I ciufolini (39 risultati)

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Hardcover. Condizione: Good. Hardcover, xiii + 412 pages, NOT ex-library. Printed in the UK. Limited signs of gentle wear, book is clean with unmarked text, free of inscriptions and stamps, securely bound. Issued without a dust jacket. -- Contents: 1 Gravitational waves, theory and experiment (an overview); Part One: Gravitational Waves, Sources and Detectors 2 Elements of gravitational waves [Mathematics of linearized theory; Using the TT gauge to understand gravitational waves; Interaction of gravitational waves with detectors; Analysis of beam detectors; Exercises] 3 Gravitational-wave detectors [Gravitational-wave observables; Physics of interferometers; Physics of resonant mass detectors; A detector in space; Gravitational and electromagnetic waves compared and contrasted] 4 Astrophysics of gravitational-wave sources [Sources detectable from ground & from space] 5 Waves and energy [Variational principle for general relativity; Variational principles and the energy in gravitational waves; Practical applications of the Isaacson energy; Exercises] 6 Mass- and current-quadrupole radiation [Expansion for the far field of a slow-motion source; Application of the TT gauge to the mass quadrupole field; Application of the TT gauge to the current-quadrupole field; Energy radiated in gravitational waves; Radiation in the Newtonian limit] 7 Source calculations [Radiation from a binary system; R-modes; Conclusion]; References; Solutions to exercises; -- Part Two: Gravitational-wave detectors 8 Resonant detectors for gravitational waves & their bandwidth [Sensitivity and bandwidth of resonant detectors; Sensitivity for various GW signals; Recent results obtained with the resonant detectors; Discussion and conclusions] 9 Earth-based large interferometer Virgo and the Low Frequency Facility [Introduction; SA suspension and requirements on the control; A few words about the Low Frequency Facility; Conclusion] 10 LISA: A proposed joint ESA-NASA gravitational-wave mission [Description of the LISA mission; Expected gravitational-wave results from LISA] 11 Detection of scalar gravitational waves [Introduction; Testing theories of gravity; Gravitational wave radiation in the JBD theory; Hollow sphere; Scalar-tensor cross sections]; -- Part Three: Stochastic Gravitational-Wave Background 12 Generalities on the stochastic GW background [Introduction; Definitions; Overlap reduction function; Achievable sensitivities to the SGWB; Observational bounds] 13 Sources of SGWB [Topological defects; Inflation; String cosmology; First-order phase transitions; Astrophysical sources]; -- Part Four: Theoretical developments 14 Infinite-dimensional symmetries in gravity [Einstein theory; Nonlinear [sigma]-models; Symmetries of nonlinear [sigma]-models; Geroch group; Linear system] 15 Gyroscopes and gravitational waves [Introduction; Splitting formalism & test particle motion: a short review; Spacetime metric; Searching for an operational frame; Precession of a gyroscope in geodesic motion; Conclusions] 16 Elementary introduction to pre-big bang cosmology and to the relic graviton background [Introduction; Motivations: duality symmetry; Kinematics: shrinking horizons; Open problems & phenomenological consequences; Cosmological perturbation theory; Relic graviton background; Conclusion; Appendix (String effective action; Duality symmetry; String cosmology equations] 17 Post-Newtonian computation of binary inspiral waveforms [Introduction; Summary of optimal signal filtering; Newtonian binary polarization waveforms; Newtonian orbital phase evolution; Post-Newtonian wave generation; Inspiral binary waveform]; -- Part Five: Numerical relativity 18 Numerical relativity [Overview; Einstein equations for relativity; Still newer formulations: towards a stable evolution system; Tools for analysing the numerical spacetimes; Computational science, numerical relativity, and the 'Cactus' code; Cactus computational toolkit; Recent applications and progress; Summary; Further reading]; References; Index.…

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Hardcover. Condizione: Fine. 1st Edition. EXCELLENT Unmarked PAGES And BINDING And COVER. Hardback. As Shown. No dust Jacket, as issued. Previous owner signature on flyleaf. Approximately 6 1/2 X 9 1/2. 412 pages.

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Hardcover. Condizione: New. Brand new book, sourced directly from publisher. Dispatch time is 7-8 days from our warehouse. Book will be sent in robust, secure packaging to ensure it reaches you securely.

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Condizione: New. pp. 428.

Condizione: New. I. Ciufolini, E. Coccia, V. Gorini, N. Vittorio. R. PersonAlthough gravity is the dominant force of nature at large distances (from intermediate scales to the Hubble length), it is the weakest of forces in particle physics, though it is believed to b.

Condizione: New. pp. 428.

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Hardcover. Condizione: Brand New. 1st edition. 412 pages. 9.75x6.50x1.25 inches. In Stock.

Soft cover. Condizione: Near Fine. 1st Edition. First edition, journal issue in original printed wrappers, of the first accurate observational confirmation of the Lense-Thirring effect. This is an effect predicted by general relativity and also known as 'frame dragging' in which the orbit of a small body orbiting around a rotating massive one is slightly perturbed by the rotation. The effect was first predicted by Austrian physicists Joseph Lense and Hans Thirring in 1918, although similar effects were obtained by Einstein and Besso in 1913. "An important early prediction of Einstein's general relativity was the advance of the perihelion of Mercury's orbit, whose measurement provided one of the classical tests of Einstein's theory. The advance of the orbital point-of-closest-approach also applies to a binary pulsar system and to an Earth-orbiting satellite. General relativity also predicts that the rotation of a body like Earth will drag the local inertial frames of reference around it, which will affect the orbit of a satellite. This Lense Thirring effect has hitherto not been detected with high accuracy, but its detection with an error of about 1 per cent is the main goal of Gravity Probe B an ongoing space mission using orbiting gyroscopes. Here we report a measurement of the Lense Thirring effect on two Earth satellites: it is 99 ± 5 per cent of the value predicted by general relativity" (from the paper). Large 8vo, pp. xviii, 883-1022, 36. Original printed wrappers (slight wear to foot of spine).…