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Related papers: Matrix Strings, Compactification Scales and Hagedo…

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In these lecture notes I give a pedagogical introduction to the thermodynamics of ideal string gases. The computation of thermodynamic quantities in the canonical ensemble formalism will be shown in detail with explicit examples. Attention…

High Energy Physics - Theory · Physics 2014-12-08 Lihui Liu

We consider M(atrix) theory compactifications to seven dimensions with eight unbroken supersymmetries. We conjecture that both M(atrix) theory on K3 and Heterotic M(atrix) theory on T^3 are described by the same 5+1 dimensional theory with…

High Energy Physics - Theory · Physics 2016-08-25 Suresh Govindarajan

Compactification of Matrix Model on a Noncommutative torus is obtained from strings ending on D-branes with background B field. The BPS spectrum of the system and a novel SL(2,Z) symmetry are discussed.

High Energy Physics - Theory · Physics 2007-05-23 F. Ardalan

The appearance of space/time non-commutativity in theories of open strings with a constant non-diagonal background metric is considered. We show that, even if the space-time coordinates commute, when there is a metric with a time-space…

High Energy Physics - Theory · Physics 2015-06-26 G. De Risi , G. Grignani , M. Orselli

According to the standard prescriptions, zero-temperature string theories can be extended to finite temperature by compactifying their time directions on a so-called "thermal circle" and implementing certain orbifold twists. However, the…

High Energy Physics - Theory · Physics 2015-06-05 Keith R. Dienes , Michael Lennek , Menika Sharma

String theory is the prime candidate for the theory of everything. However, it must be defined in ten dimensions to be consistent. To get 4D physics, the 6 other dimensions should be curled up in a small compact manifold, this procedure is…

High Energy Physics - Theory · Physics 2022-11-02 Poula Tadros , Iiro Vilja

In string theory, black holes are expected to transition into string stars as their Hawking temperatures approach the Hagedorn temperature. We study string stars and their phase transitions in the Euclidean spacetime…

High Energy Physics - Theory · Physics 2025-04-30 Jinwei Chu

We propose a Matrix Theory approach to Romans' massive Type IIA supergravity. It is obtained by applying the procedure of Matrix Theory compactifications to Hull's proposal of the Massive Type IIA String Theory as M-Theory on a twisted…

High Energy Physics - Theory · Physics 2010-04-05 David A. Lowe , Horatiu Nastase , Sanjaye Ramgoolam

We propose examples, which involve orbifolds by elements of the U-duality group, with M-theory moduli fixed at the eleven-dimensional Planck scale. We begin by reviewing asymmetric orbifold constructions in perturbative string theory, which…

High Energy Physics - Theory · Physics 2007-05-23 Michael Dine , Eva Silverstein

We derive the free energies of both the closed heterotic, and the unoriented, open and closed, type I string ensembles, consistent with the thermal (Euclidean T-duality) transformations on the String/M Duality Web. A crucial role is played…

High Energy Physics - Theory · Physics 2007-05-23 Shyamoli Chaudhuri

Two classes of stringy instanton effects, stronger than standard field theory instantons, are identified in the heterotic string theory. These contributions are established using type IIA/heterotic and type I/heterotic dualities. They…

High Energy Physics - Theory · Physics 2009-10-30 Eva Silverstein

We investigate thermodynamical properties of four and five dimensional black hole solutions of toroidally compactified string theory. We derive an analog of Smarr's formula and verify it directly using the metric.

General Relativity and Quantum Cosmology · Physics 2007-05-23 Emre Sermutlu

In this thesis, we explore two approaches to string phenomenology. In the first half of the work, we investigate M-theory compactifications on spaces with co-dimension four, orbifold singularities. We construct M-theory on C^2/Z_N by…

High Energy Physics - Theory · Physics 2008-08-28 Lara B. Anderson

The past year has seen enormous progress in string theory. It has become clear that all of the different string theories are different limits of a single theory. Moreover, in certain limits, one obtains a new, eleven-dimensional structure…

High Energy Physics - Theory · Physics 2007-05-23 Michael Dine

We consider closed type II and orientifold backgrounds where supersymmetry is spontaneously broken by asymmetric geometrical fluxes. We show that these can be used to describe thermal ensembles with chemical potentials associated to…

High Energy Physics - Theory · Physics 2008-12-18 C. Angelantonj , C. Kounnas , H. Partouche , N. Toumbas

A system H with a Hagedorn-like mass spectrum imparts its unique temperature TH to any other system coupled to it. An H system radiates particles in preexisting physical and chemical equilibrium. These particles form a saturated vapor at…

Nuclear Theory · Physics 2009-11-11 L. G. Moretto , K. A. Bugaev , J. B. Elliott , L. Phair

We study the correspondence between the linear matrix model and the interacting nonlinear string theory. Starting from the simple matrix harmonic oscillator states, we derive in a direct way scattering amplitudes of 2-dimensional strings,…

High Energy Physics - Theory · Physics 2007-05-23 A. Jevicki , J. P. Rodrigues , A. J. van Tonder

High energy fixed angle scattering is studied in matrix string theory. The saddle point world sheet configurations, which give the dominant contributions to the string theory amplitude, are taken as classical backgrounds in matrix string…

High Energy Physics - Theory · Physics 2009-10-31 Thomas Wynter

We use the quantum spectral curve to compute the Hagedorn temperature for ABJM theory in terms of the interpolating function $h(\lambda)$. At weak coupling we compute this temperature up to eight-loop order, showing that it matches the…

High Energy Physics - Theory · Physics 2023-07-14 Simon Ekhammar , Joseph A. Minahan , Charles Thull

In this paper, we discuss several explicit examples of the results obtained in JHEP 1402 (2014) 127. We elaborate on the random walk picture in these spacetimes and how it is modified. Firstly we discuss the linear dilaton background. Then…

High Energy Physics - Theory · Physics 2014-12-04 Thomas G. Mertens , Henri Verschelde , Valentin I. Zakharov