Автор: Nanda Rea; Diego F. Torres Название: High-Energy Emission from Pulsars and their Systems ISBN: 3642267076 ISBN-13(EAN): 9783642267079 Издательство: Springer Рейтинг: Цена: 49631.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание:
Radio Pulsar Phenomenology.- Radio pulsar populations.- Pulsar Results with the Fermi Large Area Telescope.- Fermi view of the EGRET pulsars.- "Garden-variety" Gamma-ray Pulsars J0248+6021& J2240+5832.- Extension studies of galactic sources with Fermi.- Advances in understanding double features in radio pulsar profiles.- Emission from the Polar Cap and Slot Gap.- Gamma-ray emission and pair creation of outer gap.- What Pulsar High-Energy Emission Model Survives?.- Current Models of Pulsar Magnetospheres.- Modeling of y-ray Pulsar Light Curves from Force-Free Magnetosphere.- A Tale of Two Current Sheets.- The high-energy emission from the pulsar striped wind.- Gamma-rays from millisecond pulsars in Globular Clusters.- Modelling the Growing Population of y-ray Millisecond Pulsars.- A Joint Radio Gamma-ray Variability Study of the Crab Pulsar.- AGILE observations of PSR B1509-58.- Understanding the fundamental parameters of millisecond pulsars.- Pulsars as gravitational wave detectors.- Magnetar outbursts: an observational review.- Wide-band X-ray Studies of Magentars with Suzaku.- Bursts and Flares from Highly Magnetic Pulsars.- Activated Magnetospheres of Magnetars.- Suzaku Detection of Hard X-ray Emission in SGR 0501+4516 Short Burst Spectrum.- The magnetar emission in the IR band: the role of magnetospheric currents.- Double features in mean pulsar profiles and the nature of their radio emission.- Can the magnetic field of long-period X-ray pulsars be supercritical ?.- X-ray emission from isolated neutron stars.- X-ray thermal radiation from hot polar cap in pulsars.- Radio polarization of RRAT J1819-1458.- Multiwavelength Observations of Pulsar Wind Nebulae.- Multi-wavelength Observations of Composite Supernova Remnants.- Fermi-LAT Results on Pulsar Wind Nebulae after 1.5 year of Observations.- Pulsar Wind Nebulae: The GeV to TeV Connection.- Extended hard X-ray emission from Vela X.- Cherenkov Telescopes Results on Pulsar Wind Nebulae and Pulsars.- Lepton Acceleration in Pulsar Wind Nebulae.- MHD models of Pulsar Wind Nebulae.- TeV Gamma Ray Survey on the Direction of Fermi-LAT Pulsars with the Tibet Air Shower Array.- Fermi results on y-ray binaries.- Cherenkov Telescope results on gamma-ray binaries.- y-ray binaries as non-accreting pulsar systems.- Relativistic motion and beamed radiation in gamma-ray binaries.- A leptonic One-Zone model of the X-Ray/VHE correlated emission in LS I +61 303.- New Optical Results on y-ray Binaries.- The International X-ray Observatory and other X-ray missions, expectations for pulsar physics.- X-ray Polarimeters.- New results on high energy cosmic ray electrons observed with Fermi LAT.- Positrons from pulsar winds.
Автор: John Antoniadis Название: Multi-Wavelength Studies of Pulsars and Their Companions ISBN: 3319098969 ISBN-13(EAN): 9783319098968 Издательство: Springer Рейтинг: Цена: 15672.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: This impressive work was awarded the Otto-Hahn Medal of the Max-Planck Society and the Best PhD in Gravity, Particle and Atomic physics award by the German Physics Society (DPG).
Автор: E.P. van den Heuvel; S.A. Rappaport Название: X-Ray Binaries and Recycled Pulsars ISBN: 9401051984 ISBN-13(EAN): 9789401051989 Издательство: Springer Рейтинг: Цена: 12157.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: Proceedings of the NATO Advanced Research Workshop on X-Ray Binaries and the Formation of Binary and Millisecond Radio Pulsars, Santa Barbara, CA, U.S.A., Januari 21-25, 1991
Описание: Neutron stars, the ultra-dense remnants of exploded stellar giants, are among the most fascinating objects in the cosmos. Katia Moskvitch introduces readers to their astonishing qualities and follows the scientists who are discovering what neutron stars can tell us about the mysteries of dark matter, black holes, and general relativity.
This book reports on the extraordinary observation of TeV gamma rays from the Crab Pulsar, the most energetic light ever detected from this type of object. It presents detailed information on the painstaking analysis of the unprecedentedly large dataset from the MAGIC telescopes, and comprehensively discusses the implications of pulsed TeV gamma rays for state-of-the-art pulsar emission models. Using these results, the book subsequently explores new testing methodologies for Lorentz Invariance Violation, in terms of a wavelength-dependent speed of light. The book also covers an updated search for Very-High-Energy (VHE), >100 GeV, emissions from millisecond pulsars using the Large Area Telescope on board the Fermi satellite, as well as a study on the promising Pulsar Wind Nebula candidate PSR J0631.
The observation of VHE gamma rays is essential to studying the non-thermal sources of radiation in our Universe. Rotating neutron stars, also known as pulsars, are an extreme source class known to emit VHE gamma rays. However, to date only two pulsars have been detected with emissions above 100 GeV, and our understanding of their emission mechanism is still lacking.
Автор: Bhattacharyya Sudip, Papitto Alessandro, Bhattacharya Dipankar Название: Millisecond Pulsars ISBN: 3030851974 ISBN-13(EAN): 9783030851972 Издательство: Springer Рейтинг: Цена: 19564.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: This book includes nine chapters written by internationally recognized experts, covering all aspects of millisecond pulsars in one concise and cohesive volume. These aspects include pulsations powered by stellar spin, accretion and thermonuclear burning of accreted matter, their physics and utility, stellar evolution and the extreme physics of super-dense stellar cores. The book includes substantial background material as well as recent theoretical and multi-wavelength observational results. The volume will thus be useful for professional astronomers and graduate students alike. What is the behavior of the strong nuclear interaction, and what are the matter constituents at ultrahigh densities in neutron star cores? How do old neutron stars in binaries evolve? How does their magnetosphere interact with the surrounding plasma to accelerate particles and emit radiation observed at all wavelengths? These are just a few of the questions that millisecond pulsars are helping us answer and will settle in the near future with the next generation of instruments. Such quickly rotating, highly magnetized neutron stars are remarkable natural laboratories that allow us to investigate the fundamental constituents of matter and their interactions under extreme conditions that cannot be reproduced in terrestrial laboratories.
Автор: John Antoniadis Название: Multi-Wavelength Studies of Pulsars and Their Companions ISBN: 3319384953 ISBN-13(EAN): 9783319384955 Издательство: Springer Рейтинг: Цена: 13059.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: This impressive work was awarded the Otto-Hahn Medal of the Max-Planck Society and the Best PhD in Gravity, Particle and Atomic physics award by the German Physics Society (DPG).
Описание: This book reports on the extraordinary observation of TeV gamma rays from the Crab Pulsar, the most energetic light ever detected from this type of object.
Описание: Modern comprehensive introduction and overview of the physics of White Dwarfs, Neutron Stars and Black Holes, including all relevant observations. Contains a basic introduction to General Relativity, including the modern 3+1 split of spacetime and of Einstein`s equations.
Автор: J.E Ventura; David Pines Название: Neutron Stars: Theory and Observation ISBN: 0792313976 ISBN-13(EAN): 9780792313977 Издательство: Springer Рейтинг: Цена: 46399.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: Proceedings of the NATO Advanced Study Institute on Neutron Stars: An Interdisciplinary Field, Agia Pelagia, Crete, Greece, September 3-14, 1990
Автор: Pantelis Pnigouras Название: Saturation of the f-mode Instability in Neutron Stars ISBN: 3030074749 ISBN-13(EAN): 9783030074746 Издательство: Springer Рейтинг: Цена: 15372.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: This book presents a study of the saturation of unstable f-modes (fundamental modes) due to low-order nonlinear mode coupling. Since their theoretical prediction in 1934, neutron stars have remained among the most challenging objects in the Universe. Gravitational waves emitted by unstable neutron star oscillations can be used to obtain information about their inner structure, that is, the equation of state of dense nuclear matter. After its initial growth phase, the instability is expected to saturate due to nonlinear effects. The saturation amplitude of the unstable mode determines the detectability of the generated gravitational-wave signal, but also affects the evolution of the neutron star. The study shows that the unstable (parent) mode resonantly couples to pairs of stable (daughter) modes, which drain the parent’s energy and make it saturate via a mechanism called parametric resonance instability. Further, it calculates the saturation amplitude of the most unstable f-mode multipoles throughout their so-called instability windows.
Автор: James J Kolata Название: Neutron Stars, Black Holes, and Gravitational Waves ISBN: 1643274236 ISBN-13(EAN): 9781643274232 Издательство: Mare Nostrum (Eurospan) Рейтинг: Цена: 8593.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: Albert Einstein's General Theory of Relativity, published in 1915, made a remarkable prediction: gravitational radiation. Just like light (electromagnetic radiation), gravity could travel through space as a wave and affect any objects it encounters by alternately compressing and expanding them. However, there was a problem. The force of gravity is around a trillion, trillion, trillion times weaker than electromagnetism so the calculated compressions and expansions were incredibly small, even for gravity waves resulting from a catastrophic astrophysical event such as a supernova explosion in our own galaxy. Discouraged by this result, physicists and astronomers didn't even try to detect these tiny, tiny effects for over 50 years. Then, in the late 1960s and early 1970s, two events occurred which started the hunt for gravity waves in earnest. The first was a report of direct detection of gravity waves thousands of times stronger than even the most optimistic calculation. Though ultimately proved wrong, this result started scientists thinking about what instrumentation might be necessary to detect these waves. The second was an actual, though indirect, detection of gravitational radiation due to the effects it had on the period of rotation of two 'neutron stars' orbiting each other. In this case, the observations were in exact accord with predictions from Einstein's theory, which confirmed that a direct search might ultimately be successful. Nevertheless, it took another 40 years of development of successively more sensitive detectors before the first real direct effects were observed in 2015, 100 years after gravitational waves were first predicted. This is the story of that hunt, and the insight it is producing into an array of topics in modern science, from the creation of the chemical elements to insights into the properties of gravity itself.
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