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1. Winds and Disk Turbulence Exert Equal Torques on Thick Magnetically Arrested Disks

   https://doi.org/10.3847/1538-4357/ad323d  

   Manikantan, Vikram; Kaaz, Nicholas; Jacquemin-Ide, Jonatan; Musoke, Gibwa; Chatterjee, Koushik; Liska, Matthew; Tchekhovskoy, Alexander (April 2024, The Astrophysical Journal)

   Abstract The conventional accretion disk lore is that magnetized turbulence is the principal angular momentum transport process that drives accretion. However, when dynamically important large-scale magnetic fields thread an accretion disk, they can produce mass and angular momentum outflows, known as winds,that also drive accretion. Yet, the relative importance of turbulent and wind-driven angular momentum transport is still poorly understood. To probe this question, we analyze a long-duration (1.2 × 10⁵r_g/c) simulation of a rapidly rotating (a= 0.9) black hole feeding from a thick (H/r∼ 0.3), adiabatic, magnetically arrested disk (MAD), whose dynamically important magnetic field regulates mass inflow and drives both uncollimated and collimated outflows (i.e., winds and jets, respectively). By carefully disentangling the various angular momentum transport processes within the system, we demonstrate the novel result that disk winds and disk turbulence both extract roughly equal amounts of angular momentum from the disk. We find cumulative angular momentum and mass accretion outflow rates of $\dot{L}\propto r^{0.9}$and $\dot{M}\propto r^{0.4}$, respectively. This result suggests that understanding both turbulent and laminar stresses is key to understanding the evolution of systems where geometrically thick MADs can occur, such as the hard state of X-ray binaries, low-luminosity active galactic nuclei, some tidal disruption events, and possibly gamma-ray bursts. 

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2. The Physical Properties of Low-redshift FeLoBAL Quasars. I. Spectral-synthesis Analysis of the Broad Absorption-line (BAL) Outflows Using SimBAL

   https://doi.org/10.3847/1538-4357/ac61d9  

   Choi 최, Hyunseop 현섭; Leighly, Karen M.; Terndrup, Donald M.; Dabbieri, Collin; Gallagher, Sarah C.; Richards, Gordon T. (September 2022, The Astrophysical Journal)

   Abstract We present the first systematic study of 50 low-redshift (0.66 <z< 1.63) iron low-ionization broad absorption-line quasars (FeLoBALQs) usingSimBAL, which represents a more than five-fold increase in the number of FeLoBALQs with detailed absorption line spectral analyses. We found the outflows have a wide range of ionization parameters, $-4\lesssim \log U\lesssim 1.2$and densities, $2.8\lesssim \log n\lesssim 8\left[{\mathrm{cm}}^{-3}\right]$. The objects in our sample showed FeLoBAL gas located at a wide range of distances $0\lesssim \log R\lesssim 4.4$[pc], although we do not find any evidence for disk winds (withR≪ 0.01 pc) in our sample. The outflow strength primarily depends on the outflow velocity with faster outflows found in quasars that are luminous or that have flat or redder spectral energy distributions. We found that ∼18% of the FeLoBALQs in the sample have the significantly powerful outflows needed for quasar feedback. Eight objects showedoverlapping troughsin the spectra, and we identified elevenloitering outflowobjects, a new class of FeLoBALQs that are characterized by low outflow velocities and high column density winds located $\log R\lesssim 1$[pc] from the central engine. The FeLoBALs in loitering outflows objects do not show properties expected for radiatively driven winds, and these objects may represent a distinct population among FeLoBALQs. We discuss how the potential acceleration mechanisms and the origins of the FeLoBAL winds may differ for outflows at different locations in quasars. 

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3. Search for Neutrino Emission from Hard X-Ray AGN with IceCube

   https://doi.org/10.3847/1538-4357/ada94b  

   Abbasi, R; Ackermann, M; Adams, J; Agarwalla, S K; Aguilar, J A; Ahlers, M; Alameddine, JM; Amin, N M; Andeen, K; Argüelles, C; et al (March 2025, The Astrophysical Journal)

   Abstract Active galactic nuclei (AGN) are promising candidate sources of high-energy astrophysical neutrinos, since they provide environments rich in matter and photon targets where cosmic-ray interactions may lead to the production of gamma rays and neutrinos. We searched for high-energy neutrino emission from AGN using the Swift-BAT Spectroscopic Survey catalog of hard X-ray sources and 12 yr of IceCube muon track data. First, upon performing a stacked search, no significant emission was found. Second, we searched for neutrinos from a list of 43 candidate sources and found an excess from the direction of two sources, the Seyfert galaxies NGC 1068 and NGC 4151. We observed NGC 1068 at flux ${\varphi }_{{\nu }_{\mu }+{\overline{\nu }}_{\mu }}$= $4.02_{-1.52}^{+1.58}\times 10^{-11}$TeV⁻¹cm⁻²s⁻¹normalized at 1 TeV, with a power-law spectral indexγ= 3.10 ${}_{-0.22}^{+0.26}$, consistent with previous IceCube results. The observation of a neutrino excess from the direction of NGC 4151 is at a posttrial significance of 2.9σ. If interpreted as an astrophysical signal, the excess observed from NGC 4151 corresponds to a flux ${\varphi }_{{\nu }_{\mu }+{\overline{\nu }}_{\mu }}$= $1.51_{-0.81}^{+0.99}\times 10^{-11}$TeV⁻¹cm⁻²s⁻¹normalized at 1 TeV andγ= 2.83 ${}_{-0.28}^{+0.35}$. 

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4. Sobolev extension in a simple case

   https://doi.org/10.1515/ans-2023-0132  

   Drake, Marjorie; Fefferman, Charles; Ren, Kevin; Skorobogatova, Anna (April 2025, Advanced Nonlinear Studies)

   Abstract In this paper, we establish the existence of a bounded, linear extension operator $T:L^{2,p}\left(E\right)\to L^{2,p}\left({\mathbb{R}}^2\right)$$$T :{L}^{2,p}\left(E\right)\to {L}^{2,p}\left({\mathbb{R}}^{2}\right)$$when 1 <p< 2 andEis a finite subset of ${\mathbb{R}}^2$$${\mathbb{R}}^{2}$$contained in a line. 

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5. Morphology modification of LiNi0.5Co0.2Mn0.3O2 by incorporating cotton textiles in lithium-ion capacitors

   https://doi.org/10.3389/fbael.2024.1388494  

   Truong, Phat; Sun, Quanwen; Tang, Wei; He, Rong; Zhou, Meng; Luo, Hongmei (May 2024, Frontiers in Batteries and Electrochemistry)

   To address the alerting issue of energy demand, lithium-ion capacitors (LICs) have been widely studied as promising electrochemical energy storage devices, which can deliver higher energy density than supercapacitors (SCs), and have higher power density with longer cycling life than lithium-ion batteries (LIBs). In this work, the active material lithium nickel cobalt manganese oxide LiNi_0.5Co_0.2Mn_0.3O₂(NCM523) is grown on a cotton textile template and building a 3-dimensional (3D) integrity to improve capacitance and energy density of LICs by enhancing the interfacial ion-exchange process. With the 3D structure, the specific discharge capacitance is increased to 718.67 $F{g}^{-1}$at 0.1 $A{g}^{-1}$from that of non-textile NCM523 (265.97 $F{g}^{-1}$), and remains a high capacitance of 254.48 $F{g}^{-1}$at 10 $A{g}^{-1}$in the half-cell capacitors. In addition, the energy density can achieve up to 36.17 $Whk{g}^{-1}$at the power density of 1,200 $Wk{g}^{-1}$in the full-cell capacitor. The textile NCM can maintain an energy density of 28.26 $Whk{g}^{-1}$at the current density of 10 $A{g}^{-1}$and power density of 6,000 $Wk{g}^{-1}$. Our results present promising applications of electrodes with the 3D porous structure for high energy density LICs. 

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