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1.
J Photochem Photobiol B ; 255: 112925, 2024 Jun.
Artículo en Inglés | MEDLINE | ID: mdl-38703451

RESUMEN

Visible light triggers free radical production in alive and intact Drosophila melanogaster. We exposed fruit flies to red (613-631 nm), green (515-535 nm), and blue (455-475 nm) light while we monitored changes in unpaired electron content with an electron spin resonance spectrometer (ESR/EPR). The immediate response to light is a rapid increase in spin content lasting approximately 10 s followed by a slower, linear increase for approximately 170 s. When the light is turned off, the spin population promptly decays with a similar time course, though never fully returning to baseline. The magnitude and time course of the spin production depends on the wavelength of the light. Initially, we surmised that eumelanin might be responsible for the spin change because of its documented ability for visible light absorption and its highly stable free radical content. To explore this, we utilized different fruit fly strains with varying eumelanin content and clarified the relation of melanin types with the spin response. Our findings revealed that flies with darker cuticle have at least three-fold more unpaired electrons than flies with yellow cuticle. However, to our surprise, the increase in unpaired electron population by light was not drastically different amongst the genotypes. This suggests that light-induced free radical production may not exclusively rely on the presence of black melanin, but may instead be dependent on light effects on quinone-based cuticular polymers.


Asunto(s)
Drosophila melanogaster , Luz , Melaninas , Animales , Radicales Libres/química , Drosophila melanogaster/metabolismo , Espectroscopía de Resonancia por Spin del Electrón , Melaninas/química , Melaninas/metabolismo , Melaninas/biosíntesis
2.
J Phys Chem Lett ; 13(19): 4215-4219, 2022 May 19.
Artículo en Inglés | MEDLINE | ID: mdl-35512393

RESUMEN

It has been known for over a century that racemic solutions of hydrogen-bonded compounds are less viscous than their component enantiomers, but this fact has so far remained unexplained. Here we confirm it using enantiomers of lactic acid and compare it to molecular dynamics (MD) simulations of lactic acid viscosity. The effect is absent in classical MD. We suggest that the anomalous viscosity of racemates may be due to a recently discovered magnetic intermolecular force due to spin-dependent charge reorganization.


Asunto(s)
Ácido Láctico , Estereoisomerismo , Viscosidad
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