715 research outputs found

    Electromagnetic cascade in high energy electron, positron, and photon interactions with intense laser pulses

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    The interaction of high energy electrons, positrons, and photons with intense laser pulses is studied in head-on collision geometry. It is shown that electrons and/or positrons undergo a cascade-type process involving multiple emissions of photons. These photons can consequently convert into electron-positron pairs. As a result charged particles quickly lose their energy developing an exponentially decaying energy distribution, which suppresses the emission of high energy photons, thus reducing the number of electron-positron pairs being generated. Therefore, this type of interaction suppresses the development of the electromagnetic avalanche-type discharge, i.e., the exponential growth of the number of electrons, positrons, and photons does not occur in the course of interaction. The suppression will occur when 3D effects can be neglected in the transverse particle orbits, i.e., for sufficiently broad laser pulses with intensities that are not too extreme. The final distributions of electrons, positrons, and photons are calculated for the case of a high energy e-beam interacting with a counter-streaming, short intense laser pulse. The energy loss of the e-beam, which requires a self-consistent quantum description, plays an important role in this process, as well as provides a clear experimental observable for the transition from the classical to quantum regime of interaction.Comment: 13 pages, 7 figure

    Pennsylvanian Geology and Mineral Resources of West Central Indiana

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    Indiana Geological Survey Guidebook 5During the period of oil and gas development in the 1950s, many petroleum geologists became interested in Pennsylvanian stratigraphy in Indiana. They hoped that the attitude of some of the key beds in the Pennsylvanian might indicate location of domes in deeper oil producing horizons. The sponsors organized this conference to give petroleum geologists, coal producers, clay producers, and other interested persons a better understanding of Pennsylvanian stratigraphy. The conference was planned to provide an opportunity to observe and discuss representative sections of the Pennsylvanian formations in western Indiana. Unfortunately, the best exposures are in the last cuts of strip mines, many of which are no longer accessible. Similar adjacent sections, however, may be available. The sections which have been selected are considered to be about average. The writers hope that the discussion both of the sections presented herein and of the problems connected with them will be mutually beneficial. The opportunity to become better acquainted and to exchange ideas is an important part of the conference.Department of Geology, Indiana University; Indiana Geological Survey; Indiana Department of Conservatio

    Nonlinear evolution of the plasma beatwave: Compressing the laser beatnotes via electromagnetic cascading

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    The near-resonant beatwave excitation of an electron plasma wave (EPW) can be employed for generating the trains of few-femtosecond electromagnetic (EM) pulses in rarefied plasmas. The EPW produces a co-moving index grating that induces a laser phase modulation at the difference frequency. The bandwidth of the phase-modulated laser is proportional to the product of the plasma length, laser wavelength, and amplitude of the electron density perturbation. The laser spectrum is composed of a cascade of red and blue sidebands shifted by integer multiples of the beat frequency. When the beat frequency is lower than the electron plasma frequency, the red-shifted spectral components are advanced in time with respect to the blue-shifted ones near the center of each laser beatnote. The group velocity dispersion of plasma compresses so chirped beatnotes to a few-laser-cycle duration thus creating a train of sharp EM spikes with the beat periodicity. Depending on the plasma and laser parameters, chirping and compression can be implemented either concurrently in the same, or sequentially in different plasmas. Evolution of the laser beatwave end electron density perturbations is described in time and one spatial dimension in a weakly relativistic approximation. Using the compression effect, we demonstrate that the relativistic bi-stability regime of the EPW excitation [G. Shvets, Phys. Rev. Lett. 93, 195004 (2004)] can be achieved with the initially sub-threshold beatwave pulse.Comment: 13 pages, 11 figures, submitted to Physical Review

    Experimental observation of nonlinear Thomson scattering

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    A century ago, J. J. Thomson showed that the scattering of low-intensity light by electrons was a linear process (i.e., the scattered light frequency was identical to that of the incident light) and that light's magnetic field played no role. Today, with the recent invention of ultra-high-peak-power lasers it is now possible to create a sufficient photon density to study Thomson scattering in the relativistic regime. With increasing light intensity, electrons quiver during the scattering process with increasing velocity, approaching the speed of light when the laser intensity approaches 10^18 W/cm^2. In this limit, the effect of light's magnetic field on electron motion should become comparable to that of its electric field, and the electron mass should increase because of the relativistic correction. Consequently, electrons in such high fields are predicted to quiver nonlinearly, moving in figure-eight patterns, rather than in straight lines, and thus to radiate photons at harmonics of the frequency of the incident laser light, with each harmonic having its own unique angular distribution. In this letter, we report the first ever direct experimental confirmation of these predictions, a topic that has previously been referred to as nonlinear Thomson scattering. Extension of these results to coherent relativistic harmonic generation may eventually lead to novel table-top x-ray sources.Comment: including 4 figure

    Optimized laser pulse profile for efficient radiation pressure acceleration of ions

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    The radiation pressure acceleration regime of laser ion acceleration requires high intensity laser pulses to function efficiently. Moreover the foil should be opaque for incident radiation during the interaction to ensure maximum momentum transfer from the pulse to the foil, which requires proper matching of the target to the laser pulse. However, in the ultrarelativistic regime, this leads to large acceleration distances, over which the high laser intensity for a Gaussian laser pulse must be maintained. It is shown that proper tailoring of the laser pulse profile can significantly reduce the acceleration distance, leading to a compact laser ion accelerator, requiring less energy to operate.Comment: 10 pages, 4 figure

    Correlation of the Waldron and Mississinewa Formations

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    Indiana Geological Survey Bulletin 3Silurian and Devonian outcrops of Indiana are divided roughly into two areas, northern and southeastern Indiana. The bedrock of the northern area is largely covered by glacial drift, whereas the bedrock of the southeastern area is well exposed. These two areas are separated by an intervening zone which is blanketed completely by glacial drift. Although accurate and detailed work has been done on the Silurian and Devonian outcrops of the state, the formations of the two areas have never been correlated. The Silurian and Devonian formations in Indiana dip off the Cincinnati and Kankakee Arches into the Michigan Basin and the Eastern Interior Basin. The formations are difficult to trace in subsurface studies, because they are composed of a series of gradational limestones, dolomites, and calcareous siltstones. The surface formations have not been recognized in the subsurface strata. Some of the subsurface beds cannot be correlated with the outcropping beds, because additional sediments deposited in the basin do not appear on the arches. The Silurian-Devonian contact lacks identifying characteristics over much of the area, and, for this reason, many subsurface reports have considered both systems as one unit. The writers believe that accurate determinations of thickening, thinning, and pinching-out of the Silurian and Devonian formations on the flanks of the arches would be of great assistance in future prospecting for oil. These two problems, the geology of the arches and the geology of the basins, go hand in hand. Additional subsurface correlation studies are needed to clarify the Silurian and Devonian stratigraphy of Indiana.Indiana Department of Conservatio

    Silurian Formations and Reef Sturctures of Northern Indiana

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    Indiana Geological Survey Guidebook 3In response to popular demand, the Silurian formations and associated reef structures of northern Indiana were chosen as the subject for the 1949 Field Conference. The numerous quaquaversal structures in the Niagaran of northern Indiana were long the subject of controversies and objects of mystery until, in 1927, Cumings and Shrock showed conclusively that they are ancient coral and stromatoporoid reefs. In the past few years, interest in reefs, recent and ancient, has been revived. The vast number of soundings taken in coral reef lagoons during the war and recent studies in connection with the Bikini atom bomb tests have shed much new light on present day reefs, and recent oil field discoveries associated with reef structures have stimulated much interest and study of the Paleozoic reefs. The conference has been planned to provide group observation and to promote group discussion of Niagaran reefs. Silurian stratigraphy is emphasized and special attention is given to lithology of reef core, reef flank, and inter-reef strata, as well as to the effect of reef structure on the overlying Devonian rocks. We hope that discussion combined with actual field examples will be of mutual benefit. This opportunity to become better acquainted and to exchange ideas is the most important part of the program.Department of Geology, Indiana University; Indiana Division of Geology; Indiana Department of Conservatio

    Resonant laser‐plasma electron acceleration

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    Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/87302/2/65_1.pd
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