By Norman K Glendenning
In a super flash approximately fourteen billion years in the past, time and topic have been born in one fast of production. An immensely scorching and dense universe started its speedy enlargement in every single place, growing area the place there has been no area and time the place there has been no time. within the extreme hearth simply after the start, the lightest components have been solid, later to shape primordial clouds that at last advanced into galaxies, stars, and planets. This evolution is the tale advised during this interesting e-book. Interwoven with the storyline are brief items at the pioneering women and men who printed these wonders to us.
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Extra info for After The Beginning: A Cosmic Journey Through Space And Time
He developed t h e theory of electrons as waves, whose wavelength A he related t h r o u g h Planck's constant ft, t h e electron mass m , and its velocity v. 5 Legend has it t h a t de Broglie's professors at t h e Sorbonne consulted Einstein about whether he should receive a degree for his thesis. Einstein replied t h a t he had better be given a Nobel Prize. T h e theory was proven correct in experiments performed in 1927. 6 He was awarded t h e prize two years later. 1). If a b e a m of 5 6 Comptes rendus de VAcadmie des Sciences, Vol.
Island Universes 23 Light seems to us in our everyday experience to be a continuous beam. And particles seem to be particles — quite discrete and distinct objects. However, light has some particlelike properties and particles have some wavelike properties. One way in which the particulate nature of light shows up is by the fact t h a t its energy is carried in small bundles, the so-called quantum of energy. T h e energy carried by the q u a n t a of light of one particular color is different from t h a t carried by the q u a n t a of another color.
Such spectra are called absorption line spectra. By comparing the absorption lines in the spectrum coming from the distant star with lines produced by known atoms in the laboratory, the elements in the star's atmosphere can be identified. 19 o1— Fig. 15. Quantum states (levels) of the single-electron hydrogen atom are represented by horizontal lines. Distances between levels represent the energy differences. Energies, as measured in a unit called the electron volt, are listed at the side. 24 Norman K.
After The Beginning: A Cosmic Journey Through Space And Time by Norman K Glendenning