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1. Prethermalization and Thermalization in Isolated Quantum Systems

   https://doi.org/10.1103/PhysRevX.9.021027  

   Mallayya, Krishnanand; Rigol, Marcos; De Roeck, Wojciech (May 2019, Physical Review X)
2. Mass and Metal Flows in Isolated IllustrisTNG Halos

   https://doi.org/10.3847/1538-4357/addf46  

   Morgan, Jacob; Bailin, Jeremy; Anderson, Annelia (September 2025, The Astrophysical Journal)

   Abstract The circumgalactic medium (CGM) is a reservoir of metals and star-forming fuel. Most baryons in the Universe are in the CGM or the intergalactic medium (IGM). The baryon cycle—how mass and metals reach the CGM from the inner regions of the galaxy and how gas from the CGM replenishes star-forming activity in the inner regions—is an essential question in galaxy evolution. In this paper, we study the flow of mass and metals in a stacked sample of 2770 isolated halos from the IllustrisTNG100 cosmological hydrodynamic simulation. The mean gas flow as a function of radius and angle is similar across a large galactic mass range when accounting for different feedback modes. Although both star formation and black holes cause powerful outflows, the flows from star formation are more angularly restricted. Black hole feedback dominates mass flow throughout the halo, while star formation feedback mainly affects the inner region. When scaling by virial radius (R_v), large dynamical changes occur at 0.2R_vfor most halos, suggesting a characteristic size for the inner galaxy. Despite kinetic-mode feedback from black holes being the primary quenching mechanism in IllustrisTNG, a small population of high-mass kinetic-mode disks are able to form stars. 

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3. Tactile Telepresence for Isolated Patients

   https://doi.org/10.1109/ISMAR-Adjunct54149.2021.00078  

   Mostofa, Nafisa; Avendano, Indira; McMahan, Ryan P.; Conner, Norma E.; Anderson, Mindi; Welch, Gregory F. (October 2021, 2021 IEEE International Symposium on Mixed and Augmented Reality Adjunct (ISMAR-Adjunct))
4. Local Oort groups and the isolated differential data criterion

   https://doi.org/10.5802/jtnb.1200  

   Dang, Huy; Das, Soumyadip; Karagiannis, Kostas; Obus, Andrew; Thatte, Vaidehee (January 2022, Journal de théorie des nombres de Bordeaux)
5. Isolated and solvated chiroptical behavior in conformationally flexible butanamines

   https://doi.org/10.1002/chir.23570  

   Lemler, Paul M.; Craft, Clayton L.; Pollok, Corina H.; Regan, Thomas P.; Vaccaro, Patrick H. (June 2023, Chirality)

   Abstract The nonresonant optical activity of two highly flexible aliphatic amines, (2R)‐3‐methyl‐2‐butanamine (R‐MBA) and (2R)‐(3,3)‐dimethyl‐2‐butanamine (R‐DMBA), has been probed under isolated and solvated conditions to examine the roles of conformational isomerism and to explore the influence of extrinsic perturbations. The optical rotatory dispersion (ORD) measured in six solvents presented uniformly negative rotatory powers over the 320–590 nm region, with the long‐wavelength magnitude of chiroptical response growing nearly monotonically as the dielectric constant of the surroundings diminished. The intrinsic specific optical rotation, (in deg dm⁻¹[g/mL]⁻¹), extracted for ambient vapor‐phase samples ofR‐MBA [−11.031(98) and −2.29 (11)] andR‐DMBA [−9.434 (72) and −1.350 (48)] at 355 and 633 nm were best reproduced by counterintuitive solvents of high polarity (yet low polarizability) like acetonitrile and methanol. Attempts to interpret observed spectral signatures quantitatively relied on the linear‐response frameworks of density‐functional theory (B3LYP, cam‐B3LYP, and dispersion‐corrected analogs) and coupled‐cluster theory (CCSD), with variants of the polarizable continuum model (PCM) deployed to account for the effects of implicit solvation. Building on the identification of several low‐lying equilibrium geometries (nine forR‐MBA and three forR‐DMBA), ensemble‐averaged ORD profiles were calculated atT = 300 K by means of the independent‐conformer ansatz, which enabled response properties predicted for the optimized structure of each isomer to be combined through Boltzmann‐weighted population fractions derived from corresponding relative internal‐energy or free‐energy values, the latter of which stemmed from composite CBS‐APNO and G4 analyses. Although reasonable accord between theory and experiment was realized for the isolated (vapor‐phase) species, the solution‐phase results were less satisfactory and tended to degrade progressively as the solvent polarity increased. These trends were attributed to solvent‐mediated changes in structural parameters and energy metrics for the transition states that separate and putatively isolate the equilibrium conformations supported by the ground electronic potential‐energy surface, with the resulting displacement of barrier locations and/or decrease of barrier heights compromising the underlying premise of the independent‐conformer ansatz. 

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