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1. Large and long-term photon energy storage in diazetidines via [2+2] photocycloaddition

   https://doi.org/10.1039/D4SC05374E  

   Nguyen, Han_P Q; Mukherjee, Anurag; Usuba, Junichi; Wan, Joshua; Han, Grace_G D (November 2024, Chemical Science)

   Photo-cycloadduct diazetidines exhibit high energy storage densities exceeding 0.3 MJ kg⁻¹, offering long-term energy storage for up to 23 years and rapid solvent-assisted energy release. 

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2. High-accuracy emulators for observables in ΛCDM, N eff, Σ m ν, and w cosmologies

   https://doi.org/10.1093/mnras/stae1201  

   Bolliet, Boris; Spurio Mancini, Alessio; Hill, J_Colin; Madhavacheril, Mathew; Jense, Hidde_T; Calabrese, Erminia; Dunkley, Jo (May 2024, Monthly Notices of the Royal Astronomical Society)

   ABSTRACT We use the emulation framework CosmoPower to construct and publicly release neural network emulators of cosmological observables, including the cosmic microwave background (CMB) temperature and polarization power spectra, matter power spectrum, distance-redshift relation, baryon acoustic oscillation (BAO) and redshift-space distortion (RSD) observables, and derived parameters. We train our emulators on Einstein–Boltzmann calculations obtained with high-precision numerical convergence settings, for a wide range of cosmological models including ΛCDM, wCDM, ΛCDM + Neff, and ΛCDM + Σmν. Our CMB emulators are accurate to better than 0.5 per cent out to ℓ = 104, which is sufficient for Stage-IV data analysis, and our P(k) emulators reach the same accuracy level out to $$k=50 \, \, \mathrm{Mpc}^{-1}$$, which is sufficient for Stage-III data analysis. We release the emulators via an online repository (CosmoPower Organisation), which will be continually updated with additional extended cosmological models. Our emulators accelerate cosmological data analysis by orders of magnitude, enabling cosmological parameter extraction analyses, using current survey data, to be performed on a laptop. We validate our emulators by comparing them to class and camb and by reproducing cosmological parameter constraints derived from Planck TT, TE, EE, and CMB lensing data, as well as from the Atacama Cosmology Telescope Data Release 4 CMB data, Dark Energy Survey Year-1 galaxy lensing and clustering data, and Baryon Oscillation Spectroscopic Survey Data Release 12 BAO and RSD data. 

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3. Electrically Controlled Biochemical Release from Micro/Nanostructures for in vitro and in vivo Applications: A Review

   https://doi.org/10.1002/cnma.201800157  

   Guo, Jianhe; Fan, Donglei (June 2018, ChemNanoMat)

   Abstract To release biosubstances, including drug molecules, DNAs, and proteins, at prescribed cellular and tissue locations with controllable rates is the Holy Grail of drug delivery that could enable an array of unprecedentedin vitroandin vivoapplications. Extensive research efforts have been focused on exploring innovative mechanisms and approaches for controlling biochemical release with prescribed dose, timing, and dynamics. Particularly, the utilization of electric fields to stimulate the release of biomolecules from synthesized micro/nanostructures has received considerable interest. In this review, we focus on the recent progresses in controlling the release of biomolecules with electric fields by a variety of mechanisms, including electrochemical desorption and actuation, electrically triggered erosion, and electrically driven nanopumps and mechanical motions. The research on external electric stimuli trigged biorelease has progressed rapidly and could make remarkable impact in single‐cell biology, cell‐cell communication, and drug discovery. 

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4. Application of J-Integral to a Random Elastic Medium

   https://doi.org/10.1115/1.4067597  

   Eliáš, Jan; Martinásek, Josef; Le, Jia-Liang (March 2025, Journal of Applied Mechanics)

   Abstract This study investigates the use of the J-integral to compute the statistics of the energy release rate of a random elastic medium. The spatial variability of the elastic modulus is modeled as a homogeneous lognormal random field. Within the framework of Monte Carlo simulation, a modified contour integral is applied to evaluate the first and second statistical moments of the energy release rate. These results are compared with the energy release rate calculated from the potential energy function. The comparison shows that, if the random field of elastic modulus is homogenous in space, the path independence of the classical J-integral remains valid for calculating the mean energy release rate. However, this path independence does not extend to the higher order statistical moments. The simulation further reveals the effect of the correlation length of the spatially varying elastic modulus on the energy release rate of the specimen. 

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5. A blast from the infant Universe: The very high- z GRB 210905A

   https://doi.org/10.1051/0004-6361/202243225  

   Rossi, A.; Frederiks, D. D.; Kann, D. A.; De Pasquale, M.; Pian, E.; Lamb, G.; D’Avanzo, P.; Izzo, L.; Levan, A. J.; Malesani, D. B.; et al (September 2022, Astronomy & Astrophysics)

   We present a detailed follow-up of the very energetic GRB 210905A at a high redshift of z  = 6.312 and its luminous X-ray and optical afterglow. Following the detection by Swift and Konus- Wind , we obtained a photometric and spectroscopic follow-up in the optical and near-infrared (NIR), covering both the prompt and afterglow emission from a few minutes up to 20 Ms after burst. With an isotropic gamma-ray energy release of E iso = 1.27 −0.19 +0.20 × 10 54 erg, GRB 210905A lies in the top ∼7% of gamma-ray bursts (GRBs) in the Konus- Wind catalogue in terms of energy released. Its afterglow is among the most luminous ever observed, and, in particular, it is one of the most luminous in the optical at t  ≳ 0.5 d in the rest frame. The afterglow starts with a shallow evolution that can be explained by energy injection, and it is followed by a steeper decay, while the spectral energy distribution is in agreement with slow cooling in a constant-density environment within the standard fireball theory. A jet break at ∼46.2 ± 16.3 d (6.3 ± 2.2 d rest-frame) has been observed in the X-ray light curve; however, it is hidden in the H band due to a constant contribution from the host galaxy and potentially from a foreground intervening galaxy. In particular, the host galaxy is only the fourth GRB host at z  > 6 known to date. By assuming a number density n  = 1 cm −3 and an efficiency η  = 0.2, we derived a half-opening angle of 8.4 ° ±1.0°, which is the highest ever measured for a z  ≳ 6 burst, but within the range covered by closer events. The resulting collimation-corrected gamma-ray energy release of ≃1 × 10 52 erg is also among the highest ever measured. The moderately large half-opening angle argues against recent claims of an inverse dependence of the half-opening angle on the redshift. The total jet energy is likely too large to be sustained by a standard magnetar, and it suggests that the central engine of this burst was a newly formed black hole. Despite the outstanding energetics and luminosity of both GRB 210905A and its afterglow, we demonstrate that they are consistent within 2 σ with those of less distant bursts, indicating that the powering mechanisms and progenitors do not evolve significantly with redshift. 

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