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Extreme Nonlinear Optics An Introduction




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Dettagli

Genere:Libro
Lingua: Inglese
Editore:

Springer

Pubblicazione: 08/2004
Edizione: 2005





Trama

Following the birth of the laser in 1960, the field of "nonlinear optics" rapidly emerged.

Today, laser intensities and pulse durations are readily available, for which the concepts and approximations of traditional nonlinear optics no longer apply. In this regime of "extreme nonlinear optics," a large variety of novel and unusual effects arise, for example frequency doubling in inversion symmetric materials or high-harmonic generation in gases, which can lead to attosecond electromagnetic pulses or pulse trains. Other examples of "extreme nonlinear optics" cover diverse areas such as solid-state physics, atomic physics, relativistic free electrons in a vacuum and even the vacuum itself.

This book starts with an introduction to the field based primarily on extensions of two famous textbook examples, namely the Lorentz oscillator model and the Drude model. Here the level of sophistication should be accessible to any undergraduate physics student. Many graphical illustrations and examples are given. The following chapters gradually guide the student towards the current "state of the art" and provide a comprehensive overview of the field. Every chapter is accompanied by exercises to deepen the reader's understanding of important topics, with detailed solutions at the end of the book.





Sommario

Selected Aspects of Few-Cycle Laser Pulses and Nonlinear Optics.- The Lorentz Oscillator Model and Beyond ….- The Drude Free-Electron Model and Beyond ….- Lorentz Becomes Drude: Bound—Unbound Transitions.- Accounting for Propagation Effects.- Extreme Nonlinear Optics of Semiconductors and Isolators.- Extreme Nonlinear Optics of Atoms and Electrons.










Altre Informazioni

ISBN:

9783540222910

Condizione: Nuovo
Collana: Advanced Texts in Physics
Dimensioni: 235 x 155 mm Ø 511 gr
Formato: Copertina rigida
Illustration Notes:X, 223 p.
Pagine Arabe: 223
Pagine Romane: x


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