval survey."— Presentation transcript:

1 Science Seminar Winter week 9, Monday.6.March.2006 Finishing up Physics of Star Trek Next week: eval conferences  sign up today  Friday: self-eval survey  email peer evals, etc. Movie: Understanding the Universe

2 Next week Eval conferences in 2272 Lab II – come 5 minutes early! Bring your  finished portfolio  hardcopy self-eval (3 copies on official form)  hardcopy eval of faculty (official form not required – 1 copy to Zita or to secretaries in 2250 Lab II)

3 Preparing: Discuss portfolios & evals. Read online guidelines (skim together). Include all responses to your essays, with authors and dates. Include all your responses, with original essays. E-portfolios are fine (optional). Make them *complete and *easy to read, with all links in one central, concisely annotated document (e.g. a web page). Advising and Writing Center have portfolio & eval workshops

4 This Friday: email to Zita Peer evaluations (a couple of sentences – be honest and specific – not on official forms) Paragraph from your best essay (50-100 words), with WebX link and reference Take Self-Eval survey online by Friday No new essays due this week.

5 New physics Changes since Physics of Star Trek and the movie came out: What is Dark Matter? We know better now:  NOT ordinary matter: less than 5% of dark matter is protons, neutrons, stars, MACHOS, …  Neutrinos are significant – though they have tiny mass, there are very many of them (over 10 90 ), but still they are less than 30% of dark matter  Probably WIMPS – Weakly Interacting Massive Particles – not yet discovered...

6 Newer physics Most of Dark Matter (70%?) may be Dark Energy!  Dark Matter is whatever causes the observed (for decades) gravitational dynamics in galaxies – most of it does not shine  Dark Energy is whatever causes the observed (since about 2001) ACCELERATING expansion of the universe  What is Dark Energy? Vacuum pressure due to virtual particle creation? How strong is it? Does it change through history?

7 Dark Energy, Dark Matter, and the Universe More questions and some answers next quarter in Science Seminar: Cosmology Quintessence (A Very Short Introduction) by Lawrence Krauss (same guy)by Peter Coles

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