Edwin Thomas – författare

Not many men emerged from Trafalgar without an ounce of credit to their names, but courtesy of an over-fondness for rum and his habitual bad luck, Lieutenant Martin Jerrold managed it. In February 1806, he is given one final chance to redeem his reputation and dispatched to Dover.Things don't augur well when, walking off the effects of a night in the tavern, Jerrold stumbles across a corpse lying on the beach. And they take a distinct turn for the worst when, to his horror and bemusement, he is suspected of murder. With a captain who despises him, and the local magistrate determined to see him hang, he knows clearing his name will require an imporbable reversal of his miserable fortunes. Somewhere in Dover's twisted streets, someone must know something. But Jerrold soon discovers that nothing is as it seems in a town where smuggling is a way of life, where everyone from the fishermen to the colonel of dragoons drinks only the finest French brandy...Distrusted by his superiors, set upon by suspiciously well-informed thugs and attacked by the French at sea, Jerrold does find some sympathy in the less-than-respectable arms of the comely Isobel, but he knows he has but two weeks to save his skin - or perish in the attempt.

August, 1806. As Britain fights alone against France, the greatest political chancer of his age hatches an audacious plot to upend the world order. Only one man stands in his way. Unfortunately, that man is Lieutenant Martin Jerrold.With powerful enemies in England to escape, Jerrold is only too happy to undertake a routine mission to America. But he'll soon wish he had stayed at home, as his journey takes him across pirate-infested seas, through the wilderness of the American frontier and down the mighty Mississippi river - into the heart of an extraordinary conspiracy. The stakes are high - the entire future of Britain's war against Napoleon rests in his not-so-capable hands. One wrong move and the consequences will be catastrophic, even by Jerrold's own dismal standards.

July 1806. Commanding a prison hulk full of French captives, Lieutenant Martin Jerrold thinks his war can't get much better. He's far away from the more life threatening aspects of naval service and he can keep his mistress close to hand. It all seems too good to last. And so it proves. When one of the prisoners goes missing, Jerrold's comfortable world is suddenly turned upside down. Ordered by the First Lord of the Admiralty to recapture the Frenchman at any cost, he finds himself racing across England: from the stinking marshes of Chatham to the wilds of Dartmoor and the fashionable resort of Brighton. But what makes this prisoner so damned important? At the Post Office, Jerrold's old friend Mr Nevell is curious; so too are politicians from either side, including the cunning Tory leader Spencer Perceval. Even the seductive Princess Caroline takes an unexpected interest. As Jerrold - dogged by his usual bad timing, bad luck and bad behaviour - closes in on his elusive quarry, he uncovers a devilish web of treachery and deceit stretching back twenty years and ensnaring the most exalted members of society. And in hot pursuit are those who will stop at nothing to stop him...

This book provides an accessible introduction to the fascinating and topical subject of black holes. It bridges the gap between popular non-mathematical expositions and advanced research texts, using simple undergraduate level calculations and the most basic knowledge of relativity to explain current research. This means the theory can be understood by a wide audience of physicists, including those who are not necessarily interested in learning higher-level mathematical techniques.This new edition introduces a chapter dedicated to a selection of recent results. Existing chapters have been updated and new explanatory material has been added to aid in the understanding of the physics.This book is recommended reading for advanced undergraduate students and first-year postgraduates who will find it a useful stepping-stone to the advanced literature.

This book provides an accessible introduction to the fascinating and topical subject of black holes. It bridges the gap between popular non-mathematical expositions and advanced research texts, using simple undergraduate level calculations and the most basic knowledge of relativity to explain current research. This means the theory can be understood by a wide audience of physicists, including those who are not necessarily interested in learning higher-level mathematical techniques.This new edition introduces a chapter dedicated to a selection of recent results. Existing chapters have been updated and new explanatory material has been added to aid in the understanding of the physics.This book is recommended reading for advanced undergraduate students and first-year postgraduates who will find it a useful stepping-stone to the advanced literature.

This introduction to the fascinating subject of black holes fills a significant gap in the literature which exists between popular, non-mathematical expositions and advanced textbooks at the research level. It is designed for advanced undergraduates and first year postgraduates as a useful stepping-stone to the advanced literature.The book provides an accessible introduction to the exact solutions of Einstein's vacuum field equations describing spherical and axisymmetric (rotating) black holes. The geometry and physical properties of these spacetimes are explored through the motion of particles and light. The use of different coordinate systems, maximal extensions and Penrose diagrams is explained. The association of the surface area of a black hole with its entropy is discussed and it is shown that with the introduction of quantum mechanics black holes cease to be black and can radiate. This result allows black holes to satisfy the laws of thermodynamics and thus be consistent with the rest of physics.In this new edition the problems in each chapter have been revised and solutions are provided. The text has been expanded to include new material on wormholes and clarify various other issues.Sample Chapter(s)

This introduction to the fascinating subject of black holes fills a significant gap in the literature which exists between popular, non-mathematical expositions and advanced textbooks at the research level. It is designed for advanced undergraduates and first year postgraduates as a useful stepping-stone to the advanced literature.The book provides an accessible introduction to the exact solutions of Einstein's vacuum field equations describing spherical and axisymmetric (rotating) black holes. The geometry and physical properties of these spacetimes are explored through the motion of particles and light. The use of different coordinate systems, maximal extensions and Penrose diagrams is explained. The association of the surface area of a black hole with its entropy is discussed and it is shown that with the introduction of quantum mechanics black holes cease to be black and can radiate. This result allows black holes to satisfy the laws of thermodynamics and thus be consistent with the rest of physics.In this new edition the problems in each chapter have been revised and solutions are provided. The text has been expanded to include new material on wormholes and clarify various other issues.Sample Chapter(s)

This introduction to the fascinating subject of black holes fills a significant gap in the literature which exists between popular, non-mathematical expositions and advanced textbooks at the research level. It is designed for advanced undergraduates and first year postgraduates as a useful stepping-stone to the advanced literature.The book provides an accessible introduction to the exact solutions of Einstein's vacuum field equations describing spherical and axisymmetric (rotating) black holes. The geometry and physical properties of these spacetimes are explored through the motion of particles and light. The use of different coordinate systems, maximal extensions and Penrose diagrams is explained. The association of the surface area of a black hole with its entropy is discussed and it is shown that with the introduction of quantum mechanics black holes cease to be black and can radiate. This result allows black holes to satisfy the laws of thermodynamics and thus be consistent with the rest of physics.Sample Chapter(s)