"Statistical Analysis of Stellar Evolution" (Next Week at the Statistics Seminar)
In which the starry heavens above submit to statistical analysis:
- David van Dyk, "Statistical
Analysis of Stellar Evolution"
- Abstract: Color-Magnitude Diagrams (CMDs) are plots that compare
the magnitudes (luminosities) of stars in different wavelengths of light
(colors). High non-linear correlations among the mass, color and surface
temperature of newly formed stars induce a long narrow curved point cloud in a
CMD known as the main sequence. Aging stars form new CMD groups of red giants
and white dwarfs. The physical processes that govern this evolution can be
described with mathematical models and explored using complex computer
models. These calculations are designed to predict the plotted magnitudes as a
function of parameters of scientific interest such as stellar age, mass, and
metallicity. Here, we describe how we use the computer models as a component of
a complex likelihood function in a Bayesian analysis that requires
sophisticated computing, corrects for contamination of the data by field stars,
accounts for complications caused by unresolved binary-star systems, and aims
to compare competing physics-based computer models of stellar evolution.
- This is joint work with Steven DeGennaro, Nathan Stein, William
H. Jefferys, Ted von Hippel, and Elizabeth Jeffery.
- Place and time: Doherty Hall A310, Monday, 23 November, 4--5 pm.
Enigmas of Chance;
The Eternal Silence of These Infinite Spaces;
Posted at November 19, 2009 12:02 | permanent link