Nuclear Science Abstracts
Author :
Publisher :
Page : 1256 pages
File Size : 11,38 MB
Release : 1973
Category : Nuclear energy
ISBN :
Author :
Publisher :
Page : 1256 pages
File Size : 11,38 MB
Release : 1973
Category : Nuclear energy
ISBN :
Author :
Publisher :
Page : 348 pages
File Size : 40,3 MB
Release : 1990
Category : Astronomical observatories
ISBN :
Chiefly reprints.
Author :
Publisher :
Page : 1666 pages
File Size : 18,53 MB
Release : 1992
Category : Aeronautics
ISBN :
Author :
Publisher :
Page : 1508 pages
File Size : 47,27 MB
Release : 1969
Category : Aeronautics
ISBN :
Author : Charles Philip Sonett
Publisher : University of Arizona Press
Page : 1040 pages
File Size : 19,74 MB
Release : 1991
Category : Science
ISBN : 9780816512973
An interdisciplinary approach to solar physics, as eighty-nine contributors trace the evolution of the Sun and provide a review of our current understanding of both its structure and its role in the origin and evolution of the solar system.
Author : F. Halle
Publisher : Springer Science & Business Media
Page : 457 pages
File Size : 37,75 MB
Release : 2012-12-06
Category : Science
ISBN : 3642811906
Author : David Peck Todd
Publisher :
Page : 506 pages
File Size : 49,82 MB
Release : 1906
Category : Astronomy
ISBN :
Author : Cole Johnston
Publisher : Springer Nature
Page : 198 pages
File Size : 20,31 MB
Release : 2021-05-21
Category : Science
ISBN : 3030663108
This thesis by Cole Johnston brings novel insights into the inner workings of young massive stars. By bridging the observational fields of binary stars and asteroseismology this thesis uses state of the art statistical techniques to scrutinise theories of modern stellar astrophysics. Developing upon the commonly used isochrone fitting methodology, the author introduces the idea of isochrone cloud fitting in order to account for the full breadth of physics observed in stars. The author combines this methodology with gravity mode asteroseismic analysis to asses the level of chemical mixing deep within the stellar core in order to determine the star‘s age and core mass. Wrapped into a robust statistical framework to account for correlations, this methodology is employed to analyse individual stars, multiple systems, and clusters alike to demonstrate that chemical mixing has dramatic impact on stellar structure and evolution.
Author : Svante Arrhenius
Publisher :
Page : 258 pages
File Size : 44,1 MB
Release : 1908
Category : Cosmogony
ISBN :
Author : H.C. Arp
Publisher : Springer Science & Business Media
Page : 364 pages
File Size : 22,40 MB
Release : 2013-11-11
Category : Science
ISBN : 1489912258
The Hidden Hypotheses Behind the Big Bang It is quite unavoidable that many philosophical a priori assumptions lurk behind the debate between supporters of the Big Bang and the anti-BB camp. The same battle has been waged in physics between the determinists and the opposing viewpoint. Therefore, by way of introduction to this symposium, I would like to discuss, albeit briefly, the many "hypotheses", essentially of a metaphysical nature, which are often used without being clearly stated. The first hypothesis is the idea that the Universe has some origin, or origins. Opposing this is the idea that the Universe is eternal, essentially without beginning, no matter how it might change-the old Platonic system, opposed by an Aristote lian view! Or Pope Pius XII or Abbe Lemaitre or Friedmann versus Einstein or Hoyle or Segal, etc. The second hypothesis is the need for a "minimum of hypotheses" -the sim plicity argument. One is expected to account for all the observations with a mini mum number of hypotheses or assumptions. In other words, the idea is to "save the phenomena", and this has been an imperative since the time of Plato and Aristotle. But numerous contradictions have arisen between the hypotheses and the facts. This has led some scientists to introduce additional entities, such as the cosmologi cal constant, dark matter, galaxy mergers, complicated geometries, and even a rest mass for the photon. Some of the proponents of the latter idea were Einstein, de Broglie, Findlay-Freundlich, and later Vigier and myself.