Non Commutative Quantum Spacetime with Topological Vortex States, and Dark Matter in the Universe

نویسنده

  • Ajay Patwardhan
چکیده

X iv :g rqc /0 31 01 36 v1 3 1 O ct 2 00 3 Non commutative quantum spacetime with topological vortex states, and dark matter in the Universe Ajay Patwardhan Physics Department, St. Xavier’s college, Mahapalika Marg, Mumbai, 400001, India Abstract Non commutative geometry is creating new possibilities for physics. Quantum spacetime geometry and post inflationary models of the universe with matter creation have an enormous range of scales of time, distances and energy in between. There is a variety of physics possible till the nucleosynthesis epoch is reached. The use of topology and non commutative geometry in cosmology is a recent approach. This paper considers the possibility of topological solutions of a vortex kind given by non commutative structures. These are interpreted as dark matter, with the grand unified Yang-Mills field theory energy scale used to describe its properties. The relation of the model with other existing theories is discussed. Introduction The role of Geometry and Topology in understanding the physics of the universe of space time and matter has a century of work that is supported by observations. Inflationary cosmological models developed for creation of matter have included the small anisotropic distributions as given by COBE and WMAP observations. The models modified to create the voids and filamentary large scale structure of the early universe , with the ratios of dark energy, dark matter and normal matter are topics of active research. The non linear evolution equations of the early universe give rise to anisotropy and inhomogenity persisting at all length scales , these are observable with even finer resolution that is expected in subsequent experiments. These indicate analogies with condensed matter. Topological defects and vortex like states in rapid expansion and cooling occur in condensed matter phases. This paper develops the role of noncommutative geometry in the formation of the vortex like topological states. The typical model of the universe, a few seconds old and a few kilometers in size, is expected to have some 10 particles of normal matter, and to form a smooth geometry given by Einstein’s theory of general relativity ; with 10 parts fluctuation in matter distribution as inferred from the temperature and thermal radiation microwave measurements. [References]. The models of the early universe In the inflation models and their variations that give the later stage expanding universe models with the correct observed properties, there are topologically non trivial states possible. A rubber sheet or expanding balloon

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

From a Dual Einstein-Kaluza Spacetime to ‘tHooft Renormalon and the Reality of Accelerated Cosmic Expansion

We use a dual Einstein-Kaluza spacetime to calculate the exact energy density of dark energy and dark matter using a novel topological computation method. Starting from the said spacetime and ‘tHooft’s topological renormalon as well as the corresponding symmetry group, we show how the zero set quantum particle and the empty set quantum wave interact with the vacuum and give rise to pure dark en...

متن کامل

Numerical analysis of the dynamics of a cosmic string loop as a vortex

Time evolution of a circular cosmic string loop is investigated by numerically solving the field equations for the scalar and the gauge fields consisting of the vortex. It is shown that the result agrees with an analytic estimate based on the Nambu-Goto action, which supports its validity in analyzing nonstraight and rapidly moving strings. The cosmic string scenario is one of the major propose...

متن کامل

Formation of Large Structures in the Acceleration Universe with a Hybrid Expansion Law

In the current paper, we have studied the effect of dark energy on for-mation where dark energy exists in the background. For this purpose, we used both WMAP9 and Planck data to study how the radius changes with redshift in these mod-els. We used different data sets to fix the cosmological parameters to obtain a solution for a spherical region under collapse. The mechanism of structure formation f...

متن کامل

Effects related to spacetime foam in astrophysics

During the quantum stage, spacetime had the foam-like structure. When the Universe cools down, the foam structure tempers and does not disappear, therefore the Friedman model represents only an idealization. We show that the large scale observational effects of the foamed structure appear as the Dark Matter and Dark Energy phenomena. We also examine the scattering of free particles on the foam-...

متن کامل

ar X iv : 0 90 4 . 45 54 v 1 [ gr - q c ] 2 9 A pr 2 00 9 Island Cosmology

If the observed dark energy is a cosmological constant, the canonical state of the universe is de Sitter spacetime. In such a spacetime, quantum fluctuations that violate the null energy condition will create islands of matter. If the fluctuation is sufficiently large, the island may resemble our observable universe. Phenomenological approaches to calculating density fluctuations yield a scale ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2003