The Origins of American Democracy, or How the People Became Judges in Their Own Causes, The Sixty-Ninth Cleveland-Marshall Fund Lecture

The awesome power of this democratic polity, with people becoming judges in their own causes, was such that our political leaders over the past two centuries have struggled to constrain and mitigate its effects. In fact, that is what our current concern with campaign financing is all about. From the very beginning of our national history we Americans have used a variety of devices and institutions to immunize ourselves from the harmful consequences of too much democracy, too much factious promotion of private interests in the name of the people. No doubt the most important of these devices has been the judiciary, the institution most removed from the people and most resistant to the pressure of private interests. Indeed, by playing the role that Madison had wanted the legislatures to play-impartially adjudicating among contending parties and interests-the judiciary suddenly emerged out of its colonial insignificance to become the principal means of protecting minority rights and individual liberties against interest-mongering popular legislatures. Many, including Madison in his later years, eventually concluded that the judiciary was the only governmental institution in America that came close to resembling the disinterested and impartial umpires that the revolutionaries had earlier yearned for

Classical Republicanism and the American Revolution

In his Classical Republicanism and the American Revolution, Professor Wood outlines the evolution of republicanism from antiquity to the eighteenth century and notes the ensuing evolution of American politics away from even this late republicanism

Influence of selected patient variables and operative blood loss on six-month survival following liver transplantation.

A group of 118 adults who underwent primary, orthotopic transplantation of the liver over a 4-year period served as the subjects of a detailed examination of their ability to survive the first 6 months as a function of their preoperative condition. As a result, a scoring system was developed empirically in an attempt to separate very high-risk from relatively low-risk patients. The scoring method is based on the high degree of correlation between survival probability and various patient characteristics. It allows for additional scoring to account for the dramatic effect of operative blood loss on the eventual outcome. The curve that best describes the relationship between patient scores and survival probability is sigmoidal in shape. Many patients will have scores located on the curve between the inflection points. They represent a group whose relative risk is difficult to estimate but for whom operative blood loss or the occurrence of surgical complications may prove particularly telling

Trends in socioeconomic inequalities in risk of sudden infant death syndrome, other causes of infant mortality, and stillbirth in Scotland: population based study

Objectives To compare changes in inequalities in sudden infant death syndrome with other causes of infant mortality and stillbirth in Scotland, 1985-2008

Time of birth and risk of neonatal death at term: retrospective cohort study

Objective To determine the effect of time and day of birth on the risk of neonatal death at term

On the Origins of the High-Latitude H-alpha Background

The diffuse high-latitude H-alpha background is widely believed to be predominantly the result of in-situ recombination of ionized hydrogen in the warm interstellar medium of the Galaxy. Instead, we show that both a substantial fraction of the diffuse high-latitude H-alpha intensity in regions dominated by Galactic cirrus dust and much of the variance in the high-latitude H-alpha background are the result of scattering by interstellar dust of H-alpha photons originating elsewhere in the Galaxy. We provide an empirical relation, which relates the expected scattered H-alpha intensity to the IRAS 100um diffuse background intensity, applicable to about 81% of the entire sky. The assumption commonly made in reductions of CMB observations, namely that the observed all-sky map of diffuse H-alpha light is a suitable template for Galactic free-free foreground emission, is found to be in need of reexamination.Comment: 26 pages, 5 figures, Accepted for publication in Ap