Interaction of [(VO)-O-IV(acac)(2)] with Human Serum Transferrin and Albumin

VO(acac)(2)] is a remarkable vanadium compound and has potential as a therapeutic drug. It is important to clarify how it is transported in blood, but the reports addressing its binding to serum proteins have been contradictory. We use several spectroscopic and mass spectrometric techniques (ESI and MALDI-TOF), small-angle X-ray scattering and size exclusion chromatography (SEC) to characterize solutions containing [VO(acac)(2)] and either human serum apotransferrin (apoHTF) or albumin (HSA). DFT and modeling protein calculations are carried out to disclose the type of binding to apoHTF. The measured circular dichroism spectra, SEC and MALDI-TOF data clearly prove that at least two VOacac moieties may bind to apoHTF, most probably forming [(VO)-O-IV(acac)(apoHTF)] complexes with residues of the HTF binding sites. No indication of binding of [VO(acac)(2)] to HSA is obtained. We conclude that (VO)-O-IV-acac species may be transported in blood by transferrin. At very low complex concentrations speciation calculations suggest that [(VO)(apoHTF)] species form.Fundacao para a Ciencia e Tecnologia (FCT), Portugal [ RECI/QEQMED/0330/2012, PTDC/QEQ-MED/1902/2014]FCT [IF/00100/2013, IF/00007/2015]PROTEOMASS Scientific SocietyUCIBIO, Unidade de Ciencias Biomoleculares Aplicadas [UID/Multi/04378/2013]ERDF [POCI-01-0145-FEDER-007728, POCI-01-0145-FEDER-007265]info:eu-repo/semantics/publishedVersio

Black holes, gravitational waves and fundamental physics: a roadmap

The grand challenges of contemporary fundamental physics—dark matter, dark energy, vacuum energy, inflation and early universe cosmology, singularities and the hierarchy problem—all involve gravity as a key component. And of all gravitational phenomena, black holes stand out in their elegant simplicity, while harbouring some of the most remarkable predictions of General Relativity: event horizons, singularities and ergoregions. The hitherto invisible landscape of the gravitational Universe is being unveiled before our eyes: the historical direct detection of gravitational waves by the LIGO-Virgo collaboration marks the dawn of a new era of scientific exploration. Gravitational-wave astronomy will allow us to test models of black hole formation, growth and evolution, as well as models of gravitational-wave generation and propagation. It will provide evidence for event horizons and ergoregions, test the theory of General Relativity itself, and may reveal the existence of new fundamental fields. The synthesis of these results has the potential to radically reshape our understanding of the cosmos and of the laws of Nature. The purpose of this work is to present a concise, yet comprehensive overview of the state of the art in the relevant fields of research, summarize important open problems, and lay out a roadmap for future progress. This write-up is an initiative taken within the framework of the European Action on 'Black holes, Gravitational waves and Fundamental Physics'

Evaluation of the binding of four anti-tumor Casiopeinas to human serum albumin

The metal complexes designated by Casiopeinas (R) are mixed-ligand Cu-II-compounds some of them having promising antineoplastic properties. We report studies of binding of Cu(glycinato)(4,7-dimethyl-1,10-phenanthroline) (Cas-II-Gly (1)), Cu(acetylacetonato)(4,7-dimethy1-1,10-phenanthroline) (Cas-III-Ea (2)), Cu(glycinato) (4,4'-dimethyl-2,2'-bipyridine) (Cas-W-Gly (3)) and Cu(acetylacetonato)(4,4'-dimethyl-2,2'-bipyridine) (Cas-IIIia (4)) to human serum albumin (HSA) by circular dichroism (CD), Electron paramagnetic resonance (EPR) and fluorescence spectroscopy. The results indicate that HSA may bind up to three molecules of the tested Casiopeinas. This is confirmed by inductively coupled plasma atomic absorption spectroscopy measurements of samples of HSA-Casiopeinas after passing by adequate size-exclusion columns. The binding of Cas-II-Gly to HSA was also confirmed by MALDI-TOF mass spectrometric experiments. In the physiological range of concentrations the Casiopeinas form 1:1 adducts with HSA, with conditional binding constants of ca. 1 x 10(9) (1), 4 x 10(7) (2), 1 x 10(6) (3) and 2 x 10(5) (4), values determined from the CD spectra measured, and the fluorescence emission spectra indicates that the binding takes place close to the Trp214 residue. Overall, the data confirm that these Casiopeinas may bind to HSA and may be transported in blood serum by this protein; this might allow some selective tumor targeting, particularly in the case of Cas-Il-Gly. In this work we also discuss aspects associated to the reliability of the frequently used methodologies to determine binding constants based on the measurement of fluorescence emission spectra of solutions containing low concentrations of proteins such as HSA and BSA, by titration with solutions of metal complexes.programme Investigador FCT [IF/00100/2013, IF/00007/2015]CONACYT 171991, MexicoBiological Mass Spectrometry Isabel MouraUCIBIOUnidade de Ciencias Biomoleculares Aplicadas [UID/Multi/04378/2013]ERDF under the Partnership Agreement [POCI-01-0145-FEDER-007728]Associate Laboratory for Green Chemistry LAQV [UID/QUI/50006/2013]ERDF under the PT Partnership Agreement [POCI-01-0145-FEDER-007265