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Related papers: The Complete Spectrum of the $W_N$ String

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String configurations with nonzero winding number describe soliton string states. We compute the Veneziano amplitude for the scattering of arbitrary winding states and show that in the large radius limit the strings always scatter trivially…

High Energy Physics - Theory · Physics 2009-10-22 Ramzi R. Khuri

An $(n, 1)$ string is a bound state of a D-string and $n$ fundamental strings. It may be described by a D-string with a world volume electric field turned on. As the electric field approaches its critical value, $n$ becomes large. We…

High Energy Physics - Theory · Physics 2008-11-26 S. Gukov , I. R. Klebanov , A. M. Polyakov

Exact superstring solutions are constructed in 4-D space-time, with positive curvature and non-trivial dilaton and antisymmetric tensor fields. The full spectrum of string excitations is derived as a function of moduli fields $T^{i}$ and…

High Energy Physics - Theory · Physics 2016-09-06 Elias Kiritsis , Costas Kounnas

N=2 heterotic strings may provide a window into the physics of M-theory radically different than that found via the other supersymmetric string theories. In addition to their supersymmetric structure, these strings carry a four-dimensional…

High Energy Physics - Theory · Physics 2007-05-23 Emil Martinec

The manifestly SU(4)xU(1) super-Poincare invariant free-field N=2 twistor- string action for the ten-dimensional Green-Schwarz superstring is quantized using standard BRST methods. Unlike the light-cone and semi-light-cone gauge-fixed…

High Energy Physics - Theory · Physics 2009-10-22 Nathan Berkovits

We propose an instrinsic worldsheet description of the ultra-high energy regime of string scattering based on worldsheet symmetries. At very high energies, the fundamental string becomes tensionless and in flat target spacetimes, the…

High Energy Physics - Theory · Physics 2026-03-31 Arjun Bagchi , Sachin Grover , Sharang Rajesh Iyer , Amartya Saha

This paper deals with a study of the cylindrically symmetric accretion of dark energy with equation of state $p=w\rho$ onto wiggly straight cosmic strings. We have obtained that when $w>-1$ the linear energy density in the string core…

Astrophysics · Physics 2009-11-13 Pedro F. Gonzalez-Diaz , Jose A. Jimenez Madrid

We use supersymmetric localization techniques to study the low-energy dynamics of BPS vortex-strings in four-dimensional N=2 theories. We focus on theories with SU(Nc)xU(1) gauge group and Nf hypermultiplets, all in the fundamental…

High Energy Physics - Theory · Physics 2018-08-14 Efrat Gerchkovitz , Avner Karasik

We consider scattering amplitudes in non-critical string theory of $N$ external states in the limit where the energy of all external states is large compared to the string tension. We argue that the amplitudes are naturally complex analytic…

High Energy Physics - Theory · Physics 2009-10-30 Kenichiro Aoki , Eric D'Hoker

Assemblies of interacting quantum particles often surprise us with properties that are difficult to predict. One of the simplest quantum many-body systems is the spin 1/2 Heisenberg antiferromagnetic chain, a linear array of interacting…

Strongly Correlated Electrons · Physics 2013-07-02 M. Mourigal , M. Enderle , A. Klöpperpieper , J. -S. Caux , A. Stunault , H. M. Rønnow

The action of tensionless spinning string invariant under reparametrizions, both local supersymmetry and dilatations, is considered. The density of energy-momentum tensor is constructed and vanishing of its covariant divergence is proved.…

High Energy Physics - Theory · Physics 2026-01-21 A. A/ Zheltukhin

We numerically solve the conjectured Quantum Spectral Curve for strings on AdS$_3\times$S$^3\times$T$^4$ with R--R charge from weak to strong coupling. At strong coupling, the spectrum organises into flat-space string mass levels with…

High Energy Physics - Theory · Physics 2026-03-31 Simon Ekhammar , Nikolay Gromov , Bogdan Stefański , Charles Thull

We explain how perturbative string theory can be viewed as an exactly renormalizable Weyl invariant quantum mechanics in the worldsheet representation clarifying why string scattering amplitudes are both finite and unambiguously normalized…

High Energy Physics - Theory · Physics 2009-11-07 Shyamoli Chaudhuri

We discuss the conditions under which the BRST operator of a $W$-string can be written as the sum of two operators that are separately nilpotent and anticommute with each other. We illustrate our results with the example of the non-critical…

High Energy Physics - Theory · Physics 2009-10-22 E. Bergshoeff , H. J. Boonstra , M. de Roo , S. Panda , A. Sevrin

We discuss new realisations of $W$ algebras in which the currents are expressed in terms of two arbitrary commuting energy-momentum tensors together with a set of free scalar fields. This contrasts with the previously-known realisations,…

High Energy Physics - Theory · Physics 2009-10-07 H. Lu , C. N. Pope , S. Schrans , X. J. Wang

Optically-trapped two-component Fermi gases near a broad Feshbach resonance exhibit universal thermodynamics, where the properties of the gas are independent of the details of the two-body scattering interactions. We present a global proof…

Statistical Mechanics · Physics 2008-03-12 J. E. Thomas

The oscillation spectrum of a perturbed neutron star is intimately related to the physical properties of the star, such as the equation of state. Observing pulsating neutron stars therefore allows one to place constraints on these physical…

High Energy Astrophysical Phenomena · Physics 2018-05-16 Arthur G Suvorov

The high-energy behavior of string scattering in warped spacetimes is studied to all orders in perturbation theory. If one assumes that the theory is finite, the amplitudes exactly fall as powers of momentum.

High Energy Physics - Theory · Physics 2009-11-10 Oleg Andreev

Free bosonic strings in noncommutative spacetime are investigated. The string spectrum is obtained in terms of light-cone quantization. We construct two different models. In the first model the critical dimension is still required to be 26…

High Energy Physics - Theory · Physics 2007-05-23 Xiao-Jun Wang

In the Unitarity Limit, the NN S-wave binding energies are zero, the scattering lengths infinite, Physics is universal, i.e. insensitive to details of the interactions, and observables display richer symmetries, namely invariance under both…

Nuclear Theory · Physics 2025-05-19 Harald W. Griesshammer