80 research outputs found

    Transient absorption spectroscopic studies on 4-nitroquinoline N-oxide: From femtoseconds to microseconds timescale

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    [EN] The singlet excited state of 4-nitroquinoline N-oxide ((1)NQNO*) has been characterized by different spectroscopic techniques, combining transient absorption with steady state and time-resolved emission spectroscopy. The energy of (1)NQNO* has been established as 255 kJ/mol from the fluorescence spectrum, whereas its lifetime has been found to be 10 ps in the femto-laser flash photolysis (LFP) experiments, where a characteristic S-1-S-n absorption band with maximum centered at 425 nm is observed. In a first stage, the triplet excited state of NQNO ((3)NQNO*) has also been characterized by emission spectroscopy in solid matrix, at low temperature. Thus, from the steady state phosphorescence spectrum the triplet energy has been estimated as 183 kJ/mol, whereas the setup with time resolution has allowed us to determine the phosphorescence lifetime as 3 ms. Formation of (3)NQNO* by intersystem crossing in solution at room temperature, has been monitored by femto-LFP, which shows the appearance of a band with maximum at 560 nm (T-1-T-n). It increases with the decreasing intensity of its precursor 425 nm(S-1-S-n) band, giving rise to an isosbestic point at 500 nm. The characterization of (3)NQNO* has been completed by nano-LFP, using xanthone as photosensitizer and oxygen as well as beta-carotene as quenchers. In addition, quenching of (3)NQNO* by electron donors (DABCO) is also observed in aprotic solvents, leading to the radical anion of NQNO (.(-)NQNO). If there is a proton source in the medium (Et3N as electron donor or MeCN:H2O/4:1 as solvent system) protonation of the radical anion results in formation of the neutral radical of NQNO (.NQNOH). In general, all processes are slower in protic solvents because of the solvation sphere. Overall, this information provides a deeper insight into the formation and behavior of excited states and radical ionic species derived from the title molecule NQNO. (C) 2019 Elsevier B.V. All rights reserved.The work was financially supported by the Regional Government of Generalitat Valenciana (PROMETEO/2017/075) as well as the Spanish Government Science Department with the CTQ-2016-78875-P and CTQ-2009-13699 projects and the N. D.-G. fellowship (BES-2010-035875). BC, CC and FE acknowledge MIUR and the University of Perugia for financial support to the project AMIS, through the program "Dipartimenti di Eccellenza - 2018-2022"Duran-Giner, N.; Carlotti, B.; Clementi, C.; Elisei, F.; Encinas Perea, S.; Miranda Alonso, MÁ. (2019). Transient absorption spectroscopic studies on 4-nitroquinoline N-oxide: From femtoseconds to microseconds timescale. Spectrochimica Acta Part A Molecular and Biomolecular Spectroscopy. 216:265-272. https://doi.org/10.1016/j.saa.2019.02.105S265272216Fuchs, T., Gates, K. S., Hwang, J.-T., & Greenberg, M. M. (1999). Photosensitization of Guanine-Specific DNA Damage by a Cyano-Substituted Quinoxaline Di-N-oxide. Chemical Research in Toxicology, 12(12), 1190-1194. doi:10.1021/tx990149sDaniels, J. S., & Gates, K. S. (1996). DNA Cleavage by the Antitumor Agent 3-Amino-1,2,4-benzotriazine 1,4-Dioxide (SR4233):  Evidence for Involvement of Hydroxyl Radical. Journal of the American Chemical Society, 118(14), 3380-3385. doi:10.1021/ja9510774Jerina, D. M., Boyd, D. R., & Daly, J. W. (1970). Photolysis of pyridine-N-oxide: an oxygen atom transfer model for enzymatic oxygenation, arene oxide formation, and the NIH shift. Tetrahedron Letters, 11(6), 457-460. doi:10.1016/0040-4039(70)80074-0Albini, A., & Alpegiani, M. (1984). The photochemistry of the N-oxide function. Chemical Reviews, 84(1), 43-71. doi:10.1021/cr00059a004Winkle, S. A., & Tinoco, I. (1978). Interactions of 4-nitroquinoline 1-oxide with four deoxyribonucleotides. Biochemistry, 17(7), 1352-1356. doi:10.1021/bi00600a033Sheng, Z., Song, Q., Gao, F., Zhou, X., Li, J., Dai, J., … Ma, X. (2000). A laser flash photolysis study of amino acids and dipeptides using 4-nitroquinoline 1-oxide as a photosensitizer: The pH dependence. Research on Chemical Intermediates, 26(7-8), 715-725. doi:10.1163/156856700x00633Yamakawa, M., Kubota, T., Ezumi, K., & Mizuno, Y. (1974). Absorption and phosphorescence spectra of 4-nitropyridine N-oxides and 4- and 3-nitroquinoline N-oxides. Spectrochimica Acta Part A: Molecular Spectroscopy, 30(11), 2103-2119. doi:10.1016/0584-8539(74)80061-9Kubota, T., Yamakawa, M., & Mizuno, Y. (1972). The Singlet-triplet Absorption Spectra of Heterocyclic AmineN-Oxides (I). Bulletin of the Chemical Society of Japan, 45(11), 3282-3286. doi:10.1246/bcsj.45.3282Kasama, K., Takematsu, A., Yamamoto, S., & Arai, S. (1984). Photochemical reactions of 4-nitroquinoline 1-oxide with DNA and related compounds. The Journal of Physical Chemistry, 88(21), 4918-4921. doi:10.1021/j150665a025Dutta Choudhury, S., & Basu, S. (2006). Interaction of 4-Nitroquinoline-1-oxide with Indole Derivatives and Some Related Biomolecules:  A Study with Magnetic Field. The Journal of Physical Chemistry B, 110(17), 8850-8855. doi:10.1021/jp055971lSeki, H., Takematsu, A., & Arai, S. (1987). Photoinduced electron transfer from amino acids and proteins to 4-nitroquinoline 1-oxide in aqueous solutions. The Journal of Physical Chemistry, 91(1), 176-179. doi:10.1021/j100285a038Shi, X., & Platz, M. S. (2004). Time Resolved Spectroscopy of Some Aromatic N-Oxide Triplets, Radical Anions, and Related Radicals. The Journal of Physical Chemistry A, 108(20), 4385-4390. doi:10.1021/jp037708vEzumi, K., Kubota, T., Miyazaki, H., & Yamakawa, M. (1976). Electronic spectra of the anion radicals of heterocyclic amine N-oxides and related substances. The Journal of Physical Chemistry, 80(9), 980-988. doi:10.1021/j100550a012Daniels, J. S., Gates, K. S., Tronche, C., & Greenberg, M. M. (1998). Direct Evidence for Bimodal DNA Damage Induced by Tirapazamine. Chemical Research in Toxicology, 11(11), 1254-1257. doi:10.1021/tx980184jBosca, F., Encinas, S., Heelis, P. F., & Miranda, M. A. (1997). Photophysical and Photochemical Characterization of a Photosensitizing Drug:  A Combined Steady State Photolysis and Laser Flash Photolysis Study on Carprofen. Chemical Research in Toxicology, 10(7), 820-827. doi:10.1021/tx9700376Carlotti, B., Cesaretti, A., Fortuna, C. G., Spalletti, A., & Elisei, F. (2015). Experimental evidence of dual emission in a negatively solvatochromic push–pull pyridinium derivative. Physical Chemistry Chemical Physics, 17(3), 1877-1882. doi:10.1039/c4cp04963bCesaretti, A., Carlotti, B., Gentili, P. L., Clementi, C., Germani, R., & Elisei, F. (2014). Spectroscopic Investigation of the pH Controlled Inclusion of Doxycycline and Oxytetracycline Antibiotics in Cationic Micelles and Their Magnesium Driven Release. The Journal of Physical Chemistry B, 118(29), 8601-8613. doi:10.1021/jp502278zCarlotti, B., Cesaretti, A., & Elisei, F. (2012). Complexes of tetracyclines with divalent metal cations investigated by stationary and femtosecond-pulsed techniques. Phys. Chem. Chem. Phys., 14(2), 823-834. doi:10.1039/c1cp22703

    Mimicking the Secretory Action of a Gland by a CompositeSystem Made of a pH-Responsive Surfactant-Based Hydrogel and a DialysisMembrane

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    The hydrogel obtained by a zwitterionic N-oxide surfactant is proposed as the core of a pH-responsive artificial gland model. The viscosity and pH variations, induced by pulse additions of acid and base, are investigated by a pyridinium salt and alizarin red S, respectively. The artificial gland model is implemented by enclosing the gel within a dialysis membrane, and its secretory action is tested by monitoring the release of a fluorescent acridinium salt

    Use of a Zwitterionic Surfactant to Improve the Biofunctional Properties of Wool Dyed with an Onion (Allium cepa L.) Skin Extract

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    To improve the loadability and antioxidant properties of wool impregnated with onion skin extract, the introduction of SB3-14 surfactant in the dyeing process was evaluated. A preliminary investigation on the surfactant–quercetin interaction indicated that the optimal conditions for dye solubility, stability, and surfactant affinity require double-distilled water (pH = 5.5) as a medium and SB3-14 in a concentration above the c.m.c. (2.5 × 10−3 M). The absorption profile of textiles showed the flavonoid absorption band (390 nm) and a bathochromic feature (510 nm), suggesting flavonoid aggregates. The higher absorbance for the sample dyed with SB3-14 indicated greater dye uptake, which was further confirmed by HPLC analysis. The Folin–Ciocalteu method was applied to evaluate the total phenol content (TPC) released from the treated wool, while the assays FRAP, DPPH, ABTS, and ORAC were applied to evaluate the corresponding total antioxidant activity (TAC). Higher TPCs (about 20%) and TACs (5–55%) were measured with SB3-14, highlighting textiles with improved biofunctional properties. Spectrophotometric analyses were also performed with an artificial sweat. The potential cytotoxic effect of SB3-14 in both monomeric and aggregated forms, cell viability, and induction of apoptosis were evaluated in RAW 264.7 cells. These analyses revealed that SB3-14 is safe at concentrations below the c.m.c

    Implementation and performances of the IPbus protocol for the JUNO Large-PMT readout electronics

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    The Jiangmen Underground Neutrino Observatory (JUNO) is a large neutrino detector currently under construction in China. Thanks to the tight requirements on its optical and radio-purity properties, it will be able to perform leading measurements detecting terrestrial and astrophysical neutrinos in a wide energy range from tens of keV to hundreds of MeV. A key requirement for the success of the experiment is an unprecedented 3% energy resolution, guaranteed by its large active mass (20 kton) and the use of more than 20,000 20-inch photo-multiplier tubes (PMTs) acquired by high-speed, high-resolution sampling electronics located very close to the PMTs. As the Front-End and Read-Out electronics is expected to continuously run underwater for 30 years, a reliable readout acquisition system capable of handling the timestamped data stream coming from the Large-PMTs and permitting to simultaneously monitor and operate remotely the inaccessible electronics had to be developed. In this contribution, the firmware and hardware implementation of the IPbus based readout protocol will be presented, together with the performances measured on final modules during the mass production of the electronics

    Mass testing of the JUNO experiment 20-inch PMTs readout electronics

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    The Jiangmen Underground Neutrino Observatory (JUNO) is a multi-purpose, large size, liquid scintillator experiment under construction in China. JUNO will perform leading measurements detecting neutrinos from different sources (reactor, terrestrial and astrophysical neutrinos) covering a wide energy range (from 200 keV to several GeV). This paper focuses on the design and development of a test protocol for the 20-inch PMT underwater readout electronics, performed in parallel to the mass production line. In a time period of about ten months, a total number of 6950 electronic boards were tested with an acceptance yield of 99.1%

    Validation and integration tests of the JUNO 20-inch PMTs readout electronics

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    The Jiangmen Underground Neutrino Observatory (JUNO) is a large neutrino detector currently under construction in China. JUNO will be able to study the neutrino mass ordering and to perform leading measurements detecting terrestrial and astrophysical neutrinos in a wide energy range, spanning from 200 keV to several GeV. Given the ambitious physics goals of JUNO, the electronic system has to meet specific tight requirements, and a thorough characterization is required. The present paper describes the tests performed on the readout modules to measure their performances.Comment: 20 pages, 13 figure

    Potential of Core-Collapse Supernova Neutrino Detection at JUNO

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    JUNO is an underground neutrino observatory under construction in Jiangmen, China. It uses 20kton liquid scintillator as target, which enables it to detect supernova burst neutrinos of a large statistics for the next galactic core-collapse supernova (CCSN) and also pre-supernova neutrinos from the nearby CCSN progenitors. All flavors of supernova burst neutrinos can be detected by JUNO via several interaction channels, including inverse beta decay, elastic scattering on electron and proton, interactions on C12 nuclei, etc. This retains the possibility for JUNO to reconstruct the energy spectra of supernova burst neutrinos of all flavors. The real time monitoring systems based on FPGA and DAQ are under development in JUNO, which allow prompt alert and trigger-less data acquisition of CCSN events. The alert performances of both monitoring systems have been thoroughly studied using simulations. Moreover, once a CCSN is tagged, the system can give fast characterizations, such as directionality and light curve

    Detection of the Diffuse Supernova Neutrino Background with JUNO

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    As an underground multi-purpose neutrino detector with 20 kton liquid scintillator, Jiangmen Underground Neutrino Observatory (JUNO) is competitive with and complementary to the water-Cherenkov detectors on the search for the diffuse supernova neutrino background (DSNB). Typical supernova models predict 2-4 events per year within the optimal observation window in the JUNO detector. The dominant background is from the neutral-current (NC) interaction of atmospheric neutrinos with 12C nuclei, which surpasses the DSNB by more than one order of magnitude. We evaluated the systematic uncertainty of NC background from the spread of a variety of data-driven models and further developed a method to determine NC background within 15\% with {\it{in}} {\it{situ}} measurements after ten years of running. Besides, the NC-like backgrounds can be effectively suppressed by the intrinsic pulse-shape discrimination (PSD) capabilities of liquid scintillators. In this talk, I will present in detail the improvements on NC background uncertainty evaluation, PSD discriminator development, and finally, the potential of DSNB sensitivity in JUNO

    Real-time Monitoring for the Next Core-Collapse Supernova in JUNO

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    Core-collapse supernova (CCSN) is one of the most energetic astrophysical events in the Universe. The early and prompt detection of neutrinos before (pre-SN) and during the SN burst is a unique opportunity to realize the multi-messenger observation of the CCSN events. In this work, we describe the monitoring concept and present the sensitivity of the system to the pre-SN and SN neutrinos at the Jiangmen Underground Neutrino Observatory (JUNO), which is a 20 kton liquid scintillator detector under construction in South China. The real-time monitoring system is designed with both the prompt monitors on the electronic board and online monitors at the data acquisition stage, in order to ensure both the alert speed and alert coverage of progenitor stars. By assuming a false alert rate of 1 per year, this monitoring system can be sensitive to the pre-SN neutrinos up to the distance of about 1.6 (0.9) kpc and SN neutrinos up to about 370 (360) kpc for a progenitor mass of 30MM_{\odot} for the case of normal (inverted) mass ordering. The pointing ability of the CCSN is evaluated by using the accumulated event anisotropy of the inverse beta decay interactions from pre-SN or SN neutrinos, which, along with the early alert, can play important roles for the followup multi-messenger observations of the next Galactic or nearby extragalactic CCSN.Comment: 24 pages, 9 figure
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