7,781 research outputs found

    Stabilization of quantum metastable states by dissipation

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    Normally, quantum fluctuations enhance the escape from metastable states in the presence of dissipation. Here we show that dissipation can enhance the stability of a quantum metastable system, consisting of a particle moving in a strongly asymmetric double well potential, interacting with a thermal bath. We find that the escape time from the metastable state has a nonmonotonic behavior versus the system-bath coupling and the temperature, producing a stabilizing effect.Comment: 4 pages, 3 figures, submitted to Phys. Rev.

    WISeREP - An Interactive Supernova Data Repository

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    We have entered an era of massive data sets in astronomy. In particular, the number of supernova (SN) discoveries and classifications has substantially increased over the years from few tens to thousands per year. It is no longer the case that observations of a few prototypical events encapsulate most spectroscopic information about SNe, motivating the development of modern tools to collect, archive, organize and distribute spectra in general, and SN spectra in particular. For this reason we have developed the Weizmann Interactive Supernova data REPository - WISeREP - an SQL-based database (DB) with an interactive web-based graphical interface. The system serves as an archive of high quality SN spectra, including both historical (legacy) data as well as data that is accumulated by ongoing modern programs. The archive provides information about objects, their spectra, and related meta-data. Utilizing interactive plots, we provide a graphical interface to visualize data, perform line identification of the major relevant species, determine object redshifts, classify SNe and measure expansion velocities. Guest users may view and download spectra or other data that have been placed in the public domain. Registered users may also view and download data that are proprietary to specific programs with which they are associated. The DB currently holds >8000 spectra, of which >5000 are public; the latter include published spectra from the Palomar Transient Factory, all of the SUSPECT archive, the Caltech-Core-Collapse Program, the CfA SN spectra archive and published spectra from the UC Berkeley SNDB repository. It offers an efficient and convenient way to archive data and share it with colleagues, and we expect that data stored in this way will be easy to access, increasing its visibility, usefulness and scientific impact.Comment: To be published in PASP. WISeREP: http://www.weizmann.ac.il/astrophysics/wiserep

    Origin of the insulating state in honeycomb iridates and rhodates

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    A burning question in the emerging field of spin-orbit driven insulating iridates, such as Na2IrO3 and Li2IrO3 is whether the observed insulating state should be classified as a Mott-Hubbard insulator derived from a half-filled relativistic j_eff=1/2 band or as a band insulator where the gap is assisted by spin-orbit interaction, or Coulomb correlations, or both. The difference between these two interpretations is that only for the former, strong spin-orbit coupling (lambda >~ W, where W is the band width) is essential. We have synthesized the isostructural and isoelectronic Li2RhO3 and report its electrical resistivity and magnetic susceptibility. Remarkably it shows insulating behavior together with fluctuating effective S=1/2 moments, similar to Na2IrO3 and Li2IrO3, although in Rh4+ (4d5) the spin-orbit coupling is greatly reduced. We show that this behavior has non-relativistic one-electron origin (although Coulomb correlations assist in opening the gap), and can be traced down to formation of quasi-molecular orbitals, similar to those in Na2IrO3.Comment: 7 pages, 7 figure

    Reinforcing the link between the double red clump and the X-shaped bulge of the Milky Way

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    The finding of a double red clump in the luminosity function of the Milky Way bulge has been interpreted as evidence for an X-shaped structure. Recently, an alternative explanation has been suggested, where the double red clump is an effect of multiple stellar populations in a classical spheroid. In this Letter we provide an observational assessment of this scenario and show that it is not consistent with the behaviour of the red clump across different lines of sight, particularly at high distances from the Galactic plane. Instead, we confirm that the shape of the red clump magnitude distribution closely follows the distance distribution expected for an X-shaped bulge at critical Galactic latitudes. We also emphasize some key observational properties of the bulge red clump that should not be neglected in the search for alternative scenarios

    Photo-oxidative and soil burial degradation of irrigation tubes based on biodegradable polymer blends

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    Irrigation tubes based on biodegradable polymers were prepared via an extrusion-drawing process by Irritec and compared to conventional pipes made of high-density polyethylene (HDPE). A commercial polylactide/poly (butyleneadipate-co-butyleneterephthalate) (PLA/PBAT) blend (Bio-Flex®) and Mater-Bi® were used. The polymers were characterized from rheological and mechanical points of view. Irrigation pipes were subjected to photoaging with continued exposure to UV radiation up to 22 days. The degradability in the soil of irrigation tube samples was studied. The influence of temperature and UV irradiation on soil burial degradation was investigated. A soil burial degradation test was carried out at 30 °C and 50 °C for up to 70 days. The degree of degradation was evaluated from the weight loss percentage. The degradation rate of irrigation tube samples based on Mater-Bi® was higher at 30 °C and was stimulated after 14 days of UV irradiation. Higher temperatures or UV aging encouraged the disintegration in soil of Bio-Flex®-based irrigation tubes. Furthermore, tube samples, before and after UV and soil burial degradation, were analyzed by Attenuated Total Reflection-Fourier Transform Infra-Red (ATR-FTIR) spectroscop

    IL SITO PREISTORICO DELLO ZUBBIO DI COZZO SAN PIETRO S.I.C. RUPI DI CATALFANO E CAPO ZAFFERANO

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    All’interno del S.I.C, “Rupi di Catalfano e Capo Zafferano”, alcune delle grotte presenti sono state frequentate dall’uomo fin dalla preistoria. Mettendo a confronto la genesi delle cavità e la loro ubicazione topografica, è evidente che la scelta dei siti consoni a essere usati dall’uomo è marcatamente strategica e ponderata. L’indagine è stata condotta dapprima individuando e raggiungendo i siti noti in bibliografia, dai quali si è cercato di elaborare un modello per individuare nuovi siti che potessero presentare evidenze di frequentazione umana risalenti alla preistoria, soprattutto recente. All’interno di una grotta, Zubbio di Cozzo San Pietro, ubicata ad una quota di 300 m s.l.m sul versante est di Cozzo San Pietro, ad una profondità di 15 m, è stato rinvenuto e fotografato un deposito contenente resti umani, ossa, denti, alcuni frammenti d’industria litica, fra cui una scheggia di ossidiana, e numerosi frammenti fittili, alcuni databili all’età del Bronzo Medio, facies di Thapsos. A breve, all’interno del sito verrà effettuato un saggio di scavo. Sulla base delle osservazioni precedenti, sono stati considerati tutti gli elementi noti sul popolamento umano del territorio indagato, con un approccio mirato alla comprensione delle dinamiche di utilizzo dell’ambiente secondo le economie del passato
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