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Gammie C: Astrophyscial Fluid Mechanics

Astrophyscial Fluid Mechanics

Foundations of Biochemistry and Biophysics

The Compressible Fluid Physics of the Human Respiratory System

This book highlights the basic concepts and equations for bioengineering flow processes. Physical concepts and meanings are emphasized while rigorous derivations are simplified, making it easier for self learning on some biological and medical flow processes. The well known Bernoulli equation in hydraulics is extended for pulsating flows, peristaltic flows and cardiac pumping. The dimensional analysis, model law and dimensionless equations can be related to computational models and experimental observations. The velocity vector imaging stored in echocardiograms can be used to analyze the pumping characteristics of the ventricular contraction. New topics included oxygen transport in membrane oxygenator and micro mixing of blood flow in capillary channels.

Bioengineering Fluid Mechanics

Advanced Series In Astrophysics And Cosmology

The current cosmological model relies on inflationary theories, which incorporate baryosynthesis, dark matter, and dark energy. Supported by precise cosmological data, it necessitates physics beyond the standard models of fundamental forces, including gravity. This connection between macroscopic gravity on large scales and quantum gravity on the smallest scales is where quantum gravity's nature becomes evident. Quantum gravity effects alter our classical understanding of gravitational phenomena as described by General Relativity, leading to observable deviations from the conventional cosmological model. The field of cosmoparticle physics explores the interplay between the micro and macro worlds, offering insights into the development of quantum gravity and its cosmological implications. In this work we hence wanted to cover all the amazing developments which have happened on the interface of quantum gravity theories and cosmology, making it a valuable resource for any researcher interested in exploring these fields in depth or starting research in them.

Quantum Gravitational Imprints On Cosmology

Handbook of Radiation Belts: Physics Throughout the Solar System provides a comprehensive overview of radiation belt processes throughout the solar system in a single book, compiling all information relevant to radiation belts in one place. It features an overview of radiation belts of each applicable planet in the Solar System to assist researchers working on individual radiation belt physics, particularly of comparative or multiplanetary scope. The handbook goes on to offer a detailed guide to basics such as measurement and particle motion to more advanced topics such as radial transport and associated acceleration. It provides the respective theory behind the physics as well as detailed derivations, with worked examples and case studies, allowing readers to follow the implementation of the theory behind the science to apply in their research. The Handbook of Radiation Belts covers all relevant topics to radiation belts in our Solar System in one complete source, offering researchers, academics and students in space physics a complete guide to the topic for those performing fundamental research and teaching, as well as professionals planning and operating space missions or assets.

Physics Throughout the Solar System

Handbook of Radiation Belts

Close your eyes and imagine the last moments of a massive star, large as the Solar System. As the mass of its core approaches a fatidic value, the enormous fabric collapses. The star plasma streams like a monstrous wave inward towards the center of the star. In a fraction of a second the core of the star becomes as dense as an atomic nucleus. And then a mighty outward shock wave forms, disrupting the whole structure, the star becoming almost as bright as the whole galaxy. This explosion is a supernova!Chinese observers studied with care these events since ancient times; the observation of these explosions by Tycho Brahe and Kepler was crucial for the adoption of the Copernican system. Do you know that each drop of your blood contains iron atoms produced in these cosmic cataclysms? We are literally star dust, disseminated in the galactic medium by supernovae.This book guides the reader in the discovery of these rare events, the most spectacular that the Universe can offer. Present models reproduce the explosion only with difficulty, as if some details were wrong, or a whole aspect of physics was missing from the equations. Different aspects of these events are illustrated, as well as their historical and scientific importance and their crucial role in the evolution of the galaxy and the living organisms.

Supernova: The Last Flash Of The Disappearing Star

Astronomers' Universe

One of the most stunning features of the night sky, and Earth's home, the Mily Way is fertile ground for exploring the mysteries of the universe. This book will provide an overview of how astronomers have attempted to uncover our Galaxy’s past, and how current models of its structure may account for some of the most recent observations.&nbsp;Indeed, the&nbsp;distribution of chemical elements in our Galaxy serves as a ‘fossil record’ of its evolutionary history and is a powerful tool for studying the formation and evolution, not only of the Milky Way, but also of other galaxies.In their journey through the history of our Galaxy the authors answer many fascinating and intriguing questions, such as: what can the Milky Way tell us about the Big Bang? What were the very first stars like? Are we able to find any of these first stars, still shining today, but born at a time when no metals had been formed and the gas and the Galaxy consisted of only hydrogen and helium? How did the main biogenic elements form and how are they distributed throughout the Galaxy? Are there regions of our Galaxy where Earth-like planets such as ours might more easily form?The text is addressed to the curious or interested reader and is intended to unveil to a general popular science audience some of the topics about the structure and evolution of our Galaxy which are now the subject of hot debate amongst professional astronomers around the world.

A Natural History of the Milky Way

Thermal and Flow Measurements

Fundamentals and Applications

Computational Fluid Dynamics in Chemical Engineering

An expert and contemporary presentation of computational analysis and design tools for professionals studying or applying the principles of aerodynamics In Aerodynamics: A Computational Introduction, a distinguished aerospace engineer and researcher Krzysztof Fidkowski delivers an up-to-date and authoritative reference text covering the essentials of aerodynamics. The book covers key topics, including basic fluid dynamics, potential flow, airfoil theory, boundary layers, wing theory, and compressible flow. Fidkowski takes a computation-first approach to the subject matter, presenting aerodynamics in a way that is compatible with the way the subject is handled in contemporary businesses and research labs. Aerodynamics offers numerical demonstrations, codes, and theory comparisons that make important derivations and conclusions easier to understand and apply. Readers will also find: <ul> <li>A self-contained introduction to the thermodynamics, mathematics, and numerical methods central to the subject of aerodynamics</li> <li>Comprehensive explorations of kinematics, dynamics, and potential flow</li> <li>Practical discussions of panel methods and airfoil theory, including design tools</li> <li>Numerical and analytical tools for boundary-layer analysis</li> <li>Complete treatment of finite-wing theory, including horseshoe vortices, lifting-line theory, and the vortex-lattice method.</li> </ul> Perfect for engineering students who want to learn how to apply basic numerical methods to large-scale aerodynamics problems, Aerodynamics: A Computational Introduction will also benefit professionals who wish to better understand aerodynamics and computational fluid dynamics.

A Computational Introduction

Aerodynamics

Advanced Mission Scenarios of the Three-Body Problem

Dynamics and Astrophysics of Galaxies

Series in Astronomy and Astrophysics

This book focuses on observing magnetic fields in order to understand their role in star and planet formation. Polarimetry observers will gain a better understanding of all the various techniques, especially those beyond what they themselves use. Theorists will gain an understanding of exactly what one can infer from the observational data, including both the limitations and the power of the different techniques. Readers not actively involved in star formation research will gain a clear understanding of the possible roles played by magnetic fields and the current state of the observational field. The book provides a foundation for future research in this field.

This book focuses on observing magnetic fields in order to understand their role in star and planet formation. Polarimetry observers will gain a better understanding of all the various techniques, especially those beyond what they themselves use. Theorists will gain an understanding of exactly what one can infer from the observational data, including both the limitations and the power of the different techniques. Readers not actively involved in star formation research will gain a clear understanding of the possible roles played by magnetic fields and the current state of the observational field. The book provides a foundation for future research in this field.

Observations and Implications

Magnetic Fields in Regions of Star Formation

Astrophyscial Fluid Mechanics

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Schlagworte

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