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Understanding Cultural Continuity in Korean Music

In this lecture/workshop, Dr. Donna Lee Kwon will introduce Korean music and facilitate its understanding by focusing on its unique characteristics. She will discuss traditional folk genres such as p'ungmul drumming, p'ansori, and folksongs but also bring out cultural continuities in Korean popular music as well. Come prepared to sing, dance and tap the rhythms of Korean music. 

Date:
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Location:
Niles Gallery located in the Fine Arts Library
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Cultural Differences between German and American Universities: Kaffeestunde

Have you ever thought about German culture? Do you want to know some cultural differences between colleges in Germany and the US? Are the grades any different? How are the teachers in Germany? The classes? College life? Dorms? Come to Kaffeestunde (Hour of Coffee) to hear about Germany's culture! Refreshments will be provided.

Hosted by the German Department and sponsored by the Cultural Diversity Festival.

Date:
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Location:
Max Kade German House (212 E. Maxwell Street) in the 1st floor Dining Room
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Organic Semiconductors: Bright future for old materials

Organic molecules such as tetracene crystallize into solids that can be semiconductors, metals, or even superconductors. Although they were first developed over half a century ago, it is only fairly recently that the considerable promise that organic semiconductors hold as materials for electroncs, display technologies, and solar cells has begun to be realized. Lightweight, flexible, and inexpensive, these materials offer an attractive balance between cost and performance, complemented by versatility, and functionally accomplished by means of molecular design. I will review the physics of organic semiconductors and describe how their electronic and optical properties can be utilized in a variety of applications.

Date:
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Location:
CP155

Proton and electron-hydrogen collisions for Rydberg n,l-changing transitions in the early Universe

Cosmic Microwave Background (CMB) is a vestige radiation generated during the Recombination era, some 390,000 years after the Big Bang, when the Universe had become transparent for the first time. Initial observations of CMB made by the Wilkinson Microwave Anisotropy Probe (WMAP) led to determining the age of the Universe. The mechanisms that drove the recombination have been discovered by using modeling of the primordial plasma and seeking agreement with the observations. The new Plank Surveyor Instrument launched in 2009 has been expected to produce data about the recombination era of an unprecedented accuracy, that require including better information regarding the basic atomic physics processes into the present models. In this talk, I will review the results for various Rydberg atom - charge particle collisions and establish their relative importance during the stages of recombination era, with respect to each other and to radiative processes. Energy changing and angular momentum changing collisions with electrons and ions are considered.

Date:
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Location:
CP179
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Word Games with Friends Night- Sigma Tau Delta

Do you dominate at Scrabble? Do you know how to perfectly fit nouns and adjectives together in Apples to Apples to form hilarious pairs? Do you have a secret passion for Bananagrams? 
 
If you do (and even if you don't), you are invited to Sigma Tau Delta's Word Games with Friends Night this Saturday (3/8/14) from 6-8 PM in the Cats Den! Bring your favorite word games to play with others while enjoying some snacks and drinks.
 
See the attached flyer for more information--we hope to see you there!
Date:
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Location:
Cats Den

The Road to Observationally Constraining Pre-Main Sequence Evolutionary Models

Pre-Main Sequence (PMS) evolutionary models are an important tool for deriving the fundamental parameters of young stars. Unfortunately, there are upwards of 10 groups producing PMS models which leads to mass and age differences between models of 50-200%. The goal of this study is to provide the first constraint on the evolutionary models in the F and G spectral regime. We can achieve this constraint by obtaining high resolution spectroscopy of young stars with known ages and deriving their masses to test against the PMS models. Currently, we have performed a detailed analysis on a group of 10 stars which were proposed members of the ~125 Myr moving group AB Doradus. Before the PMS models can be tested, the stars need to be confirmed members of a group in order to identify the proper age. We characterize these 10 stars via three techniques: 1) chemical composition, 2) kinematic traceback, and 3) isochrone fitting. After this analysis, we find 8 confirmed AB Doradus members, 1 plausible member, and 1 likely non-member. We are currently extending this technique to younger groups to populate more of the HR-diagram and successfully constrain the PMS models.
 
Date:
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Location:
CP179
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