Astrophysics Seminars

Nov
19
2009

Institute for Advanced Study Informal Astrophysics Seminar

The Effective Theory of Quintessence and Its Observational Signatures
Guido D'Amico
11:30am|Bloomberg Hall Astrophysics Library
I will study generic single-field dark energy models, by a parametrization of the most general theory of their perturbations around a given background, including higher derivative terms. In appropriate limits this approach reproduces standard...
Nov
12
2009

Institute for Advanced Study Informal Astrophysics Seminar

Approaches to Understanding Inflation: Theory, Experiment, and Observation
Mark Hertzberg
11:30am|Bloomberg Hall Astrophysics Library
Although the observational evidence for cosmological inflation is growing, the physical mechanism behind it is still unknown. In part this is because inflation probably occurred at energy scales many orders of magnitude higher than that at man-made...
Nov
10
2009

Institute for Advanced Study Astrophysics Seminar

Chromospheric Activity in Low-Mass Stars
Jill Knapp
11:00am|Bloomberg Hall Astrophysics Library
Magnetic activity in the Sun manifests itself as sunspot activity, flares, and reversals in the CaII H and K lines, and is believed to originate in the transition region between the convective and radiative zones. Lower- mass stars become fully...
Oct
29
2009

Institute for Advanced Study Informal Astrophysics Seminar

Ly-alpha Emission from Galaxy Formation
Claude-André Faucher-Giguère
11:30am|Bloomberg Hall Astrophysics Library
Astronomers have exquisite observations of both galaxies (by directly imaging their stars) and of the intergalactic medium (in absorption spectra of background sources). While we know that the galactic baryons must have been accreted from the IGM...
Oct
22
2009

Institute for Advanced Study Informal Astrophysics Seminar

Balancing Outflows and Gas Dilution: The Mass-Metallicity Relation at z=0
Molly Peeples
11:30am|Bloomberg Hall Astrophysics Library
The gas-phase oxygen abundances of star-forming galaxies are tightly correlated with the galaxies' stellar masses such that more massive galaxies are more oxygen-rich. Because oxygen is produced on relatively short timescales (~10 Myr), this so...