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Fluorescence intensity ratio (FIR) thermometry is an ideal non-contact temperature measurement method with rapid response and high sensitivity. Improving sensitivity and stability is always the research hotspot in this field. Energy transfer between the emission centers plays a key role to improve temperature sensitivity. A new method based on synergistic regulation of local surface plasmon resonance (LSPR) effect and energy transfer is introduced in this paper. Tb (TMHD)/Eu(dbm)phen composite films are prepared by coating method. Silver buffer layers and gold nanorods are used to tune the emissions of Tb and Eu. The energy transfer from Tb to Eu is present with 40 % energy transfer efficiency. Silver buffer layers have an overall enhancement effect on the emissions of Tb and Eu, and gold nanorods have a preferential enhancement on the emissions of Eu. With the measurement temperature decreasing, the luminous intensity of the composited film is enhanced by silver layer, but there is no significant influence on the fluorescence intensity ratio. The film covered with Au nanorods presents the highest relative sensitivity of 1.8 % K and has the widest temperature range. This suggests that LSPR effect is an efficient method to tune the temperature sensing property and has potential application in highly sensitive optical thermometers.
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http://dx.doi.org/10.1016/j.saa.2025.126698 | DOI Listing |
J Phys Chem B
September 2025
Department of Chemistry, Indian Institute of Technology Kanpur, Kanpur, Uttar Pradesh 208016, India.
Understanding the evaporation mechanism of liquid ethanol and ethanol-water binary mixtures is important for numerous scientific and industrial processes. The amount of water in liquid water-ethanol mixtures can significantly affect how quickly ethanol molecules evaporate. Here, we study the mechanism and rate of evaporation of ethanol from pure liquid ethanol and ethanol/water binary mixtures through both unbiased molecular dynamics simulations and biased simulations using the umbrella sampling method.
View Article and Find Full Text PDFJ Am Chem Soc
September 2025
National Engineering Research Center of Lower-Carbon Catalysis Technology, Dalian National Laboratory for Clean Energy, Dalian Institute of Chemical Physics, Chinese Academy of Sciences, Dalian 116023, China.
Zeolite-confined Rh-based catalysts have emerged as promising heterogeneous candidates for olefin hydroformylation. However, they face challenges of reactant- and product-induced Rh leaching and aggregation. Herein, zeolite framework-anchored Rh-(O-Zn) sites were designed and are shown to have remarkable activity and stability for gas-phase ethylene hydroformylation.
View Article and Find Full Text PDFCrit Care Sci
September 2025
Brazilian Biosciences National Laboratory, Brazilian Center for Research on Energy and Materials - Campinas (SP), Brazil.
Objective: To develop a score (Palineo score) to identify the palliative care needs of newborn patients admitted to a Brazilian neonatal intensive care unit of a tertiary maternity hospital that serves as a reference center for high-risk pregnancies, ensuring timely follow-up by a specialist.
Methods: Patients were assessed by three specialists using a questionnaire that included the same clinical elements as those used for the Palineo score but did not assign scores to the criteria. The score was determined by the consensus reached by the specialists.
PLoS One
September 2025
Computational Chemistry Laboratory, Chemistry Department, Faculty of Science, Minia University, Minia, Egypt.
Polar protic and aprotic solvents can effectively simulate the maturation of breast carcinoma cells. Herein, the influence of polar protic solvents (water and ethanol) and aprotic solvents (acetone and DMSO) on the properties of 3-(dimethylaminomethyl)-5-nitroindole (DAMNI) was investigated using density functional theory (DFT) computations. Thermodynamic parameters retrieved from the vibrational analysis indicated that the DAMNI's entropy, heat capacity, and enthalpy increased with rising temperature.
View Article and Find Full Text PDFPhys Rev Lett
August 2025
Università degli Studi di Padova, Dipartimento di Fisica e Astronomia, Via Marzolo 8, 35131 Padova, Italy.
Feebly interacting particles, such as sterile neutrinos, dark photons, and axions, can be abundantly produced in the proto-neutron star (PNS) formed in core-collapse supernovae (CCSNe). These particles can decay into photons or charged leptons, depositing energy outside the PNS. Strong bounds on new particles can thus be derived from the observed luminosity of CCSNe, with even tighter bounds obtained from low-energy SNe observations.
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