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We analyse the world-volume theory of multiple Kaluza-Klein monopoles in string and M-theory by identifying the appropriate zero modes of various fields. The results are consistent with supersymmetry, and all conjectured duality symmetries.…

High Energy Physics - Theory · Physics 2008-11-26 Ashoke Sen

The Kaluza-Klein (KK) modes of graviton are studied in the IIB superstring compactification where the warped geometry is realized at the Klebanov-Strassler (KS) throat. Knowledge of the metric of the KS throat enables us to determine their…

High Energy Physics - Theory · Physics 2008-11-26 Tatsuya Noguchi , Masahiro Yamaguchi , Masakazu Yamashita

We show that a cosmic string associated with spontaneous $U(1)_R$ symmetry breaking gives a constraint for supersymmetric model building. In some models, the string can be viewed as a tube-like domain wall with a winding number…

High Energy Physics - Theory · Physics 2015-06-12 Minoru Eto , Yuta Hamada , Kohei Kamada , Tatsuo Kobayashi , Keisuke Ohashi , Yutaka Ookouchi

We consider a 2-parameter class of solvable closed superstring models which `interpolate' between Kaluza-Klein and dilatonic Melvin magnetic flux tube backgrounds. The spectrum of string states has similarities with Landau spectrum for a…

High Energy Physics - Theory · Physics 2009-09-17 A. A. Tseytlin

Towards the end of the brane inflationary epoch in the brane world, cosmic strings (but not texture, domain walls or monopoles) are copiously produced during brane collision. These cosmic strings are D$p$-branes with $(p-1)$ dimensions…

High Energy Physics - Theory · Physics 2009-11-07 Saswat Sarangi , S. -H. Henry Tye

Gravitational wave signatures from cosmic strings are analyzed numerically. Cosmic string networks form during phase transistions in the early universe and these networks of long cosmic strings break into loops that radiate energy in the…

General Relativity and Quantum Cosmology · Physics 2009-09-30 Matthew R Depies

We study the evolution of cosmic strings taking into account the frictional force due to the surrounding radiation. We consider small perturbations on straight strings, oscillation of circular loops and small perturbations on circular…

High Energy Physics - Theory · Physics 2009-10-22 J. Garriga , M. Sakellariadou

I report on recent numerical simulations of the simplest field theory with cosmic string solutions, the Abelian Higgs model. We find that random networks of string quickly converge to a scaling solution in which the network scale length…

High Energy Physics - Phenomenology · Physics 2016-10-26 Mark Hindmarsh

Chiral cosmic strings are produced naturally at the end of inflation in supersymmetric models where the symmetry is broken via a D-term. Consequently in such theories, where both inflation and cosmic strings contribute to the density and…

Astrophysics · Physics 2009-10-31 A. C. Davis , T. W. B. Kibble , M. Pickles , D. A. Steer

The origin and nature of ultrahigh-energy cosmic ray events, above the Greisen-Zatsepin-Kuzmin (GZK) cutoff energy, constitute a long-standing, unsolved mistery. Neutrinos are proposed candidates but their standard interactions with matter…

High Energy Physics - Phenomenology · Physics 2007-05-23 Jose I. Illana

In the early Universe, as a consequence of $U(1)_{B-L}$ gauge symmetry-breaking, the so-called $B-L$ cosmic strings are expected to be produced at the breaking scale $\eta_{B-L}$ according to the Kibble mechanism. The decaying, collapsing…

High Energy Physics - Phenomenology · Physics 2009-11-11 Pei-Hong Gu , Hong Mao

Recent work suggests that fundamental and Dirichlet strings, and their (p,q) bound states, may be observed as cosmic strings. The evolution of cosmic string networks, and therefore their observational signals, depends on what happens when…

High Energy Physics - Theory · Physics 2009-11-10 Mark G. Jackson , Nicholas T. Jones , Joseph Polchinski

We include the effect of the frictional force caused by interactions between cosmic strings and the particles of the background plasma in the computation of the stochastic gravitational wave background generated by cosmic string loops.…

Cosmology and Nongalactic Astrophysics · Physics 2024-04-23 S. Mukovnikov , L. Sousa

The Kaluza-Klein (KK) modes of a massive scalar field on a 3-brane embedded in six dimensional multiply warped spacetime are determined. Due to the presence of warping along both the extra dimensions the KK mass spectrum splits into two…

High Energy Physics - Theory · Physics 2010-11-10 Ratna Koley , Joydip Mitra , Soumitra SenGupta

Cosmic strings are generically predicted in many extensions of the Standard Model of particle physics. We propose a new avenue for detecting cosmic strings through their effect on the filamentary structure in the cosmic web. Using…

Cosmology and Nongalactic Astrophysics · Physics 2020-08-11 M. A. Fernandez , Simeon Bird , Yanou Cui

We propose a mechanism for the generation of temperature fluctuations of cosmic microwave background. We consider a large number of fields, such as Kaluza-Klein modes and string excitations. Each field contributes to the gravitational…

High Energy Physics - Theory · Physics 2015-05-27 Yoshinobu Habara , Hikaru Kawai , Masao Ninomiya , Yasuhiro Sekino

We review the existence, formation and properties of cosmic strings in string theory, the wide variety of observational techniques that are being employed to detect them, and the constraints that current observations impose on string theory…

High Energy Physics - Theory · Physics 2015-05-28 Edmund J. Copeland , Levon Pogosian , Tanmay Vachaspati

Perturbative breaking of supersymmetry in four-dimensional string theories predict in general the existence of new large dimensions at the TeV scale. Such large dimensions lie in a domain of energies accessible to particle accelerators.…

High Energy Physics - Phenomenology · Physics 2009-10-28 I. Antoniadis , K. Benakli , M. Quirós

We consider the cosmological consequences of a network of superconducting cosmic strings. For strong enough current the period of friction domination never ends. Instead a plasma scaling solution is reached. We demonstrate that this gives…

High Energy Physics - Phenomenology · Physics 2009-10-31 K. Dimopoulos , A. C. Davis

The flux of cosmic rays beyond the GZK cutoff ($\sim 10^{20}$ eV) may be explained through their production by ultra high energy cosmic neutrinos, annihilating on the relic neutrino background, in the vicinity of our galaxy. This process is…

High Energy Physics - Phenomenology · Physics 2009-10-31 H. Davoudiasl , J. L. Hewett , T. G. Rizzo