The Affordable Care Act raises the stakes on worker classification; what does this mean for the Voluntary Classification Settlement Program

This research considers worker classification and the many implications an employer must consider when classifying a worker as employee or independent contractor. One implication relates to healthcare benefits and healthcare taxes. As such, this research will evaluate the new healthcare taxes and implications resulting from the Affordable Care Act. Furthermore, this research will relate and explain worker classification with regards to the Voluntary Classification Settlement Program. This is a program offered by the Internal Revenue Service allowing employers to prospectively classify workers as employees with tax relief for past misclassification. The healthcare implications from the Affordable Care Act have raised the stakes on worker classification. This research will confirm whether this will provide greater incentive for employers to classify workers as employees or independent contractors. This research considers worker classification and the many implications an employer must consider when classifying a worker as employee or independent contractor. One implication relates to healthcare benefits and healthcare taxes. As such, this research will evaluate the new healthcare taxes and implications resulting from the Affordable Care Act. Furthermore, this research will relate and explain worker classification with regards to the Voluntary Classification Settlement Program. This is a program offered by the Internal Revenue Service allowing employers to prospectively classify workers as employees with tax relief for past misclassification. The healthcare implications from the Affordable Care Act have raised the stakes on worker classification. This research will confirm whether this will provide greater incentive for employers to classify workers as employees or independent contractors

Influence of Slippery Pacemaker Leads on Lead-Induced Venous Occlusion

The use of medical devices such as pacemakers and implantable cardiac defibrillators have become commonplace to treat arrhythmias. Pacing leads with electrodes are used to send electrical pulses to the heart to treat either abnormally slow heart rates, or abnormal rhythms. Lead induced vessel occlusion, which is commonly seen after placement of pacemaker or implantable cardiac defibrillators leads, may result in lead malfunction and/or superior vena cava syndrome, and makes lead extraction difficult. The association between the anatomic locations at risk for thrombosis and regions of venous stasis have been reported previously. The computational studies reveal obvious flow stasis in the proximity of the leads, due to the no-slip boundary condition imposed on the lead surface. With recent technologies capable of creating slippery surfaces that can repel complex fluids including blood, we explore computationally how local structures may be altered in the regions around the leads when the no-slip boundary condition on the lead surface is relaxed using various slip lengths. The slippery surface is modeled by a Navier slip boundary condition. Analytical studies are performed on idealized geometries, which were then used to validate numerical simulations. A patient-specific model is constructed and studied numerically to investigate the influence of the slippery surface in a more physiologically realistic environment. The findings evaluate the possibility of reducing the risk of lead-induced thrombosis and occlusion by implementing a slippery surface conditions on the leads

Small Space Stream Summary for Matroid Center

In the matroid center problem, which generalizes the k-center problem, we need to pick a set of centers that is an independent set of a matroid with rank r. We study this problem in streaming, where elements of the ground set arrive in the stream. We first show that any randomized one-pass streaming algorithm that computes a better than Delta-approximation for partition-matroid center must use Omega(r^2) bits of space, where Delta is the aspect ratio of the metric and can be arbitrarily large. This shows a quadratic separation between matroid center and k-center, for which the Doubling algorithm [Charikar et al., 1997] gives an 8-approximation using O(k)-space and one pass. To complement this, we give a one-pass algorithm for matroid center that stores at most O(r^2 log(1/epsilon)/epsilon) points (viz., stream summary) among which a (7+epsilon)-approximate solution exists, which can be found by brute force, or a (17+epsilon)-approximation can be found with an efficient algorithm. If we are allowed a second pass, we can compute a (3+epsilon)-approximation efficiently. We also consider the problem of matroid center with z outliers and give a one-pass algorithm that outputs a set of O((r^2+rz)log(1/epsilon)/epsilon) points that contains a (15+epsilon)-approximate solution. Our techniques extend to knapsack center and knapsack center with z outliers in a straightforward way, and we get algorithms that use space linear in the size of a largest feasible set (as opposed to quadratic space for matroid center)

A deep UVBRI CCD photometric study of open clusters Tr 1 and Be 11

We present deep $UBVRI$ CCD photometry for the young open star clusters Tr 1 and Be 11. The CCD data for Be 11 is obtained for the first time. The sample consists of $\sim$ 1500 stars reaching down to $V$ $\sim$ 21 mag. Analysis of the radial distribution of stellar surface density indicates that radius values for Tr 1 and Be 11 are 2.3 and 1.5 pc respectively. The interstellar extinction across the face of the imaged clusters region seems to be non-uniform with a mean value of $E(B-V)$ = 0.60$\pm$0.05 and 0.95$\pm$0.05 mag for Tr 1 and Be 11 respectively. A random positional variation of $E(B-V)$ is present in both the clusters. In the cluster Be 11, the reason of random positional variation may be apparent association of the HII region (S 213). The 2MASS $JHK$ data in combination with the optical data in the cluster Be 11 yields $E(J-K)$ = 0.40$\pm$0.20 mag and $E(V-K)$ = 2.20$\pm$0.20 mag. Colour excess diagrams indicate a normal interstellar extinction law in the direction of cluster Be 11. The distances of Tr 1 and Be 11 are estimated as 2.6$\pm$0.10 and 2.2$\pm$0.10 Kpc respectively, while the theoretical stellar evolutionary isochrones fitted to the bright cluster members indicate that the cluster Tr 1 and Be 11 are 40$\pm$10 and 110$\pm$10 Myr old. The mass functions corrected for both field star contamination and data incompleteness are derived for both the clusters. The slopes $1.50\pm0.40$ and $1.22\pm0.24$ for Tr 1 and Be 11 respectively are in agreement with the Salpeter's value. Observed mass segregations in both clusters may be due to the result of dynamical evolutions or imprint of star formation processes or both.Comment: 15 pages, 13 figures. Accepted for publication in MNRA