The United Student-Athletes of America: Should College Athletes Organize in Order to Protect Their Rights and Address the Ills of Intercollgiate Athletics?

This note will focus on the legal feasibility and practicality of forming a student-athlete players association or union. It assumes that a strike is a possible avenue the CAC may take in the future. Unlike the professional sports unions, the make-up of athletes on college campuses is in constant flux. This will obviously make it harder to initiate a strike. Part I of the note will concentrate on the realities of major college sports and the athletes that play them. This background will establish why student-athletes may want to form a players association. Part II will analyze the NCAA governing structure and how a players association may fit among this myriad of rules. Part III will analyze labor law and how it relates to the formation of a student-athlete players association. Part IV will compare the famed Knight Commission with the CAC and decide which one is better suited to lead an intercollegiate athletic reform movement. Finally, the proper role of a student-athlete association will be suggested

The Future of eDiscovery in Tennessee

This Article begins by outlining changes in the modern digital world through an examination of essential laws of computing unfamiliar to most lawyers but crucial to an understanding of the changing landscape of technology and its projected impact on modern society. Part II then applies these principles to the practice of law in the context of electronic discovery, pointing to the challenges posed under the current Rules of Civil Procedure, an ever-increasing overabundance of discoverable data, and the inadequacy of existing technology and processes possessed by the typical lawyer to deal with these challenges. Finally, Part III of this Article will examine and advocate for the adoption of the proposed changes to the Federal Rules of Civil Procedure, as well as adoption of similar provisions in Tennessee, and ultimately offer suggestions to reform eDiscovery through process improvement, collaboration, and technology implementation

Mechanical behavior and failure phenomenon of an in situ-toughened silicon nitride

The Weibull modulus, fracture toughness and crack growth resistance of an in-situ toughened, silicon nitride material used to manufacture a turbine combustor were determined from room temperature to 1371 C. The material exhibited an elongated grain structure that resulted in improved fracture toughness, nonlinear crack growth resistance, and good elevated temperature strength. However, low temperature strength was limited by grains of excessive length (30 to 100 microns). These excessively long grains were surrounded by regions rich in sintering additives

Fast frequency response from offshore multi-terminal VSC-HVDC schemes

This paper analyses the frequency support characteristics of multi-terminal VSC-HVDC (MTDC) schemes using the energy transferred from wind turbine rotating mass and other AC systems. An alternative coordinated control (ACC) scheme, which gives priority to a frequency versus active power droop fitted to onshore VSCs is proposed to: (i) transfer wind turbine recovery power to undisturbed AC grids and (ii) allow correct control operation of MTDC systems during multiple power imbalances on different AC grids. The fast frequency response capability of MTDC systems equipped with the proposed ACC scheme is compared against a coordinated control (CC) scheme, which uses a frequency versus DC voltage droop. The frequency control schemes are demonstrated on an experimental test rig which represents a 3-terminal HVDC system. Also, the MTDC frequency support capability when wind farms do not provide extra power is tested using a 4-terminal HVDC system

Bimodal Phase Diagram of the Superfluid Density in LaAlO3/SrTiO3 Revealed by an Interfacial Waveguide Resonator

We explore the superconducting phase diagram of the two-dimensional electron system at the LaAlO3/SrTiO3 interface by monitoring the frequencies of the cavity modes of a coplanar waveguide resonator fabricated in the interface itself. We determine the phase diagram of the superconducting transition as a function of temperature and electrostatic gating, finding that both the superfluid density and the transition temperature follow a dome shape, but that the two are not monotonically related. The ground state of this 2DES is interpreted as a Josephson junction array, where a transition from long- to short-range order occurs as a function of the electronic doping. The synergy between correlated oxides and superconducting circuits is revealed to be a promising route to investigate these exotic compounds, complementary to standard magneto-transport measurements.Comment: 5 pages, 4 figures and 10 pages of supplementary materia

Tracking Salmonella-Specific CD4 T Cells In Vivo Reveals a Local Mucosal Response to a Disseminated Infection

AbstractA novel adoptive transfer system was used to track the fate of naive Salmonella-specific CD4 T cells in vivo. These cells showed signs of activation in the Peyer's patches as early as 3 hr after oral infection. The activated CD4 T cells then produced IL-2 and proliferated in the T cell areas of these tissues before migrating into the B cell-rich follicles. In contrast, Salmonella-specific CD4 T cells were not activated in the spleen and very few of these cells migrated to the liver, despite the presence of bacteria in both organs. These results show that the T cell response to pathogenic Salmonella infection is localized to the gut-associated lymphoid tissue and does not extend efficiently to the major sites of late infection

Dense, Parsec-Scale Clumps near the Great Annihilator

We report on Combined Array for Research in Millimeter-Wave Astronomy (CARMA) and James Clerk Maxwell Telescope (JCMT) observations toward the Einstein source 1E 1740.7-2942, a LMXB commonly known as the "Great Annihilator." The Great Annihilator is known to be near a small, bright molecular cloud on the sky in a region largely devoid of emission in 12-CO surveys of the Galactic Center. The region is of interest because it is interior to the dust lanes which may be the shock zones where atomic gas from HI nuclear disk is converted into molecular gas. We find that the region is populated with a number of dense (n ~ 10^5 cm^-3) regions of excited gas with small filling factors, and estimate that up to 1-3 x 10^5 solar masses of gas can be seen in our maps. The detection suggests that a significant amount of mass is transported from the shock zones to the GC star-forming regions in the form of small, dense bundles.Comment: 26 pages, 7 figures, accepted for publication by the Astrophysical Journal, abstract abridge