On the cosmological implications of the Calogero conjecture
نویسنده
چکیده
We discuss the implications of the Calogero hypothesis on the \cosmic origin of quantization" 1], and of the variation of h with time it implies, for cosmology. We focus on two issues: (a) how the relation between redshift and distance would be modiied; and (b) how the observations on the cosmic background radiation, and the estimation they give of the time elapsed since its production, would be interpreted in the light of Calogero hypothesis. We also check that the hypothesis is compatible with the present bounds on the variations of fundamental constants and with the observed blackbody distribution of the cosmic background radiation.
منابع مشابه
Bianchi Type I Cosmology and the Euler-calogero-sutherland Model
The Bianchi type I cosmological model is brought into a form where the evolution of observables is governed by the unconstrained Hamiltonian that coincides with the Hamiltonian describing the relative motion of particles in the integrable three-body hyperbolic Euler-Calogero-Sutherland system.
متن کاملStudy of a Restricted Modified Gravity on astrophysical and cosmological scales
p { margin-bottom: 0in; direction: rtl; text-align: right; }p.ctl { font-size: 12pt; }a:link { color: rgb(0, 0, 255); } In this paper, we study a restricted modified gravity in which diffeomorphism symmetry is broken. We investigate the astrophysical implications of the model by using the corresponding gravitational potential. By using the weight function of the weak lensing , for the model,...
متن کاملar X iv : g r - qc / 0 20 80 37 v 2 2 3 Se p 20 02 Bianchi type I cosmology and Euler - Calogero - Sutherland model
The Bianchi type I cosmological model is brought into a form where the evolution of observables is governed by the unconstrained Hamiltonian that coincides with the Hamiltonian describing the relative motion of particles in the integrable 3-body hyperbolic Euler-Calogero-Sutherland system.
متن کاملX iv : g r - qc / 0 20 80 37 v 1 1 4 A ug 2 00 2 Bianchi I cosmology and Euler - Calogero - Sutherland model
The Bianchi I cosmological model is brought into a form where the evolution of observables is governed by the unconstrained Hamiltonian that coincides with the Hamiltonian describing the relative motion of particles in the integrable 3-body hyperbolic Euler-Calogero-Sutherland system.
متن کاملShape Invariance in the Calogero and Calogero-Sutherland Models
We show that the Calogero and Calogero-Sutherland models possess an N -body generalization of shape invariance. We obtain the operator representation that gives rise to this result, and discuss the implications of this result, including the possibility of solving these models using algebraic methods based on this shape invariance. Our representation gives us a natural way to construct supersymm...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2007