1994
DOI: 10.1016/0550-3213(94)90458-8
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Scattering of macroscopic heterotic strings

Abstract: We show that macroscopic heterotic strings, formulated as strings which wind around a compact direction of finite but macroscopic extent, exhibit non-trivial scattering at low energies. This occurs at order velocity squared and may thus be described as geodesic motion on a moduli space with a non-trivial metric which we construct. Our result is in agreement with a direct calculation of the string scattering amplitude. 5/93

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Cited by 20 publications
(31 citation statements)
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“…Similar conclusion should apply also to the generalisations [20,21,22,23] of the FS model (2.13), in particular, to the following one (n = ±1) [12] …”
Section: Fundamental String Solutionmentioning
confidence: 86%
“…Similar conclusion should apply also to the generalisations [20,21,22,23] of the FS model (2.13), in particular, to the following one (n = ±1) [12] …”
Section: Fundamental String Solutionmentioning
confidence: 86%
“…Special cases of the model (6.2) include chiral plane waves (F = 1) and generalisations of the fundamental string solution, e.g., describing travelling waves along fundamental string, A i = 0, F −1 = 1 + M/r D−4 , K = K(u, x) (some of these solutions were originally found as the leading-order solutions of the string effective equations in [81,82,83,102]). In particular, in the u-independent spherically symmetric case K = a + b/r D−4 = a ′ + b ′ F −1 so that (redefining u and v) the action (6.2) can be put into the simple form…”
Section: Chiral Null Modelsmentioning
confidence: 99%
“…(2b) The extreme electric dilatonic (a = 1) D = 4 black hole [85,86] can be obtained [36] by dimensional reduction from a generalised D = 5 fundamental string model (found as a leading order solution in [83,102]) which is also an exact string solution [36,20].…”
Section: Exact D = 4 Extreme Black Hole Solutionsmentioning
confidence: 99%
“…Evidence in favor of the identification of elementary BPS states of heterotic strings with extremal black holes has been also obtained in scattering processes of these states in [8] and [9] (in [9], as well as in [10] such black holes are obtained by compactifying macroscopic strings [11]), and in scattering of massless scalar states from such BPS states in [12] (where the inelastic thresholds are also examined).…”
Section: Introductionmentioning
confidence: 99%