The Self Creation Challenge to the Cosmological 'concordance Model'
نویسنده
چکیده
It is important to have viable alternatives against which standard theories may be tested. In this paper such an alternative to the standard cosmological 'concordance model' is examined. It is shown how the theory of Self Creation Cosmology is as concordant as the standard model with cosmological observations and local experiments. This is due to a degeneracy in the interpretation of the data. However, unlike the standard model, Self Creation Cosmology does not require the speculative hypotheses of inflation, dark matter or dark energy. The theory is highly predictive and when its only free parameter, H, is fixed empirically, all other cosmological constraints are then determined and are remarkably consistent with observations. It is highly testable and as such 'throws down the gauntlet' before General Relativity in the geodetic precession measurement that should be made by the Gravity Probe B satellite towards the middle of the year 2004. This will be the first physical experiment that has the capability of distinguishing between the two theories. The new theory predicts a geodetic precession of 5/6 of that of General Relativity, that is, Self Creation theory predicts a precession about a direction perpendicular to the plane of the orbit of 5.5 arc/sec/yr. The predictions of the 'frame dragging' precessions of that experiment are equal in both theories. Furthermore, there are also at least two other experiments that will distinguish between the two theories, which ask the questions, " Do photons fall at the same rate as particles? " and " Is there a cutoff to the Casimir force that approaches zero as curvature approaches flatness? " It is suggested that these experiments be performed at the earliest opportunity if the geodetic measurement should indeed prove to be consistent with the Self Creation theory.
منابع مشابه
Bulk Viscous Bianchi Type VI0 Cosmological Model in the Self-creation Theory of Gravitation and in the General Theory of Relativity
In the second self-creation theory of gravitation and in the general theory of relativity, Bianchi type VI0 cosmological model in the presence of viscous fluid is studied. An exact solution of the field equations is given by considering the cosmological model yields a constant decelerations parameter q=constant and the coefficients of the metric are taken as A(t)=[c1t+c<su...
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 کاملCo-Creation Intention; Presenting a Model of Antecedents and its Impact on Attitude Toward the Product (Case Study in Shatel Company)
Virtual co-creation is a tool which assists marketers in better recognizing customers’ needs and in increasing new products success rates. Despite the importance of co-creation in new product development, little empirical research is being conducted in order to clarify the concept. Studies are mostly company centric, overlooking consumer’s value perception of co-creation and how it affects his ...
متن کاملLocal Self-concordance of Barrier Functions Based on Kernel-functions
Many efficient interior-point methods (IPMs) are based on the use of a self-concordant barrier function for the domain of the problem that has to be solved. Recently, a wide class of new barrier functions has been introduced in which the functions are not self-concordant, but despite this fact give rise to efficient IPMs. Here, we introduce the notion of locally self-concordant barrier functio...
متن کاملBubble Cosmology : A concordant cosmological model ? ⋆
The Fractal Bubble model has been proposed as a viable cosmology that does not require dark energy to account for cosmic acceleration, but rather attributes its observational signature to the formation of structure. In this paper it is demonstrated that, in contrast to previous findings, this model is not a good fit to cosmological supernovae data; there is significant tension in the best fit p...
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 2004