2001
DOI: 10.1016/s0167-7322(01)00223-9
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Colloids with polymer stars: the interaction

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Cited by 11 publications
(14 citation statements)
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“…This is consistent with simulations and renormalization group theory. 13 At longer distances an exponential decay is found for both F and f, as expected.…”
Section: Hybrid Mc-scf Methodssupporting
confidence: 81%
“…This is consistent with simulations and renormalization group theory. 13 At longer distances an exponential decay is found for both F and f, as expected.…”
Section: Hybrid Mc-scf Methodssupporting
confidence: 81%
“…For f = 2, it yields for the prefactor αf 3/2 the value 0.786, which is very close to the exact value 0.8 calculated by means of renormalization group techniques by des Cloizeaux [72]. Moreover, recent renormalization group calculations show that the functional form (5/18)f 3/2 yields excellent agreement with the 'exact' value, at least up to f = 6 [73][74][75][76].…”
Section: Theorysupporting
confidence: 71%
“…This assumption nicely reproduces the contact exponents as derived from 3-loop perturbation theory [9] as is displayed in table 5 taken from the [33]. In table 5 we use the approximate values of η f to calculate the cone estimation of the contact exponents and compare these with the corresponding values of a renormalization group calculation.…”
Section: Colloids With Polymer Stars: the Interactionsupporting
confidence: 68%
“…Numerical values for the exponent λ mn as well as perturbation theory expansions for them follow from tables 2, 3 and are analyzed in detail in [9,[42][43][44]. Here, let us analyze several particular cases for an absorbing m-star with a reactant trap at its core and simply absorbing traps along all chains:…”
Section: Diffusion-controlled Reactions In Presence Of Polymersmentioning
confidence: 99%