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相关论文: Genericity of Cosmic Strings Formation in SUSY GUT…

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Supersymmetry breaking in string theory is expected to occur when moduli fields acquire non-trivial expectation values. In the early universe these fields start out displaced from their final destinations. I present some recent ideas about…

高能物理 - 理论 · 物理学 2007-05-23 R. Brustein

We give an upper estimate for the number of gamma ray bursts from ordinary (non-superconducting) cosmic strings expected to be observed at terrestrial detectors. Assuming that cusp annihilation is the mechanism responsible for the bursts we…

高能物理 - 唯象学 · 物理学 2016-09-01 R. H. Brandenberger , A. T. Sornborger , M. Trodden

Grand Unified Theories (GUT) predict proton decay as well as the formation of cosmic strings which can generate gravitational waves. We determine which non-supersymmetric $SO(10)$ breaking chains provide gauge unification in addition to a…

高能物理 - 唯象学 · 物理学 2021-11-05 Stephen F. King , Silvia Pascoli , Jessica Turner , Ye-Ling Zhou

The predictions of the inflationary LCDM paradigm match today's high-precision measurements of the cosmic microwave background anisotropy extremely well. The same data put tight limits on other sources of anisotropy. Cosmic strings are a…

宇宙学与河外天体物理 · 物理学 2013-05-29 Cora Dvorkin , Mark Wyman , Wayne Hu

We propose an alternative scenario to cosmic inflation for producing the initial seeds of cosmic structures. The cosmological fluctuations are generated by thermal fluctuation of the energy density of the ideal string gas in three compact…

高能物理 - 理论 · 物理学 2007-05-23 Ali Nayeri

It is tempting to inflate along one of the many flat directions that arise in supersymmetric theories. The required flatness of the potential to obtain sufficient inflation and to not overproduce density fluctuations occurs naturally.…

高能物理 - 唯象学 · 物理学 2009-10-28 Katherine Freese , Tony Gherghetta , Hideyuki Umeda

A class of finite GUTs in curved spacetime is considered in connection with the cosmological inflation scenario. It is confirmed that the use of the running scalar-gravitational coupling constant in these models helps realizing a successful…

高能物理 - 唯象学 · 物理学 2019-08-15 Seiji Mukaigawa , Taizo Muta , Sergei D. Odintsov

Cosmic strings provide a radically different paradigm for the formation of structure to the prevailing inflationary one. They afford some extra technical complications: for example, the calculation of the power spectrum of matter and…

天体物理学 · 物理学 2007-05-23 Mark Hindmarsh , Mairi Sakellariadou , Graham R. Vincent

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

Inflation of cosmic gauge and global strings is investigated by numerically solving the combined Einstein and field equations. Above some critical symmetry-breaking scales, the strings undergo inflation along the radial direction as well as…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Inyong Cho

We consider F and D-term cosmic strings formed in supersymmetric theories. Supersymmetry is broken inside the string core, but restored outside. In global SUSY, this implies the existence of goldstino zero modes, and the string potentially…

高能物理 - 唯象学 · 物理学 2008-11-26 Rachel Jeannerot , Marieke Postma

A network of cosmic strings (CS), if present, would continue emitting gravitational waves (GW) as it evolves throughout the history of the Universe. This results in a characteristic broad spectrum making it a perfect source to infer the…

宇宙学与河外天体物理 · 物理学 2023-09-12 Francesc Ferrer , Anish Ghoshal , Marek Lewicki

It has recently been shown that a Hagedorn phase of string gas cosmology may provide a causal mechanism for generating a nearly scale-invariant spectrum of scalar metric fluctuations, without the need for an intervening period of de Sitter…

高能物理 - 理论 · 物理学 2008-11-26 Robert H. Brandenberger , Ali Nayeri , Subodh P. Patil , Cumrun Vafa

The cosmic string theory for cosmological fluctuations is a good example of healthy scientific progress in cosmology. It is a well defined physically motivated model that has been tested by cosmological observations and has been ruled out…

天体物理学 · 物理学 2009-11-10 L. Perivolaropoulos

We study in detail the structure of Grand Unified Theories derived as the low-energy limit of orbifold four-dimensional strings. To this aim, new techniques for building level-two symmetric orbifold theories are presented. New classes of…

高能物理 - 理论 · 物理学 2009-10-09 G. Aldazabal , A. Font , L. E. Ibanez , A. M. Uranga

We explore the formation of cosmic string Y-junctions when strings of two different types collide, which has recently become important since string theory can yield cosmic strings of distinct types. Using a model containing two types of…

高能物理 - 理论 · 物理学 2008-11-26 Neil Bevis , Paul M. Saffin

Cosmic strings can be created in the early universe during symmetry-breaking phase transitions, such as might arise if the gauge structure of the standard model is extended by additional U(1) factors at high energies. Cosmic strings present…

高能物理 - 唯象学 · 物理学 2009-10-29 Yanou Cui , David E. Morrissey

Cosmic strings are generic cosmological predictions of many extensions of the Standard Model of particle physics, such as a $U(1)^\prime$ symmetry breaking phase transition in the early universe or remnants of superstring theory. Unlike…

高能物理 - 唯象学 · 物理学 2018-06-13 Yanou Cui , Marek Lewicki , David E. Morrissey , James D. Wells

In string theory, the traditional picture of a Universe that emerges from the inflation of a very small and highly curved space-time patch is a possibility, not a necessity: quite different initial conditions are possible, and not…

高能物理 - 理论 · 物理学 2017-06-01 M. Gasperini , G. Veneziano

The cosmic string scenario in an open universe is developed -- including the equations of motion, a model of network evolution, the large angular scale CMB temperature anisotropy, and the power spectrum of density fluctuations produced by…

天体物理学 · 物理学 2009-10-30 P. P. Avelino , R. R. Caldwell , C. J. A. P. Martins