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相关论文: Cosmic Strings in an Open Universe: Quantitative E…

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We provide a general overview of the velocity-dependent one-scale model for cosmic string evolution and discuss two further extensions to it. We introduce and justify a new ansatz for the momentum parameter $k$, and also incorporate the…

高能物理 - 唯象学 · 物理学 2014-11-17 C. J. A. P. Martins , E. P. S. Shellard

We set up and analyse a model for the non-equilibrium evolution of a network of cosmic strings initially containing only loops and no infinite strings. Due to this particular initial condition, our analytical approach differs significantly…

高能物理 - 唯象学 · 物理学 2009-10-31 E. J. Copeland , T. W. B. Kibble , D. A. Steer

Previously developed analytic models for the evolution of cosmic string and monopole networks are applied to networks of monopoles attached to two or more strings; the former case is usually known as cosmic necklaces. These networks are a…

高能物理 - 唯象学 · 物理学 2014-11-21 C. J. A. P. Martins

In the present work we discuss inflation, dark matter and cosmological evolution in the context of the brane-world scenario. Being string theory inspired, the brane-world models provide corrections to the General Relativity, which is…

高能物理 - 唯象学 · 物理学 2012-05-28 G. Panotopoulos

The string-dominated universe locally resembles an open universe, and fits dynamical measures of power spectra, cluster abundances, redshift distortions, lensing constraints, luminosity and angular diameter distance relations and microwave…

天体物理学 · 物理学 2009-10-28 David Spergel , Ue-Li Pen

In the inflationary scenarios suggested by string theory, the vacuum fluctuations of the electromagnetic field can be amplified by the time-evolution of the dilaton background, and can grow large enough to explain both the origin of the…

天体物理学 · 物理学 2010-01-06 M. Gasperini , M. Giovannini , G. Veneziano

We analyze all individual cosmic strings of various lengths in a large ensemble of the global cosmic string networks in the post-inflationary scenario, obtained from numerical simulations on a discrete lattice with $N^3 = 4096^3$. A strong…

高能物理 - 唯象学 · 物理学 2025-09-19 Heejoo Kim , Minho Son

The role of anisotropic components on the dark energy and the dynamics of the universe is investigated. An anisotropic dark energy fluid with different pressures along different spatial directions is assumed to incorporate the effect of…

综合物理 · 物理学 2018-04-16 B. Mishra , S. K. Tripathy , Pratik P Ray

We study the behaviour and consequences of cosmic string networks in contracting universes. They approximately behave during the collapse phase as a radiation fluids. Scaling solutions describing this are derived and tested against…

天体物理学 · 物理学 2015-06-24 P. P. Avelino , C. J. A. P. Martins , C. Santos , E. P. S. Shellard

We study the behaviour of cosmic string networks in contracting universes, and discuss some of their possible consequences. We note that there is a fundamental time asymmetry between defect network evolution for an expanding universe and a…

天体物理学 · 物理学 2009-11-07 P. P. Avelino , C. J. A. P. Martins , C. Santos , E. P. S. Shellard

In the present work we discuss cosmic strings in natural inflation. Our analysis is based entirely on the CMB quadrupole temperature anisotropy and on the existing upper bound on the cosmic string tension. Our results show that the allowed…

高能物理 - 唯象学 · 物理学 2010-10-27 Grigoris Panotopoulos

Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In models which admit strings, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the…

宇宙学与河外天体物理 · 物理学 2015-06-12 Robert H. Brandenberger

We compare the anisotropies in the cosmic microwave background radiation measured by the COBE experiment to the predictions of cosmic strings. We use an analytic model for the $\Delta T/T$ power spectrum that is based on our previous…

高能物理 - 唯象学 · 物理学 2009-10-22 David P. Bennett , Albert Stebbins , Francois R. Bouchet

The evolution of cosmic string networks is an interesting dynamical problem. The equations governing these networks are classical and fully specified, but the length scale at which cosmic string loops form has been uncertain to tens of…

天体物理学 · 物理学 2009-06-23 Joseph Polchinski

We briefly review certain aspects of cosmic microwave background anisotropies as generated in passive and active models of structure formation. We then focus on cosmic strings based models and discuss their status in the light of current…

天体物理学 · 物理学 2009-11-07 Alejandro Gangui , Levon Pogosian , Serge Winitzki

We use Nambu-Goto numerical simulations to compute the cosmic microwave background (CMB) temperature anisotropies induced at arcminute angular scales by a network of cosmic strings in a Friedmann-Lemaitre-Robertson-Walker (FLRW) expanding…

天体物理学 · 物理学 2008-11-26 Aurélien A. Fraisse , Christophe Ringeval , David N. Spergel , François R. Bouchet

We consider the propagation of classical and quantum strings on cosmological space-times which interpolate from a collapsing phase to an expanding phase. We begin by considering the classical propagation of strings on space-times with…

高能物理 - 理论 · 物理学 2009-11-11 Andrew J. Tolley

This is a pedagogical introduction to the basics of the cosmic string theory and also a review of the recent progress made with respect to the macrophysical predictions of the theory. Topics covered include, string formation and evolution,…

天体物理学 · 物理学 2009-09-25 L. Perivolaropoulos

We study the impact of kinks on the cosmic microwave background (CMB) anisotropies generated by cosmic string networks. To do so, we extend the Unconnected Segment Model to describe the stress-energy tensor of a network of cosmic strings…

宇宙学与河外天体物理 · 物理学 2023-08-02 Rodrigo P. Silva , Lara Sousa , Ivan Yu. Rybak

We compute maps of CMB temperature fluctuations seeded by cosmic strings using high resolution simulations of cosmic strings in a Friedmann-Robertson-Walker universe. We create full-sky, 18-degree and 3-degree CMB maps, including the…

宇宙学与河外天体物理 · 物理学 2011-02-23 M. Landriau , E. P. S. Shellard