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mICROENDOSCOPIC SPECTRAL ImAGING AS A TOOL FOR SmALL DUCTUAL DIAGNOSTICS:PRELImINARY EXPERIENCE

Journal of Innovative Optical Health Sciences 2012年第3期5卷 64-70页

作者： A.DOUPLIK W.L.LEONG a.m.easson S.DONE B.C.WILSON A.SHAHmOON Z.ZALEVSKY Department of Physics Ryerson University 350 Victoria StreetToronto M5B 2K3Canada School of Advanced Optical Technologies(SAOT)Friedrich-Alexander Erlangen-Nuremberg University ErlangenGermany Ontario Cancer Institute University Health Network TorontoCanada Xillix Ltd TorontoCanada medical Photonics Engineering Group(mPEG)Chair of Photonics Technologies Friedrich-Alexander Erlangen-Nuremberg University ErlangenGermany Department of Surgical Oncology Princess margaret Hospital University Health Network TorontoCanada Department of medical Biophysics University of Toronto TorontoCanada Faculty of Engineering Bar-Ilan University Ramat GanIsrael

A technical feasibility of autofluorescence ductoscopy in breast milk ducts as blood vessels phantoms has been assessed as *** tumor can be clearly identified through the milk *** also present the operation principle as well as the preliminary experimental results of a new type of microsize multicorefiber that enables imaging through blood vessel *** of a manipulated microwire through a drilled phantom is presented.

关键词： Cancer margin delineation endoscopy microendoscopy autofluorescence imaging surgical guidance multicorefibers

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Primordial black hole mass functions as a probe of cosmic origin

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Science China(Physics,mechanics & Astronomy) 2024年第5期67卷 164-171页

作者： Yi-Fu Cai Chengfeng Tang Geyu mo Sheng-Feng Yan Chao Chen Xiao-Han ma Bo Wang Wentao Luo Damien A.easson Antonino marcianò Deep Space Exploration Laboratory/School of Physical Sciences University of Science and Technology of ChinaHefei 230026China CAS Key Laboratory for Researches in Galaxies and Cosmology/Department of Astronomy School of Astronomy and Space ScienceUniversity of Science and Technology of ChinaHefei 230026China Istituto Nazionale di Fisica Nucleare(INFN) Sezione di MilanoMilano 20146Italy DiSAT Universitàdegli Studi dell'InsubriaComo 22100Italy Jockey Club Institute for Advanced Study The Hong Kong University of Science and TechnologyHong KongChina Department of Physics Arizona State UniversityTempe 85287-1504USA Department of Physics&Center for Field Theory and Particle Physics Fudan UniversityShanghai 200433China Laboratori Nazionali di Frascati INFN Via Enrico Fermi 541 Frascati(Roma)00044Italy INFN sezione Roma Tor Vergata Rome I-00133Italy School of Physics University of Electronic Science and Technology of ChinaChengdu11731China

We discuss a novel window to probe the origin of our universe via the mass functions of primordial black holes(PBHs).The mass functions of PBHs are simply estimated using the conventional Press-Schechter formalism for two paradigms of cosmic origin,including inflationaryΛCDm and bounce *** standard inflationaryΛCDm model cannot generate an appreciable number of massive PBHs;however,non-trivial inflation models with blue-tilted power spectra at small scales and matter bounce cosmology provide formation mechanisms for heavy PBHs,which in turn,may seed the observed supermassive black holes(SmBHs).By fitting the SmBH mass functions at high redshift(z~6)derived from Sloan Digital Sky Survey(SDSS)and Canada-France High-z Quasar Survey(CFHQS)quasars,for two paradigms of cosmic origin,we derive constraints on the PBH density fraction fPBHat z~6 and the characteristic mass m_(★),with the prior assumption that all SmBHs stem from *** demonstrate that this newly proposed procedure,relying on astronomical measurements that utilize deep-field surveys of SmBHs at high redshift,can be used to constrain models of cosmic ***,although not the main focus of this paper,we evolve the mass function from z~6 to z~0 through an assumption of 3×10^(8)-year Eddington’s accretion,and give a rough estimation of fPBHat z~0.

关键词： origin cosmic massive

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