Results 81 to 90 of about 40,854 (217)
PC is used as the host to achieve doped films with both phosphorescence and photochromic properties, PC can be paired with dozens of phosphorescence guests and photochromic guests, achieving full‐color phosphorescence emission from blue to red, as well as rapid and reversible transitions from colorless to pink, red, or blue–purple.
Peng Chen +9 more
wiley +1 more source
Designing dark energy afterglow experiments
Chameleon fields, which are scalar field dark energy candidates, can evade fifth force constraints by becoming massive in high-density regions. However, this property allows chameleon particles to be trapped inside a vacuum chamber with dense walls ...
Chou, Aaron S. +2 more
core +1 more source
The afterglow and host galaxy of GRB 090205: evidence for a Ly-alpha emitter at z=4.65 [PDF]
Gamma-ray bursts have been proved to be detectable up to distances much larger than any other astrophysical object, providing the most effective way, complementary to ordinary surveys, to study the high redshift universe. To this end, we present here the
A. Fernández-Soto +58 more
core +2 more sources
Endowing Photodeformation Film With Near‐Infrared Afterglow
We present rigid–flexible partitioned molecular design that enables simultaneous visible‐light‐driven photocontraction (up to 48%) and persistent NIR afterglow in PET films. This strategy resolves the fundamental conflict between molecular flexibility required for photodeformation and structural rigidity essential for persistent afterglow, enabling ...
Shiyue Tang +5 more
wiley +1 more source
On the External Inverse Compton Scattering off the Prompt Emission in GRB 221009A
The temporal evolution of the TeV emission of GRB 221009A displays a smooth transition from an initial rapid rise to a slower rise and eventually a decay phase. The smooth light curve suggests an afterglow origin of the TeV emission. The temporal overlap
Cui-Yuan Dai +4 more
doaj +1 more source
Environment and Energy Injection Effects in GRB Afterglows [PDF]
In a recent paper (Dai & Lu 1999), we have proposed a simple model in which the steepening in the light curve of the R-band afterglow of the gamma-ray burst (GRB) 990123 is caused by the adiabatic shock which has evolved from an ultrarelativistic phase ...
Dai Z. G. +8 more
core +2 more sources
Association Between Meteor Radio Afterglows and Optical Persistent Trains [PDF]
K. S. Obenberger +7 more
openalex +1 more source
Mechanochromic Organic Materials: Molecular Mechanisms and Multidimensional Applications
Mechanochromic (MC) organic materials change color in response to mechanical force. This review elucidates the molecular mechanisms (e.g., aggregation‐induced emission, AIE) and explores their multidimensional applications in sensors, anti‐counterfeiting, biomedical devices, and structural health monitoring, providing a roadmap for future smart ...
Xiaozhe Yin +5 more
wiley +1 more source
First hours of the GRB 030329 optical afterglow
We present the first results of the observations of the extremely bright optical afterglow of gamma-ray burst (GRB) 030329 with the 1.5m Russian-Turkish telescope RTT150 (TUBITAK National Observatory, Bakyrlytepe, Turkey).
Alpar, M. A. +14 more
core +1 more source
X‐ray controlled release strategy in cancer therapy
A comprehensive review on the design principles and current strategies of X‐ray stimulated release systems in cancer therapy, focusing on the X‐ray responsive functional groups and materials as well as discussing the advantages and current challenges of X‐ray controlled release systems in cancer therapy.
Yiling Ruan +5 more
wiley +1 more source

