The Mystery of the Cosmological Constant
ثبت نشده
چکیده
W hat determines the struc ture of space and time in the universe? According to Ein stein's general theory of relativity, the geometric properties of space are related to the density of energy (and momentum) in the universe. To un derstand the structure of spacetime, therefore, we must identify potential ly relevant sources of energy and evaluate their contributions to the to tal energy (and momentum) density. The most obvious energy sources that come to mind are ordinary mat ter and radiation. A much less obvi ous source of energy that can have an enormous impact on the structure of the universe is empty space itself: the vacuum. The notion that the vacuum can be a source of energy may seem coun terintuitive. But present theories of elementary particles and forces not only allow for a nonzero vacuum en ergy density but also strongly sug gest that it should have a large value. Is the vacuum energy density really as large as these theories appear to suggest it is? The answer is most emphatically no. The geometric structure of the universe is extremely sensitive to the value of the vacuum energy density. So important is this value that a con stant proportional to the vacuum en ergy density has been defined. It is called the cosmological constant. If the vacuum energy density, or equivalently the cosmological con stant, were as large as theories of ele mentary particles suggest, the uni verse in which we live would be dra matically different, with properties we would find both bizarre and un settling. What has gone wrong with our theories? We do not know the an-
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 کاملSpacetimes admitting quasi-conformal curvature tensor
The object of the present paper is to study spacetimes admitting quasi-conformal curvature tensor. At first we prove that a quasi-conformally flat spacetime is Einstein and hence it is of constant curvature and the energy momentum tensor of such a spacetime satisfying Einstein's field equation with cosmological constant is covariant constant. Next, we prove that if the perfect flui...
متن کاملDark Energy: Mystery of the Millennium
Nearly seventy per cent of the energy density in the universe is unclustered and exerts negative pressure. This conclusion — now supported by numerous observations — poses the greatest challenge for theoretical physics today. I discuss this issue with special emphasis on the cosmological constant as the possible choice for the dark energy. Several curious features of a universe with a cosmologi...
متن کاملافت و خیزهای برداری حول جواب وسون
In Wesson's canonical model, the universe is assumed to be five dimensional (5D) empty space time. This model corresponds to a solution of the Einstein field equation in five dimensions which, from a four dimensional point of view, is equivalent to a universe with a positive cosmological constant. In this model, the fifth direction is perpendicular to the four dimensional space time and is not...
متن کاملجوابهای کیهانشناسی معادلات برانس- دیکی با ثابت کیهانشناسی
In this paper, the analytical solutions of Brans-Dicke (B-D) equations with cosmological constant are presented, in which the equation of state of the universe is P=mÙ° ρ , under the assumption φRn=c between the B-D field and the scale factor of the universe. The flat (K=0) Robertson- Walker metric has been considered for the metric of the universe. These solutions are rich in the sense that ...
متن کاملOn the mystery of the cosmic vacuum energy density
After a short history of the Λ-term it is explained why the (effective) cosmological constant is expected to obtain contributions from short-distance physics, corresponding to an energy at least as large as the Fermi scale. The actual tiny value of the cosmological constant by particle physics standards represents, therefore, one of the deepest mysteries of present-day fundamental physics. Rece...
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 2008