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Equations of Motion and Initial and Boundary Conditions for Gamma-ray Burst
C.L. Bianco,G.V. Vereshchagin,R. Ruffini,S.-S. Xue 한국물리학회 2006 THE JOURNAL OF THE KOREAN PHYSICAL SOCIETY Vol.49 No.2I
We compare and contrast the three different approaches to the optically thick adiabatic phase of Gamma-ray Burst(GRB) all the way to transparency. Special attention is given to the role of the rate equation in self-consistently solving the rate equation with the relativistic hydrodynamic equations. The works of Shemi and Piran [1], Piran, Shemi and Narayan [2], M´esz´aros, Laguna and Rees [3] and Ruffini, Salmonson, Wilson and Xue [4,5] are compared and contrasted. The roles of the baryonic loading in these three treatments are pointed out. The constraints on initial conditions for the fireball produced by an electro-magnetic black hole are obtained.
I.D. Bianco,S.F. Ausar,M. Morcillo,A.E. Leon,P.D. Ribotta,R. Masih,M. Vilaro Mainero,J.L. Amigone,G. Rubin,C. Lescano,L.F. Castagna,D.M. BeltramoG. Diaz 한국식품영양과학회 2003 Journal of medicinal food Vol.6 No.4
In this work we evaluated the efficacy and safety of a bread formulation containing chitosan in dyslipidemictype 2 diabetic subjects. For this purpose a total of 18 patients were allowed to incorporate to their habitual diets 120 g/dayof bread containg 2% (wt/wt) chitosan (chitosan group, n 5 9) or standard bread (control group, n 5 9). Before the studyand after 12 weeks on the modified diet, the following parameters were evaluated: body weight, plasma cholesterol, high-den-sity lipoprotein (HDL)-cholesterol, low-density lipoprotein (LDL)-cholesterol, triglyceride, and hemoglobin A 1c(HbA1c). Com-pared with the control group, the patients receiving chitosan-containg bread decreased their mean levels of LDL-cholesteroland significantly increased their mean levels of HDL-cholesterol at the end of the study. There were no significant differencesin the body weight, serum triglyceride, and HbA 1c. These results suggest that chitosan incorporated into bread formulationscould improve the lipoprotein balance similar to typical biliary salts trappers, increasing the HDL- and lowering the LDL-cholesterol, without changing the triglyceride levels. These results warrant further studies over a longer period of time to eval-uate if a persistent improvement in levels of lipoproteins can be attained with this strategy.
Correlated Λd pairs from the K<sub>stop</sub><sup>-</sup>A->ΛdA<sup>'</sup> reaction
FINUDA Collaboration,Agnello, M.,Beer, G.,Benussi, L.,Bertani, M.,Bhang, H.C.,Bianco, S.,Bonomi, G.,Botta, E.,Bregant, M.,Bressani, T.,Bufalino, S.,Busso, L.,Calvo, D.,Camerini, P.,Caponero, M.,Cerell North-Holland Pub. Co 2007 Physics letters: B Vol.654 No.3
Correlated Λd pairs emitted after the absorption of negative kaons at rest K<SUB>stop</SUB><SUP>-</SUP>A->ΛdA<SUP>'</SUP> in light nuclei <SUP>6</SUP>Li and <SUP>12</SUP>C are studied. Λ-hyperons and deuterons are found to be preferentially emitted in opposite directions. The Λd invariant mass spectrum of <SUP>6</SUP>Li shows a bump whose mass is 3251+/-6 MeV/c<SUP>2</SUP>. The bump mass (binding energy), width and yield are reported. The appearance of a bump is discussed in the realm of the [K@?3N] clustering process in nuclei. The experiment was performed with the FINUDA spectrometer at DAΦNE (LNF).
FINUDA Collaboration,Agnello, M.,Beer, G.,Benussi, L.,Bertani, M.,Bhang, H.C.,Bianco, S.,Bonomi, G.,Botta, E.,Bregant, M.,Bressani, T.,Bufalino, S.,Busso, L.,Calvo, D.,Camerini, P.,Caponero, M.,Cerell North-Holland Pub. Co 2007 Physics letters: B Vol.649 No.1
The inelastic charge exchange reaction (K<SUP>+</SUP>, K<SUP>0</SUP>) on <SUP>7</SUP>Li has been experimentally investigated close to threshold with the FINUDA spectrometer at the e<SUP>+</SUP>e<SUP>-</SUP> collider DAΦNE by searching for K<SUB>S</SUB><SUP>0</SUP> decays. It is the first time that this process has been studied at such low momentum. An upper limit of 2.0 mb (at 95% confidence level) has been measured for the total cross section.
Ishioka, R.,Wang, S.-Y.,Zhang, Z.-W.,Lehner, M. J.,Alcock, C.,Axelrod, T.,Bianco, F. B.,Byun, Y.-I.,Chen, W. P.,Cook, K. H.,Kim, D.-W.,King, S.-K.,Lee, T.,Marshall, S. L.,Protopapas, P.,Rice, J. A.,Sc American Institute of Physics 2014 The Astronomical journal Vol.147 No.4
<P>The Taiwanese-American Occultation Survey project is designed for the detection of stellar occultations by small-size Kuiper Belt Objects, and it has monitored selected fields along the ecliptic plane by using four telescopes with a 3 deg<SUP>2</SUP> field of view on the sky since 2005. We have analyzed data accumulated during 2005-2012 to detect variable stars. Sixteen fields with observations of more than 100 epochs were examined. We recovered 85 variables among a total of 158 known variable stars in these 16 fields. Most of the unrecovered variables are located in the fields observed less frequently. We also detected 58 variable stars which are not listed in the International Variable Star Index of the American Association of Variable Star Observers. These variable stars are classified as 3 RR Lyrae, 4 Cepheid, 1 δ Scuti, 5 Mira, 15 semi-regular, and 27 eclipsing binaries based on the periodicity and the profile of the light curves.</P>