About Science, Myself and Others by V.L. Ginzburg PDF

By V.L. Ginzburg

ISBN-10: 075030992X

ISBN-13: 9780750309929

ISBN-10: 142003474X

ISBN-13: 9781420034745

In approximately technology, Myself and Others, Vitaly Lazarevich Ginzburg, co-recipient of the 2003 Nobel Prize in Physics and Editor of the evaluation magazine Physics-Uspekhi, presents an perception into smooth physics, the lives and works of alternative famous physicists he has recognized, and perception into his personal existence and perspectives on physics and past.

Divided into 3 elements, the e-book begins with a evaluate of the most important difficulties in modern physics, astrophysics, and cosmology, analyzing their historic improvement and why they pose this sort of problem to brand new physicists and for society. half One additionally contains information of a few of Professor Ginzburg's paintings, together with superconductivity and superfluidity. half encompasses numerous articles at the lives and works of a number of widespread physicists, together with the writer. The 3rd half is a set of articles that supply a private view of the writer, describing his own perspectives and reminiscences on quite a number wider themes.

Taken jointly, this choice of articles creates an stress-free assessment of physics, its philosophy, and key avid gamers in its smooth improvement within the twentieth Century. surely, it is going to be an stress-free learn for pro physicists and non-scientists alike.

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Extra resources for About Science, Myself and Others

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4 × 104 GeV will be obtained (hopefully in 2006–07) in the center-of-mass frame, in cosmic rays the energy of up to 3 × 1011 GeV is fixed, and the Planck energy is mg c2 ∼ 1016 erg ∼ 1019 GeV. In the Grand Unification theory, energies of up to 1016 GeV figure (particles of mass mGUT ∼ 10−8 g). This region is the arena of intense theoretical studies. Turning to problem 24 (neutron stars and pulsars, supernova stars), I note, first of all, that the hypothesis of the existence of neutron stars was formulated, as far as I know, in 1934.

More details concerning gamma-bursts are given in the review [103] (see also [245]). GRB 021004 (detected, as clear from its designation, on 4 October, 2002) proved to be very intriguing. It was accompanied by a prolonged optical afterglow. 5, which corresponds to a distance of 11×109 light years [154] from us. It should be emphasized that gamma-ray emission from gamma-ray bursts is most probably anisotropic. Additional strong evidence for this that z = (λobs − λsource )/λsource , where λobs is the observed wavelength of the spectral line and λsource is the wavelength in the source.

I have already mentioned the detection of neutrinos from the explosion of supernova SN 1987A. Monitoring is now being carried out and if we are lucky and another supernova explodes near the Sun (in the Galaxy or Magellanic Clouds), we shall obtain rich material (supernovae explode in the Galaxy on average approximately once every 30 years but this figure is inaccurate and, what is important, an explosion may occur at any moment). The problem of detecting relic low-energy neutrinos which may contribute to the dark matter is especially noteworthy.

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About Science, Myself and Others by V.L. Ginzburg

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