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Cosmic Strings and Quintessence

Duan Yi-Shi, Ren Ji-Rong and Yang Jie

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Using torsion two-form we present a new Lorentz gauge invariant U(1) topological field theory in Riemann–Cartan space–time manifold U4. By virtue of the decomposition theory of U(1) gauge potential and the phi-mapping topological current theory, it is proven that the U(1) complex scalar field phi(x) can be looked upon as the order parameter field in our Universe, and a set of zero points of phi(x) create the cosmic strings as the space–time defects in the early Universe. In the standard cosmology, this complex scalar order parameter field possesses negative pressure, provides an accelerating expansion of Universe, and be able to explain the inflation in the early Universe. Therefore this complex scalar field is not only the order parameter field created the cosmic strings in the early universe, but also reasonably behaves as the quintessence, the dark energy.


PACS

11.27.+d Extended classical solutions; cosmic strings, domain walls, texture

11.30.Cp Lorentz and Poincare invariance

98.80.Cq Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)

02.40.Pc General topology

95.35.+d Dark matter (stellar, interstellar, galactic, and cosmological)

Subjects

Mathematical physics

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 12 (December 2003)

Received 22 September 2003



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