2010
DOI: 10.1007/jhep11(2010)100
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High-energy string-brane scattering: leading eikonal and beyond

Abstract: We extend previous techniques for calculations of transplanckian-energy stringstring collisions to the high-energy scattering of massless closed strings from a stack of N Dp-branes in Minkowski spacetime. We show that an effective non-trivial metric emerges from the string scattering amplitudes by comparing them against the semiclassical dynamics of high-energy strings in the extremal p-brane background. By changing the energy, impact parameter and effective open string coupling λ = gN , we are able to explore… Show more

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Cited by 58 publications
(138 citation statements)
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“…There is also a string-size-corrected weak-gravity regime (corresponding to somewhat smaller impact parameters) in which tidal excitations of the incoming closed string become important or even dominant [4]. In this regime we are still able to provide an exactly unitary S-matrix, but unitarity now works in an enlarged Hilbert space containing excited closed strings besides the incoming one.…”
Section: Jhep03(2016)030mentioning
confidence: 99%
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“…There is also a string-size-corrected weak-gravity regime (corresponding to somewhat smaller impact parameters) in which tidal excitations of the incoming closed string become important or even dominant [4]. In this regime we are still able to provide an exactly unitary S-matrix, but unitarity now works in an enlarged Hilbert space containing excited closed strings besides the incoming one.…”
Section: Jhep03(2016)030mentioning
confidence: 99%
“…It can be simplified, however, under the assumption that R p , while comparable or even larger than b, is still smaller than the string length parameter l s , enhanced by a square root of the logarithm of the energy, as we will discuss in more detail in the rest of the paper. 1 When this is the case the eikonal resummation of the leading terms (in energy) of the higher-order string amplitudes [4,11,12] should give a correct representation of the dynamics for every value of the impact parameter, all the way down to b = 0. Although in this limit a geometric interpretation of the brane background is lacking, the dynamics of the string-brane system remains extremely rich and interesting.…”
Section: Jhep03(2016)030mentioning
confidence: 99%
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