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Bovy J: Dynamics and Astrophysics of
Galaxies

Dynamics and Astrophysics of Galaxies

Interdisciplinarity In The Sciences: Nonlinear Dynamics, Chaos And Complexity

Advances in Quantum Chemistry

Recent developments of molecular electronic structure theory: Volume 91

Black Holes and Our Place on Earth

Facing Infinity

How do you explore distant stars, buried water on Mars or the first moments after the Big Bang - without leaving your back garden? In The Radio Universe, award-winning astrophysicist Emma Chapman takes us on an electrifying voyage through the cosmos using one of the most powerful, yet overlooked, tools in science: the radio wave. With dazzling clarity and humour, Chapman reveals how these invisible messengers glide through space, bounce off planets, tunnel through clouds and slip past galactic dust - carrying secrets of the universe that no other kind of light can uncover. We follow a single radio wave as it escapes Earth and travels outward - ricocheting off the Moon, tunnelling through Venus's furnace-thick atmosphere, tracing ancient ice hidden in Mercury's shadows and diving deep into the swirling arms of the Milky Way. Along the way, we meet black holes that roar louder than stars, pulsars more precise than atomic clocks and galaxies lit by the very first starlight. We explore volcanic pancake planets, death-defying neutron stars, the eerie possibility of alien broadcasts - and the fragile question of our own future in the cosmos. A celebration of human ingenuity and cosmic curiosity, The Radio Universe reveals that the true frontier of space isn't 'out there' - it's humming quietly all around us, waiting to be heard.

How to Explore Outer Space Without Leaving Earth

The Radio Universe

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

Lectures On Quantum State Estimation

Astronomy and astrophysics library

This book is based in part on classroom tested lectures related to the first stars (Pop III stars), but also draws from the author's review articles of the main physical principles involved. The book will thus combine pedagogical introductory chapters with more advanced ones to survey the cutting-edge advances from the frontier of research.The formation of Pop III stars and galaxies is one of the great outstanding challenges in modern astrophysics and cosmology. The first stars are likely key drivers for early cosmic evolution and will be at the center of attention over the next decade. The best available space and ground-based telescopes like the Hubble Space Telescope probe the Universe to high redshifts and provide us with tantalizing hints; but they cannot yet directly detect the first generation of stars and the formation of the first galaxies. This is left as key science for future telescopes like the James Webb Space Telescope.The book covers the theory of first star formation, the relation between first stars and dark matter, their impact on cosmology, their observational signatures, the transition to normal star formation as well as the assembly of the first galaxies. It will prepare advanced students and researchers entering the field for interpreting observational findings and their cosmological implications.

This book is based in part on classroom tested lectures related to the first stars (Pop III stars), but also draws from the author's review articles of the main physical principles involved. The book will thus combine pedagogical introductory chapters with more advanced ones to survey the cutting-edge advances from the frontier of research.The formation of Pop III stars and galaxies is one of the great outstanding challenges in modern astrophysics and cosmology. The first stars are likely key drivers for early cosmic evolution and will be at the center of attention over the next decade. The best available space and ground-based telescopes like the Hubble Space Telescope probe the Universe to high redshifts and provide us with tantalizing hints; but they cannot yet directly detect the first generation of stars and the formation of the first galaxies. This is left as key science for future telescopes like the James Webb Space Telescope.The book covers the theoryof first star formation, the relation between first stars and dark matter, their impact on cosmology, their observational signatures, the transition to normal star formation as well as the assembly of the first galaxies. It will prepare advanced students and researchers entering the field for interpreting observational findings and their cosmological implications.

The First Stars

Life on Earth depends on the Sun -- our star. The book describes the past 100 years of research to understand and build a model of a star -- using the most creative and advanced technologies of the 20th and 21st centuries. Starting from a breakthrough in 1938 of our understanding of the nuclear fusion reactions that power the Sun and other stars, we have created explosions using the same nuclear physics that powers stars. Now, we are developing complex machines that use the same nuclear physics to reproduce the nuclear fusion reactions that power the Sun and the billions of other stars in the galaxies -- to develop electric power.Nuclear laboratories around the world have built complex machines that produce solar nuclear fusion reactions for periods of seconds. This book describes the history of the first early attempts to build fusion reactors and how man has worked for decades to build a machine based on the nuclear reactions that power the stars.It also describes laboratories carrying out the research and the building of the machines designed to start and maintain the steady solar nuclear burning of hydrogen that powers the stars. It is a fascinating read of the history and the current state of international efforts to build star power.

Star Power

This student textbook clearly explains the connections between nuclear and particle physics, giving students a comprehensive understanding of this subject area. The book is suitable for those taking courses dedicated to both particle and nuclear physics, as well as for students taking a course in either nuclear or particle physics, who need to place their studies in a broader context. The book opens with an examination of the Big Bang and the birth of nuclear and particle physics, and concludes with coverage of highly practical experiments and applications, including medical physics, environmental science, nuclear fusion and nuclear fission. Worked examples and problems are provided.

This student textbook clearly explains the connections between nuclear and particle physics, giving students a comprehensive understanding of this subject area. The book is suitable for those taking courses dedicated to both particle and nuclear physics, as well as for students taking a course in either nuclear or particle physics, who need to place their studies in a broader context. The book opens with an examination of the Big Bang and the birth of nuclear and particle physics, and concludes with coverage of highly practical experiments and applications, including medical physics, environmental science, nuclear fusion and nuclear fission. Worked examples and problems are provided.

From the Early Universe to Nuclear Energy

Nuclear and Particle Physics

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

Dynamics and Astrophysics of Galaxies

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