1998
DOI: 10.1016/s0375-9601(97)00964-x
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Formation of dusty plasma molecules

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Cited by 75 publications
(55 citation statements)
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“…Resendes et al [14], obtain the same result, as have we [16] and Riley [17]. Chen et al [6] use a simpler, more approximate method to calculate the energy, but arrive at a similar conclusion.…”
Section: Debye-hückel Approximationsupporting
confidence: 59%
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“…Resendes et al [14], obtain the same result, as have we [16] and Riley [17]. Chen et al [6] use a simpler, more approximate method to calculate the energy, but arrive at a similar conclusion.…”
Section: Debye-hückel Approximationsupporting
confidence: 59%
“…This is the procedure implied by Resendes et al [14] and Chen et al [6]. It is incorrect in this case, however, because the system is not isolated.…”
Section: Debye-hückel Approximationmentioning
confidence: 91%
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“…It clearly demonstrates the nonmonotonic behavior of the intergrain interaction which turns especially pronounced while increasing the grain number density or decreasing the screening parameter. The nonmonotonic behavior surely indicates that an attraction between grains turns possible for at least some values of plasma parameters which was also witnessed in [5]. The attraction mechanism remains the same as, e.g., for the molecule formation.…”
Section: Numerical Results For Macropotentials and Conclusionsupporting
confidence: 61%
“…In many theoretical studies of dusty-plasma phase transitions, dust transport, two-body interactions, and dust-particle agglomeration, the charge on individual dust particles has been assumed constant during particle-particle interactions. [3][4][5][6] However, the charge on dust particles in a plasma can vary for many reasons. [7][8][9][10] One cause is the spatial variation in the electron velocity distribution function.…”
Section: Introductionmentioning
confidence: 99%