Relativity: The Special and General Theory (Illustrated Edition)

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The Higgs Boson

As the old adage goes, where there’s smoke, there’s fire. Where there is effect, there must be cause. The planet Neptune was found in 1846 because the mathematics of Newton's laws, when applied to the orbit of Uranus, said some massive body had to be there. Astronomers eventually found it, using the best telescopes available to peer into the sky. This same logic is applied to the search for the Higgs boson. One consequence of the prevailing theory of physics, called the Standard Model, is that there has to be some field that gives particles their particular masses. With that there has to be a corresponding particle, made by creating waves in the field, and this is the Higgs boson, the so-called God particle. This book chronicles the ongoing search – and demonstrates the power of a good theory. Based on the Standard Model, physicists believed something had to be there, but it wasn't until the Large Hadron Collider was built that anyone could see evidence of the Higgs – and finally in July 2012, they did. A Higgs-like particle was found near the energies scientists expected to find it. Now, armed with better evidence and better questions, the scientific process continues. This book gathers the best reporting and analysis from Scientific American to explain that process – the theories, the search, the ongoing questions. In essence, everything you need to know to separate Higgs from hype.

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$10.69

Why Does E=mc2?: (And Why Should We Care?)

By: Brian Cox, Jeff Forshaw

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Why Does E=mc2?: (And Why Should We Care?)

By: Brian Cox, Jeff Forshaw

The most accessible, entertaining, and enlightening explanation of the best-known physics equation in the world, as rendered by two of today’s leading scientists.

Professor Brian Cox and Professor Jeff Forshaw go on a journey to the frontier of 21st century science to consider the real meaning behind the iconic sequence of symbols that make up Einstein’s most famous equation, E=mc2. Breaking down the symbols themselves, they pose a series of questions: What is energy? What is mass? What has the speed of light got to do with energy and mass? In answering these questions, they take us to the site of one of the largest scientific experiments ever conducted. Lying beneath the city of Geneva, straddling the Franco-Swiss boarder, is a 27 km particle accelerator, known as the Large Hadron Collider. Using this gigantic machine—which can recreate conditions in the early Universe fractions of a second after the Big Bang—Cox and Forshaw will describe the current theory behind the origin of mass.

Alongside questions of energy and mass, they will consider the third, and perhaps, most intriguing element of the equation: 'c' - or the speed of light. Why is it that the speed of light is the exchange rate? Answering this question is at the heart of the investigation as the authors demonstrate how, in order to truly understand why E=mc2, we first must understand why we must move forward in time and not backwards and how objects in our 3-dimensional world actually move in 4-dimensional space-time. In other words, how the very fabric of our world is constructed. A collaboration between two of the youngest professors in the UK, Why Does E=mc2? promises to be one of the most exciting and accessible explanations of the theory of relativity in recent years.

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$3.99

The History of Physics from 2000BCE to 1945

By: Sheldon Cohen

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The History of Physics from 2000BCE to 1945

By: Sheldon Cohen

Physics is the science that deals with the properties and interrelationship of matter and energy. It studies mechanics, heat, light, sound, electricity, magnetism, radiation, and atomic structure. This tale stretches from 2000 BCE to 1945 and introduces the reader to the brilliant men and women from Thales of Miletos to Albert Einstein who working alone or collaboratively made it all possible.

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Does the Inertia of a Body Depend on its Energy Content? (Illustrated Edition)

By: Albert Einstein

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Does the Inertia of a Body Depend on its Energy Content? (Illustrated Edition)

By: Albert Einstein

Albert Einstein (1879-1955) needs no formal introduction, as he is known around the world as one of historys most brilliant geniuses and one of its most influential scientists. Einstein is often regarded as the father of modern physics and received the 1921 Nobel Prize in Physics "for his services to theoretical physics, and especially for his discovery of the law of the photoelectric effect". Einstein published more than 300 scientific papers along with over 150 non-scientific works. His great intelligence and originality have made the word "Einstein" synonymous with genius. Einsteins greatest and most famous theory is the theory of relativity, which fundamentally changed the understanding of physics and astronomy during the 20th century. When first published, relativity superseded a 200-year-old theory of mechanics put forth by Isaac Newton. The theory of relativity overturned the concept of motion from Newton's day, into all motion is relative. Time was no longer uniform and absolute. Therefore, no longer could physics be understood as space by itself, and time by itself. Instead, an added dimension had to be taken into account with curved spacetime. Time now depended on velocity, and contraction became a fundamental consequence at appropriate speeds. In the field of physics, relativity catalyzed and added an essential depth of knowledge to the science of elementary particles and their fundamental interactions, along with ushering in the nuclear age. With relativity, cosmology and astrophysics predicted extraordinary astronomical phenomena such as neutron stars, black holes, and gravitational waves. This edition of Einsteins short essay Does the Inertia of a Body Depend on its Energy Content is specially formatted with a Table of Contents and is illustrated with pictures of the great thinker.

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The New Biography of the Universe

By: Matthias Matting

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The New Biography of the Universe

By: Matthias Matting

May I introduce: the universe. Born 13.75 billion years ago. Constantly growing. Nearly empty. Electrically neutral. Poor in antimatter. Populated by 100 billion galaxies, including 130 sextillion stars with approximately just as many planets.
Consisting of only 4 percent known forms of matter. The other 96 percent is made up of 23 percent dark matter and 73 percent dark energy. The home of black holes, giant stars, pulsars, quasars, galaxy clusters, and nebulas - as well as lifeforms such as humans.

Where did the universe come from? What were the conditions at its birth? What amazing processes have been taking place since then? When and how will it die? What science knows about these things has changed dramatically in recent years. Let yourself be taken away into a world that goes beyond everything imaginable – the universe in which you live.

With 31 images. Buyers of the ePub version may also receive for free the PDF version with additional, fascinating images that can be read on a computer (see imprint of the eBook).

Table of contents:

Chapter 1. Presenting the Universe

Chapter 2. The Time Before Time
A world made from strings
Loop over loop
Reborn from nothing
Nothing but theories?

Chapter 3. The Big Bang
The 0 hour
The laws of physics begin
The world – a soccer ball
The first particles
All of the forces are already there
The next round of extinction

Chapter 4. The Clear Universe
The first beacons
They die young
A fascinating death
Group dynamics
Fragile spirals
Planets from the waste

Chapter 5. The Life and Death of Stars
Too small: brown dwarfs
The Joe Six-Pack of the universe: red dwarfs
The Sun’s relatives: main-sequence stars
The future of the Sun: white dwarf
Extremely dense: neutron stars
The odd balls: quark stars
Where space and time are meaningless: black holes
Even stranger: exotic stars
How large can stars be? The hyper-giants

Chapter 6. The Planets
Our home: The Solar System
Life-giving: the Sun
The closest to the Sun: Mercury
The most like Earth: Venus
The blue planet: Earth
The red planet: Mars
An unfinished work: the Asteroid Belt
Holding everything together: Jupiter
The lord of the Rings: Saturn
The icy one: Uranus
Another blue planet: Neptune
Way out there: the Kuiper Belt
The garbage dump: the Oort Cloud
The extraterrestrials: exoplanets
The mavericks: planemos

Chapter 7. The End of the Universe
Death by freezing
Death by tearing apart
Death by being crunched
Death by annihilation
Death by disintegration
Death by solidification
One cross each!
The future biography of the universe
Imprint

About the author: Matthias Matting, born 1966, is a physicist and journalist. For his eBook "Travel to Fukushima" he received the first german eBook price. In 2011, he was the official bestselling author at Amazon Germany. He's working in the science & technology department of the german news magazine FOCUS. Since five years he authors the weekly gadget review video series "Mattings Warentest" at FOCUS.de.

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$1.99

Lectures on the Forces of Matter

By: Michael Faraday

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Lectures on the Forces of Matter

By: Michael Faraday

Michael Faraday, FRS (22 September 1791 25 August 1867) was an English chemist and physicist (or natural philosopher, in the terminology of the time) who contributed to the fields of electromagnetism and electrochemistry. Faraday studied the magnetic field around a conductor carrying a DC electric current. While conducting these studies, Faraday established the basis for the electromagnetic field concept in physics, subsequently enlarged upon by James Maxwell. He similarly discovered electromagnetic induction, diamagnetism, and laws of electrolysis. He established that magnetism could affect rays of light and that there was an underlying relationship between the two phenomena. His inventions of electromagnetic rotary devices formed the foundation of electric motor technology, and it was largely due to his efforts that electricity became viable for use in technology. Although Faraday received little formal education and knew little of higher mathematics, such as calculus, he was one of the most influential scientists in history. Historians of science refer to him as the best experimentalist in the history of science. Throughout his life, Faraday discussed science and his work in letters to contemporaries, and he also delivered lectures on numerous topics. All of these materials were published near the end of the 19th century. These six lectures on gravitation, cohesion, chemical affinity, heat, magnetism, and electricity were intended for young audiences. Together, they offer the reader a fascinating introduction to some of Faraday's most important work on the correlation between the physical forces of the universe. This edition of Faradays Lectures on the Forces of Matter is specially formatted with a Table of Contents.

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$0.99

On the Electrodynamics of Moving Bodies (Illustrated Edition)

By: Albert Einstein

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On the Electrodynamics of Moving Bodies (Illustrated Edition)

By: Albert Einstein

Albert Einstein (1879-1955) needs no formal introduction, as he is known around the world as one of historys most brilliant geniuses and one of its most influential scientists. Einstein is often regarded as the father of modern physics and received the 1921 Nobel Prize in Physics "for his services to theoretical physics, and especially for his discovery of the law of the photoelectric effect". Einstein published more than 300 scientific papers along with over 150 non-scientific works. His great intelligence and originality have made the word "Einstein" synonymous with genius. Einsteins greatest and most famous theory is the theory of relativity, which fundamentally changed the understanding of physics and astronomy during the 20th century. When first published, relativity superseded a 200-year-old theory of mechanics put forth by Isaac Newton. The theory of relativity overturned the concept of motion from Newton's day, into all motion is relative. Time was no longer uniform and absolute. Therefore, no longer could physics be understood as space by itself, and time by itself. Instead, an added dimension had to be taken into account with curved spacetime. Time now depended on velocity, and contraction became a fundamental consequence at appropriate speeds. In the field of physics, relativity catalyzed and added an essential depth of knowledge to the science of elementary particles and their fundamental interactions, along with ushering in the nuclear age. With relativity, cosmology and astrophysics predicted extraordinary astronomical phenomena such as neutron stars, black holes, and gravitational waves. This edition of Einsteins On the Electrodynamics of Moving Bodies is specially formatted with a Table of Contents and is illustrated with pictures of the great thinker.

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$15.49

The Quantum Universe

By: Brian Cox, Jeff Forshaw

$15.49

The Quantum Universe

By: Brian Cox, Jeff Forshaw

In The Quantum Universe, Brian Cox and Jeff Forshaw approach the world of quantum mechanics in the same way they did in Why Does E=mc2? and make fundamental scientific principles accessible-and fascinating-to everyone.

The subatomic realm has a reputation for weirdness, spawning any number of profound misunderstandings, journeys into Eastern mysticism, and woolly pronouncements on the interconnectedness of all things. Cox and Forshaw’s contention? There is no need for quantum mechanics to be viewed this way. There is a lot of mileage in the weirdness” of the quantum world, and it often leads to confusion and, frankly, bad science. The Quantum Universe cuts through the Wu Li and asks what observations of the natural world made it necessary, how it was constructed, and why we are confident that, for all its apparent strangeness, it is a good theory.

The quantum mechanics of The Quantum Universe provide a concrete model of nature that is comparable in its essence to Newton’s laws of motion, Maxwell’s theory of electricity and magnetism, and Einstein’s theory of relativity.

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