WebTranscribed image text: f(1-F) (8) where f fi/f and F = F/F2 If the term on the left-hand side is plotted against the coefficient of r, a straight line results where slope is ri and ordinate intercept is r2. The graph obtained using equation (8) is called the Fineman-Ross plot WebNov 29, 2014 · According to the Fineman-Ross method , r 1 and r 2 can be estimated from the slope and the intercept in a G–F plot as shown in Fig. 3a. Fig. 3 Determination of reactivity ratios for copolymerization of AM with DMAPS by the Fineman-Ross ( a ) and the Kelen-Tüdös ( b ) methods ( black square for the experimental value and red line stands …
Fineman-Ross method - Big Chemical Encyclopedia
WebSep 1, 1996 · The monomer reactivity ratios (MRRs) of M 1 and M 2 were estimated by the Fineman—Ross and Kelen—Tüdos methods, by analysing copolymer compositions which were determined by 1 H nuclear magnetic resonance (n.m.r.) ... (W W 0 versus time plot). Previous article in issue; Next article in issue. Keywords. 7-acryloyloxy-4 … WebDec 2, 2024 · The Fineman–Ross linearization method revealed a strong correlation (R 2 = 0.9994) between monomer percentage in the feed and monomer incorporated into the polymer. starfall numbers feeding the animals
Reactivity Ratio - an overview ScienceDirect Topics
WebUsing the data in Table III, the general copolymer composition equations, and the Fineman-Ross procedure (16), the reactivity ratios were estimated at rx — 0.40 and 0.42 and r2 = … WebFeb 15, 2024 · According to the Fineman-Ross plot (Fig. S36), the competitive reactivity ratios are r E = 1.32 and r FSt5 = 0.12. All copolymers of ethylene and FSt4 were examined by both 1 H NMR and 13 C NMR to reveal their compositions and … Webterms of Fineman–Ross plots, which are used below to evaluate the copolymerization behavior of DPAAc complexes with differ- ... Then, a Fineman–Ross plot was constructed based on the calculated values of F(f 1)/F and F2/f (Table 1), eventually determining that reactivity ratios r 1 and r 2 were 0.991 and 1.04, respectively (Fig. 2a). The starfall numbers 1 to 20