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1. Non-invertible symmetries in SN orbifold CFTs and holography

   https://doi.org/10.1007/JHEP09(2024)110  

   Gutperle, Michael; Li, Yan-Yan; Rathore, Dikshant; Roumpedakis, Konstantinos (September 2024, Journal of High Energy Physics)

   We study non-invertible defects in two-dimensionalS_Norbifold CFTs. We construct universal defects which do not depend on the details of the seed CFT and hence exist in any orbifold CFT. Additionally, we investigate non-universal defects arising from the topological defects of the seed CFT. We argue that there exist universal defects that are non-trivial in the large-Nlimit, making them relevant for the AdS₃/CFT₂correspondence. We then focus on AdS₃×S³×$$ {\mathcal{M}}_4 $$ $M_4$with one unit of NS-NS flux and propose an explicit realization of these defects on the worldsheet. 

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2. Non-planar corrections in ABJM theory from quantum M2 branes

   https://doi.org/10.1007/JHEP11(2024)056  

   Giombi, Simone; Kurlyand, Stefan A; Tseytlin, Arkady A (November 2024, Journal of High Energy Physics)

   A<sc>bstract</sc> The quantization of semiclassical strings in AdS spacetimes yields predictions for the strong-coupling behaviour of the scaling dimensions of the corresponding operators in the planar limit of the dual gauge theory. Finding non-planar corrections requires computing string loops (corresponding to torus and higher genus surfaces), which is a challenging task. It turns out that in the case of theU_k(N) ×U_−k(N) ABJM theory there is an alternative approach: one may semiclassically quantize M2 branes in AdS₄×S⁷/ℤ_kwhich are wrapped around the 11d circle of radius 1/k=λ/N. Such M2 branes are the M-theory generalization of the strings in AdS × CP³. In this work, we show that by expanding in large M2 brane tensionT₂~$$ \sqrt{kN} $$ $\sqrt{\mathrm{kN}}$for fixedk, followed by an expansion in largek, we can predict the largeλasymptotics of the non-planar corrections to the dimensions of the dual ABJM operators. As a specific example, we consider the M2 brane configuration that generalizes the long folded string with large spin in AdS₄, and compute the 1-loop correction to its energy. This calculation allows us to determine non-planar corrections to the universal scaling function or cusp anomalous dimension. We extend our analysis to the semiclassical M2 branes that generalize the “short” and “long” circular strings with two equal angular momenta in CP³. The “short” M2 brane corresponds to a dual operator whose dimension at strong coupling scales as ∆ ∼λ^1/4+ …, and we derive the leading non-planar correction to it. 

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3. Multiphase ISM in the z = 5.7 Hyperluminous Starburst SPT 0346–52

   https://doi.org/10.3847/1538-4357/ac58f9  

   Litke, Katrina C.; Marrone, Daniel P.; Aravena, Manuel; Béthermin, Matthieu; Chapman, Scott C.; Dong, Chenxing; Hayward, Christopher C.; Hill, Ryley; Jarugula, Sreevani; Malkan, Matthew A.; et al (April 2022, The Astrophysical Journal)

   Abstract With Σ_SFR∼ 4200M_⊙yr⁻¹kpc⁻², SPT 0346–52 (z= 5.7) is the most intensely star-forming galaxy discovered by the South Pole Telescope. In this paper, we expand on previous spatially resolved studies, using ALMA observations of dust continuum, [Nii] 205μm, [Cii] 158μm, [Oi] 146μm, and undetected [Nii] 122μm and [Oi] 63μm emission to study the multiphase interstellar medium (ISM) in SPT 0346–52. We use pixelated, visibility-based lens modeling to reconstruct the source-plane emission. We also model the source-plane emission using the photoionization codecloudyand find a supersolar metallicity system. We calculateT_dust= 48.3 K andλ_peak= 80μm and see line deficits in all five lines. The ionized gas is less dense than comparable galaxies, withn_e< 32 cm⁻³, while ∼20% of the [Cii] 158μm emission originates from the ionized phase of the ISM. We also calculate the masses of several phases of the ISM. We find that molecular gas dominates the mass of the ISM in SPT 0346–52, with the molecular gas mass ∼4× higher than the neutral atomic gas mass and ∼100× higher than the ionized gas mass. 

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4. Physical Conditions of the Ionized Superwind in NGC 253 with VLT/MUSE

   https://doi.org/10.3847/1538-4357/add738  

   Cronin, Serena A; Bolatto, Alberto D; Congiu, Enrico; Donaghue, Keaton; Kreckel, Kathryn; Leroy, Adam K; Levy, Rebecca C; Veilleux, Sylvain; Walter, Fabian; Nolasco, Lenin (July 2025, The Astrophysical Journal)

   Abstract We present an analysis of the Hα-emitting ionized gas in the warm phase of the NGC 253 outflow using integral field spectroscopy from the Multi Unit Spectroscopic Explorer. In each spaxel, we decompose Hα, [Nii], and [Sii] emission lines into a system of up to three Gaussian components, accounting for the velocity contributions due to the disk and both intercepted walls of an outflow cone. In the approaching southern lobe of the outflow, we find maximum deprojected outflow velocities down to ∼−500 km s⁻¹. Velocity gradients of this outflowing gas range from ∼−350 to −550 km s⁻¹kpc⁻¹with increasing distance from the nucleus. Additionally, [Nii]/Hαand [Sii]/Hαintegrated line ratios are suggestive of shocks as the dominant ionization source throughout the wind. Electron densities, inferred from the [Sii] doublet, peak at 2100 cm⁻³near the nucleus and reach ≲50 cm⁻³in the wind. Finally, at an uncertainty of 0.3 dex on the inferred mass of 4 × 10⁵M_⊙, the mass-outflow rate of the Hα-emitting gas in the southern outflow lobe is ∼0.4M_⊙yr⁻¹. This yields a mass-loading factor ofη ∼ 0.1 and a ∼2% starburst energy efficiency. 

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5. Scattering from (p, q)-strings in AdS5 × S5

   https://doi.org/10.1007/JHEP03(2025)181  

   Pufu, Silviu S; Rodriguez, Victor A; Wang, Yifan (March 2025, Journal of High Energy Physics)

   A<sc>bstract</sc> Motivated by understanding the scattering of gravitons and their superpartners from extended (p,q)-strings in type IIB string theory via AdS/CFT, we study an integrated two-point function of stress tensor multiplet operators in the presence of a half-BPS line defect in$$ \mathcal{N} $$ $N$= 4 SU(N) super-Yang-Mills theory. We determine this integrated correlator at the five lowest non-trivial orders in$$ 1/\sqrt{N} $$ $1/\sqrt{N}$at fixed Yang-Mills coupling andθangle. Our calculations are performed explicitly when the line defect is a Wilson line, in which case we find a finite number of perturbative contributions at each order in$$ 1/\sqrt{N} $$ $1/\sqrt{N}$, as well as instanton contributions. Using SL(2,ℤ) transformations, our results can also be applied to Wilson-’t Hooft line defects dual to extended (p,q)-strings in the bulk. We analyze features of these integrated correlators in the weak coupling expansion by comparing with open-closed amplitudes of type IIB string theory on AdS₅× S⁵, as well as in its flat space limit. We predict new higher-derivative interaction vertices on the D1-brane and, more generally, on (p,q)-strings. 

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