Supernovae and gamma-ray bursts are the strongest explosions in the Universe. Observations show that, rather than being symmetrical, they are driven by strong jets of energy and other asymmetrical effects. These observations demand theories and computations that challenge the biggest computers. This volume marks the transition to a fresh paradigm in the study of stellar explosions. It highlights the burgeoning era of routine supernova polarimetry and the insights into core collapse and thermonuclear explosions. With chapters by leading scientists, the book summarises the status of a fresh perspective on stellar explosions and should be a valuable resource for graduate students and research scientists.
Supernovae are among the most energetic phenomena in the Universe and - lated to almost all aspects of modern astrophysics including starburst gal- ies, cosmic ray acceleration, neutron star and black hole formation, nuc- osynthesis and ISM chemical enrichment, energy input to the ISM, cosmic distance scale determination, dark energy related cosmological acceleration, gamma-ray bursts, extra-solar system neutrino burst detection, gravity wave generation, and many more. Additionally, the past 15 years have been p- ticularly productive with many new results and new understanding due in particular to the closest SN in 400 years in SN 1987A in the Large M- ellanic Cloud, and the unusually bright and close SN 1993J and SN 1994I in the nearby galaxies M81 and M51, respectively. In addition, the disc- ery of the ?-ray burst GRB 980425 and its related supernova SN 1998bw, and the con?rmation of GRB 030329/SN 2003dh, tied the study of SNe and GRBs inextricably together. With the many developments since the last - jor supernova meeting in La Serena, Chile in 1997, we felt that it was an appropriate time to bring together experts and students interested in the subject for a meeting where SN and GRB properties and interrelationships could be discussed. The tenth anniversary of SN 1993J provided such an - portunity and, appropriately, the meeting was held in Spain where SN 1993J was discovered on the early morning of 28 March 1993 by a Spanish amateur astronomer, Francisco Garc ́ ?a.
During the past several years, research teams around the world have developed astrophysics-relevant utilizing high energy-density facilities such as intense lasers and z-pinches. Research is underway in many areas, such as compressible hydrodynamic mixing, strong shock phenomena, radiation flow, radiative shocks and jets, complex opacities, equations of stat, and relativistic plasmas. Beyond this current research and the papers it is producing, plans are being made for the application, to astrophysics-relevant research, of the 2 MJ National Ignition Facility (NIF) laser at Lawrence Livermore National Laboratory; the 600 kj Ligne d'Intégration Laser (LIL) and the 2 MJ Laser Mégajoule (LMJ) in Bordeaux, France; petawatt-range lasers now under construction around the world; and current and future Z pinches. The goal of this conference and these proceedings is to continue focusing attention on this emerging research area. The conference brought together different scientists interested in this emerging new field, with topics covering: - Hydrodynamic instabilities in astrophysics, - Supernovae and supernova remnant evolution, - Astrophysical shocks, blast waves, and jets, - Stellar opacities, - Radiation and thermal transport, - Dense plasma atomic physics and EOS, - X-ray photoionized plasmas, - Ultrastrong magnetic field generation.
Recent observations have demonstrated that supernovae and gamma ray bursts are driven by strong jets of energy and other asymmetrical effects that reveal unknown physical properties. This volume highlights the burgeoning era of routine supernova polarimetry and the new insights into core collapse and thermonuclear explosions. Chapters by leading scientists summarize the status of a rapidly developing perspective on stellar explosions in a valuable resource for graduate students and research scientists.
These peer-reviewed NIC XV conference proceedings present the latest major advances in nuclear physics, astrophysics, astronomy, cosmochemistry and neutrino physics, which provide the necessary framework for a microscopic understanding of astrophysical processes. The book also discusses future directions and perspectives in the various fields of nuclear astrophysics research. In addition, it also includes a limited number of section of more general interest on double beta decay and dark matter.
Targeting advanced students of astronomy and physics, as well as astronomers and physicists contemplating research on supernovae or related fields, David Branch and J. Craig Wheeler offer a modern account of the nature, causes and consequences of supernovae, as well as of issues that remain to be resolved. Owing especially to (1) the appearance of supernova 1987A in the nearby Large Magellanic Cloud, (2) the spectacularly successful use of supernovae as distance indicators for cosmology, (3) the association of some supernovae with the enigmatic cosmic gamma-ray bursts, and (4) the discovery of a class of superluminous supernovae, the pace of supernova research has been increasing sharply. This monograph serves as a broad survey of modern supernova research and a guide to the current literature. The book’s emphasis is on the explosive phases of supernovae. Part 1 is devoted to a survey of the kinds of observations that inform us about supernovae, some basic interpretations of such data, and an overview of the evolution of stars that brings them to an explosive endpoint. Part 2 goes into more detail on core-collapse and superluminous events: which kinds of stars produce them, and how do they do it? Part 3 is concerned with the stellar progenitors and explosion mechanisms of thermonuclear (Type Ia) supernovae. Part 4 is about consequences of supernovae and some applications to astrophysics and cosmology. References are provided in sufficient number to help the reader enter the literature.
On July 23, 1999, the Chandra X-Ray Observatory, the most powerful X-ray telescope ever built, was launched aboard the space shuttle Columbia. Since then, Chandra has given us a view of the universe that is largely hidden from telescopes sensitive only to visible light. In Chandra's Cosmos, the Smithsonian Astrophysical Observatory's Chandra science spokesperson Wallace H. Tucker uses a series of short, connected stories to describe the telescope's exploration of the hot, high-energy face of the universe. The book is organized in three parts: "The Big," covering the cosmic web, dark energy, dark matter, and massive clusters of galaxies; "The Bad," exploring neutron stars, stellar black holes, and supermassive black holes; and "The Beautiful," discussing stars, exoplanets, and life. Chandra has imaged the spectacular, glowing remains of exploded stars and taken spectra showing the dispersal of their elements. Chandra has observed the region around the supermassive black hole in the center of our Milky Way and traced the separation of dark matter from normal matter in the collision of galaxies, contributing to both dark matter and dark energy studies. Tucker explores the implications of these observations in an entertaining, informative narrative aimed at space buffs and general readers alike.
Few individuals have had as great an impact on the law--both its practice and its history--as A. Leon Higginbotham, Jr. A winner of the Presidential Medal of Freedom, the nation's highest civilian honor, he has distinguished himself over the decades both as a professor at Yale, the University of Pennsylvania, and Harvard, and as a judge on the United States Court of Appeals. But Judge Higginbotham is perhaps best known as an authority on racism in America: not the least important achievement of his long career has been In the Matter of Color, the first volume in a monumental history of race and the American legal process. Published in 1978, this brilliant book has been hailed as the definitive account of racism, slavery, and the law in colonial America. Now, after twenty years, comes the long-awaited sequel. In Shades of Freedom, Higginbotham provides a magisterial account of the interaction between the law and racial oppression in America from colonial times to the present, demonstrating how the one agent that should have guaranteed equal treatment before the law--the judicial system--instead played a dominant role in enforcing the inferior position of blacks. The issue of racial inferiority is central to this volume, as Higginbotham documents how early white perceptions of black inferiority slowly became codified into law. Perhaps the most powerful and insightful writing centers on a pair of famous Supreme Court cases, which Higginbotham uses to portray race relations at two vital moments in our history. The Dred Scott decision of 1857 declared that a slave who had escaped to free territory must be returned to his slave owner. Chief Justice Roger Taney, in his notorious opinion for the majority, stated that blacks were "so inferior that they had no right which the white man was bound to respect." For Higginbotham, Taney's decision reflects the extreme state that race relations had reached just before the Civil War. And after the War and Reconstruction, Higginbotham reveals, the Courts showed a pervasive reluctance (if not hostility) toward the goal of full and equal justice for African Americans, and this was particularly true of the Supreme Court. And in the Plessy v. Ferguson decision, which Higginbotham terms "one of the most catastrophic racial decisions ever rendered," the Court held that full equality--in schooling or housing, for instance--was unnecessary as long as there were "separate but equal" facilities. Higginbotham also documents the eloquent voices that opposed the openly racist workings of the judicial system, from Reconstruction Congressman John R. Lynch to Supreme Court Justice John Marshall Harlan to W. E. B. Du Bois, and he shows that, ironically, it was the conservative Supreme Court of the 1930s that began the attack on school segregation, and overturned the convictions of African Americans in the famous Scottsboro case. But today racial bias still dominates the nation, Higginbotham concludes, as he shows how in six recent court cases the public perception of black inferiority continues to persist. In Shades of Freedom, a noted scholar and celebrated jurist offers a work of magnificent scope, insight, and passion. Ranging from the earliest colonial times to the present, it is a superb work of history--and a mirror to the American soul.
LIGHT, the primordial, eternal, pure, almighty energy, is the brightest as well as darkest riddle that has been puzzling to all earthlings for millennia. Whoever truly knows light has already cracked the greatest mystery of the cosmos. Surprisingly! This riddle has been actually cracked independently by three thinkers of different ages. Heraclitus, the Hellenic thinker 2500 years ago, is the first cracker of the riddle with his doctrines that things are constantly changing (universal flux), that opposites coincide, and that fire is the source and nature of all things—We just decode his Fire into LIGHT. 2400 years later, there comes the second cracker Nikola Tesla, the modern Heraclitus, who, in 1899, explicitly declares that Everything is LIGHT. Matter is created from the original and eternal energy that we know as LIGHT. Solatle Lu is the third cracker, the first narrator of the riddle. He explicitly declares, in 2019 in his An Outline of Force Cosmology, that All particles are derived from photons and live forever, substantially honors LIGHT as the Creator of all things, hence elevates the common idea of the three to the Highest Knowledge of 21st century, the Primary Cause, the First Principle. This event marks a great leap in the continuous rational movement of mankind, a new start.
