Abstract:We derive the energy of pulsating string, as function of oscillation number and angular momenta, which oscillates in AdS 3 with an extra angular momentum along S 1 . We find similar solutions for the strings oscillating in S 3 in addition to extra angular momentum. Further we generalize the result of the oscillating strings in Anti de-Sitter space in the presence of both spin and angular momentum in AdS 5 × S 1 .
“…After putting κ = 0, we can get the energy for the short string which oscillates near the center of AdS 3 with an angular momentum in S 1 in undeformed AdS 3 × S 1 as computed in [55]. With both κ and angular momentum as zero we can get back the energy expression for the strings oscillating in one plane for small energy limit as in the [47].…”
Section: Jhep03(2015)010mentioning
confidence: 98%
“…Here we wish to study pulsating string solution in the sub sectors of the deformed background as they are more stable than rotating ones [37]. After the inception of the pulsating string in [38], they have been studied both in AdS and non-AdS background [39][40][41][42][43][44][45][46][47][48][49][50][51][52][53][54][55][56].…”
Abstract:We derive the energy of pulsating strings as a function of adiabatic invariant oscillation number, which oscillates in S 2 κ . We find similar solutions for the strings oscillating in deformed AdS 3 . Furthermore, we generalize the result of the oscillating strings in anti-de Sitter space in the presence of extra angular momentum in (AdS 3 × S 1 ) κ .
“…After putting κ = 0, we can get the energy for the short string which oscillates near the center of AdS 3 with an angular momentum in S 1 in undeformed AdS 3 × S 1 as computed in [55]. With both κ and angular momentum as zero we can get back the energy expression for the strings oscillating in one plane for small energy limit as in the [47].…”
Section: Jhep03(2015)010mentioning
confidence: 98%
“…Here we wish to study pulsating string solution in the sub sectors of the deformed background as they are more stable than rotating ones [37]. After the inception of the pulsating string in [38], they have been studied both in AdS and non-AdS background [39][40][41][42][43][44][45][46][47][48][49][50][51][52][53][54][55][56].…”
Abstract:We derive the energy of pulsating strings as a function of adiabatic invariant oscillation number, which oscillates in S 2 κ . We find similar solutions for the strings oscillating in deformed AdS 3 . Furthermore, we generalize the result of the oscillating strings in anti-de Sitter space in the presence of extra angular momentum in (AdS 3 × S 1 ) κ .
“…It is obvious that the presence of flux in the background does not affect the conserved charges in the case of a pulsating string. Now expressing the Virasoro constraint(4.9) in terms of E = E √ 2λ and J a = Ja √ 2λ , the oscillation number can be written as [41]…”
Section: String Profile and Conserved Chargesmentioning
Neumann-Rosochatius system is a well known one dimensional integrable system. We study the rotating and pulsating string in AdS 4 × CP 3 with a B NS holonomy turned on over CP 1 ⊂ CP 3 , the so called Aharony-Bergman-Jafferis (ABJ) background. We observe that the string equations of motion in both cases are integrable and the Lagrangians reduce to a form similar to that of a deformed Neumann-Rosochatius system. We find out the scaling relations among various conserved charges and comment on the finite size effect for the dyonic giant magnons on R t × CP 3 with two angular momenta. For the pulsating string we derive the energy as function of oscillation number and angular momenta along CP 3 .
“…In this case it has the most unusual form, 27) Which is a completely new scaling for such long strings and does not reduce to the usual form of oscillation number for AdS strings. The constant a 1 = 0.1516.…”
Section: Semiclassical Quantization and 'Long' String Solutionmentioning
Abstract:The so called one-parameter (often called κ) deformed AdS string sigma models have attracted a lot of attention lately in the study of integrability in string theory. We construct various circular string solutions in the (AdS 3 ×S 3 ) κ background and describe the characteristics of such solutions qualitatively. We study the Bohr-Sommerfeld like quantization for these string states to characterise the motion. Further we find a 'long' string limit of such circular strings in the κ-deformed AdS 3 and find a novel dependence of the oscillation number on the energy in the next to leading order expansion.
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