Name: Structure and Expansion of a Universe Whose Vacuum is Modelled as a set of Identical, Bi-Modal, Frequency-Quantised, Simple Quantum Harmonic Oscillators. (en Inglés)
SKU: 63018616
Price: 516.33 MXN
Availability: InStock
Author: William Fidler
ISBN: 9783668667587

portada Structure and Expansion of a Universe Whose Vacuum is Modelled as a set of Identical, Bi-Modal, Frequency-Quantised, Simple Quantum Harmonic Oscillators. (en Inglés)

Structure and Expansion of a Universe Whose Vacuum is Modelled as a set of Identical, Bi-Modal, Frequency-Quantised, Simple Quantum Harmonic Oscillators. (en Inglés)

Formato

Libro Físico

Editorial

Grin Verlag

Autor

William Fidler

Idioma

Inglés

N° páginas

Encuadernación

Tapa Blanda

ISBN13

9783668667587

Structure and Expansion of a Universe Whose Vacuum is Modelled as a set of Identical, Bi-Modal, Frequency-Quantised, Simple Quantum Harmonic Oscillators. (en Inglés)

William Fidler (Autor) · Grin Verlag · Tapa Blanda

Libro Nuevo Importado

Envío: 23 a 28 días háb.

$ 938.79$ 516.33

-45%

Costos de importación incluídos en el precio ✅

Libro Nuevo

Quedan 10 unidades

$ 516.33

¡Envío Gratis! Llega entre el 12 Oct y el 20 Oct a CUAUHTÉMOC, Ciudad de México. Seleccionar ubicación

Agregar a lista de deseos

Reseña del libro "Structure and Expansion of a Universe Whose Vacuum is Modelled as a set of Identical, Bi-Modal, Frequency-Quantised, Simple Quantum Harmonic Oscillators. (en Inglés)"

Academic Paper from the year 2018 in the subject Physics - Astronomy, grade: 1.00, language: English, abstract: The 'fabric' of the model presented here consists of identical, contiguous cubes of space, each of which is occupied by a simple quantum harmonic oscillator. A possible structure is proposed for the ensemble of cubes, and it is shown also that other configurations, on all scales can exist in the ensemble, even although the members of that collection are absolutely identical. The expansion of space is considered initially from the standpoint of a universe which is not accelerating, and equations are developed which relate to this 'coasting' condition, and, in which the Hubble parameter, H, is shown to be a function of time. These equations are extended by the inclusion of the deceleration parameter of cosmology, q, treating q as a parameter.