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Bagging sequence

In Catalysis, navigating through a collection yields a like collection Bag->Bag, Sequence->Sequence, and so on. The asSet, asSeq, and asBag operators (or asType (T) equivalents) provide conversions. Thus, the following yields a bag of last names containing as many (possibly duplicated) entries as joe has friends. [Pg.710]

Most systems use a time-sequence to control the cleaning frequency. If the particulate load entering the bag-house is constant, this approach would be valid. However, the incoming load generally changes constantly. As a result, the straight time-sequence methodology does not provide the most efficient mode of operation. [Pg.780]

Collection types include sets (no duplicates), bags (duplicates), and sequences (duplicates, ordered). In the following description, explanations in italics indicate where we use Catalysis semantics or extensions or alternative syntax. Functions on collections also apply to sets, sequences, and bags. [Pg.706]

Table 1. The critical mass and energy released in the conversion process of an HS into a QS for several values of the Bag constant and the surface tension. Column labeled MQs,max denotes the maximum gravitational mass of the final QS sequence. The value of the critical gravitational mass of the initial HS is reported on column labeled Mcr whereas those of the mass of the final QS and the energy released in the stellar conversion process are shown on columns labeled Mfi and Econv respectively. BH denotes those cases in which the baryonic mass of the critical mass configuration is larger than the maximum baryonic mass of the QS sequence (M r > MQS>max). In these cases the stellar conversion process leads to the formation of a black hole. Units of B and a are MeV/fm3 and MeV/fm2 respectively. All masses are given in solar mass units and the energy released is given in units of 10B1 erg. The hadronic phase is described with the GM1 model, ms and as are always taken equal to 150 MeV and 0 respectively. The GM1 model predicts a maximum mass for the pure HS of 1.807 M . Table 1. The critical mass and energy released in the conversion process of an HS into a QS for several values of the Bag constant and the surface tension. Column labeled MQs,max denotes the maximum gravitational mass of the final QS sequence. The value of the critical gravitational mass of the initial HS is reported on column labeled Mcr whereas those of the mass of the final QS and the energy released in the stellar conversion process are shown on columns labeled Mfi and Econv respectively. BH denotes those cases in which the baryonic mass of the critical mass configuration is larger than the maximum baryonic mass of the QS sequence (M r > MQS>max). In these cases the stellar conversion process leads to the formation of a black hole. Units of B and a are MeV/fm3 and MeV/fm2 respectively. All masses are given in solar mass units and the energy released is given in units of 10B1 erg. The hadronic phase is described with the GM1 model, ms and as are always taken equal to 150 MeV and 0 respectively. The GM1 model predicts a maximum mass for the pure HS of 1.807 M .
Mhs of the HS corresponding to the given value of the central pressure, as implied by the solution of the Tolmann-Oppeneimer-Volkov equations for the pure Hadronic Star sequences. The results of our calculations are reported in Fig. 2 which is relative to the GM1 EOS for the hadronic phase. Each curve refers to a different value of the bag constant and the surface tension. [Pg.363]

In Fig. 3, we show the MR curve for pure HS within the GM1 model for the EOS of the hadronic phase, and that for hybrid stars or strange stars for different values of the bag constant B. The configuration marked with an asterisk on the hadronic MR curves represents the hadronic star for which the central pressure is equal to Pq. The full circle on the hadronic star sequence represents the critical mass configuration, in the case a = 30 MeV/fm2. The full... [Pg.363]

Figure Jt. The maximum mass MQs,max for the quark star configurations (HS or SS), the critical mass Mcr and the mass Mfi of the stable QS to which it evolves are plotted as a function of the bag constant B. The vertical doted fines labeled B1 — BIV mark the boundary of different ranges of the bag constant which give a different astrophysical output for our scenario, as discussed in the text. The dashed horizontal line gives the value of the maximum mass for the pure hadronic star sequence. All the results are relative to the GM3 model for the EOS for the hadronic phase, the surface tension a is taken equal to 30 MeV/fm2. Figure Jt. The maximum mass MQs,max for the quark star configurations (HS or SS), the critical mass Mcr and the mass Mfi of the stable QS to which it evolves are plotted as a function of the bag constant B. The vertical doted fines labeled B1 — BIV mark the boundary of different ranges of the bag constant which give a different astrophysical output for our scenario, as discussed in the text. The dashed horizontal line gives the value of the maximum mass for the pure hadronic star sequence. All the results are relative to the GM3 model for the EOS for the hadronic phase, the surface tension a is taken equal to 30 MeV/fm2.
Heat penetration study was performed per plant SOP. Using four shelves of the trolley, distribute the load and thermocouples were distributed per the following sequence. Note All bags were to be positioned with Tyvek side down and HDPE side up. [Pg.663]

After prehybridization, replace the liquid with 20 mL of hybridization solution, exclude air bubbles, reseal the bags, and immerse in the water bath. Brief incubations (1 h) are sufficient for the detection of relatively abundant sequences, such as unamplified plasmid pBR322 m E. coli. More extensive incubations (45 h) may be necessary to detect less abundant sequences. [Pg.401]

The catalytic packing MULTIPAK (147) applied in this case study consists of corrugated wire gauze sheets and catalyst bags of the same material assembled in alternate sequence. Sufficient mass transfer between gas and liquid phase is... [Pg.350]


See other pages where Bagging sequence is mentioned: [Pg.297]    [Pg.297]    [Pg.87]    [Pg.139]    [Pg.297]    [Pg.297]    [Pg.87]    [Pg.139]    [Pg.200]    [Pg.6]    [Pg.1603]    [Pg.407]    [Pg.407]    [Pg.410]    [Pg.778]    [Pg.401]    [Pg.191]    [Pg.29]    [Pg.58]    [Pg.87]    [Pg.707]    [Pg.707]    [Pg.49]    [Pg.144]    [Pg.121]    [Pg.345]    [Pg.95]    [Pg.365]    [Pg.56]    [Pg.339]    [Pg.6]    [Pg.435]    [Pg.8]    [Pg.465]    [Pg.204]    [Pg.272]    [Pg.289]    [Pg.132]    [Pg.120]    [Pg.24]    [Pg.1425]    [Pg.54]    [Pg.142]    [Pg.179]   
See also in sourсe #XX -- [ Pg.297 ]




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