Papers in Physics, vol. 6, art. 060008 (2014) Received: 10 October 2014, Accepted: 10 October 2014 Edited by: L. A. Pugnaloni Licence: Creative Commons Attribution 3.0 DOI: http://dx.doi.org/10.4279/PIP.060008 www.papersinphysics.org ISSN 1852-4249 Commentary on “Jamming transition in a two-dimensional open granular pile with rolling resistance” Roberto Arévalo1∗ I. Introduction The paper “Jamming transition in a two- dimensional open granular pile with rolling resis- tance” studies the jamming transition using the flow of granular particles from piles. In this com- mentary I would like to give a perspective on the results by Magalhães et al. [1] and previous related studies obtained in silos. We speak about jamming transition in a silo when an arch forms at the outlet effectively arrest- ing the flow. This is likely to happen when the size of the outlet is a few times bigger than that of the flowing particles. What factors control the probability of arch formation? If we fix the na- ture of the particles, it is found that the pressure close to the outlet has a major influence. In Ref. [2], it was shown that altering this pressure in a two-dimensional silo can change the probability of arch formation by two orders of magnitude. At the same time, the flow rate or velocity field are modi- fied only slightly. In a flat-bottomed silo, pressure increases lin- early from the free surface toward the bottom. At a certain depth, however, pressure saturates and remains constant until the base. This is the well known Janssen effect. It is usually attributed to ∗E-mail: aroberto@ntu.edu.sg 1 Nanyang Technological University, School of Physi- cal and Mathematical Sciences, Physics and Applied Physics, 21 Nanyang Link, 637371, Singapore. the friction of the walls that sustains part of the weight of the column of particles. The depth at which pressure saturates depends on properties of the grains (like the Poisson ratio) and the geometry of the silo. This scenario for the silo contrasts greatly with that of a pile, as the ones studied in Ref. [1]. Piles have no lateral walls so no Janssen effect is present. Further, the geometry of the pile itself assures that pressure is not homogeneous. As it could be ex- pected, pressure increases linearly from the exte- rior as we move toward the center. Surprisingly, the pressure is not maximum at the center of the pile. Instead, it shows a drop that has been termed “pressure dip” [3]. When one opens an orifice at the base of a silo, the material inside outpours driven by gravity. As stated, if the size of the outlet is a few times that of the flowing particles, an arch may form that jams the flow. As the size of the orifice grows, the prob- ability of arch formation decreases. Eventually, for relatively large orifices, no arches are observed dur- ing the accessible time-scale and the flow seems continuous. Actually, the last statement is currently under debate. Some authors have conjectured that there exist two regimes in the silo discharge. One for ori- fices with radius R < Rc, where Rc is some critical value (in units of the particles’ radii. Since most of the literature concerns disks in 2D or spheres in 3D, I will refer here to the radii of the parti- cles and that of the orifice). In this regime arching 060008-1 Papers in Physics, vol. 6, art. 060008 (2014) / R. Arévalo probability is always bigger than zero and arches are bound to appear. A second regime is claimed to exist for R > Rc, in which the probability to ob- serve a stable arch is zero and the flow is actually continuous. II. Silos, piles and jamming Several works have been devoted in the last years to try to settle the accuracy of this picture, and to obtain the value of Rc for different geometries. In Ref. [4], Zuriguel et al. experimentally study the case of a cylindrical silo filled with spherical particles as well as other shapes (small cylinders with low aspect ratio and rice). They measure the size s of the avalanches, defined as the number of particles fallen between two clogs. It is found that their data are well described by a power law of the form < s >= A/ (Rc −R) γ . (1) This leads them to propose that the avalanche size indeed diverges at Rc (whose value depends slightly on the shape of the particles). For spheres, they find Rc = 4.94 and γ = 6.9. A finite size analysis was carried out in Ref. [5]. To this end, the jamming probability function J (N,R) was defined as the probability that the flow clogs before N particles have fallen. In other words, the probability to observe an avalanche of size N for a given aperture size R. Fixing the value of N, the authors compute the jamming probabil- ity JN (R). For low values of N, JN (R) presents a maximum value of 1 for low R and a minimum value 0 for big aperture size. The transition be- tween these values is fast but smooth, with a well defined slope. Upon increasing N, the transition becomes more abrupt and the slope steepens. A limiting step function as N → ∞ would be the hallmark of a real abrupt transition separating the two regimes at Rc. The authors fit the data to JN (R) = {1 − tanh [α (R−Rc)]}/2, which actu- ally converges to the Heaviside function in the limit α → ∞. However, there is no theoretical justifica- tion for this expression, apart from the good fit. An analogous research in 2D (using spherical particles) was carried out in Ref. [6]. It was found that the data on avalanche size could be fit with the same expression than in the 3D case, with val- ues Rc = 8.5 and γ = 12.7. Nevertheless, a careful finite-size system analysis leads the authors to con- clude that there are no two separated regimes in this case. As in the 3D case, the jamming proba- bility function J (N,R) is used. Also in this case, the data from experiments show an apparent con- vergence toward a step function. However, by a subsequent theoretical analysis, the authors found a limiting function which is smooth and shows a doubly exponential dependence in R. The fact that the experimental data could be fit by Eq. (1) is explained taking into account that the maximum measured avalanche is for R ' 5.5 while the pre- sumed critical value is much higher, Rc = 8.5. To et al. [7] have studied the jamming of disks in 2D in a hopper geometry. Measuring the jam- ming probability defined above, they find that their data can be fitted with several different expres- sions. First, by an independent theoretical analy- sis of their experiment, an expression for JN (R) is found which is formally analogous to the one pro- posed by Janda et al., and does not contain any divergence. However, their data can be well fit by Eq. (1) and an exponential containing a diver- gent term. Being the curves indistinguishable in the range of data available, the conclusion is that the question of the existence of a critical outlet size cannot be settled. Recently, Magalhães et al. have proposed a se- ries of simulations [1, 8] addressing the existence of a critical outlet for the flow of grains in a different geometrical setting. They use a realistic soft par- ticle molecular dynamics method with static fric- tion, which is supplemented with rolling resistance in their contribution to this volume. Briefly, the protocol implemented is as follows: in 2D a pile of grains is created by allowing particles to “rain” over a base of a certain width L, which is used as a mea- sure of the size of the initial piles. Once the pile is stable, a hole of size R is opened at the center of the base and particles flow through it. The pile ends up in one of two possible final states: i) a stable arch appears around the outlet blocking the flow; ii) no arch is formed and the pile collapses com- pletely, only a few particles remain at both sides of the outlet. In both cases, the number of particles fallen is recorded and, in case i), also the height h of the final pile. The authors propose that this scenario can be 060008-2 Papers in Physics, vol. 6, art. 060008 (2014) / R. Arévalo likened to a phase transition between the two regimes. Taking h as an order parameter, the plot h (R) shows three regimes. For small apertures, h is essentially a constant which depends on the size of the initial pile. For big R, the pile collapses and so h = 0. The transition between the two values is gradual for small piles and becomes more abrupt for larger piles. The fluctuations of h as a function of the outlet size present a well defined peak at some value R∗ which depends on the size L of the initial pile. As L grows, R∗ seems to converge to a limiting value, and when extrapolating L → ∞, the authors find a critical outlet size Rc = 5.0. In this case, there is no attempt at a theoretical analysis of the observations that could further sup- port the extrapolation of h (R) to a step function. In their contribution to this volume, the authors revisit this problem with new simulations in which they implement rolling friction, making them more realistic. The main conclusion is that the picture drawn in their first work holds, although a correc- tion in the value of Rc is introduced. III. A critical outlet? Let us, at this point, critically address the results summarized in the previous section. Regarding the 3D silo, the conclusion that there exists a criti- cal outlet size is based on the good fit of the data on avalanche size by Eq. (1). In principle, there is no reason precluding the idea that avalanches keep growing for large orifices, with the probability of arch formation decreasing without ever reaching zero. That this is not observed could be simply due to the limitations of the experimental setup. The observations were carried out keeping the height of material inside the silo constant. This is required to assure steady state conditions and, in particu- lar, that there is always a Janssen effect present (if the height of the material decreases too much, pressure does not saturate). Under this conditions, it was simply not possible to refill the silo in order to measure avalanches bigger that a few million of grains. From a more theoretical perspective, Eq. (1) might seem a bit unsatisfactory. In first place, coef- ficient A lacks a fundamental interpretation, being just the size of the avalanche for an orifice of size R = Rc−1. In second place, the value of the expo- nent γ is rather high compared to what one usually finds in phase transitions; and this holds for both the 2D and 3D silos. Third, the avalanche size should approach zero as the outlet size approaches one, in units of the diameter of the particles. As a matter of fact, other expressions can be found to fit the available data. For example < s >= A(R−1)e(B·R C) gives a good fit with A ' 3.4, B ' 0.04 and C ' 3.8. This expression is not diver- gent and goes to zero as the outlet size approaches that of the particles. Although given without the- oretical motivation, it shows that the present data are not enough to settle the question of the exis- tence of a critical outlet size. A better understand- ing of the process of arch formation and how it is affected by the flow is required to gain insight into this problem. In the case of 2D silos we find, in addition to a wealth of experimental data and careful finite size study, a theoretical insight into the process of arch- ing. In both the independent analysis by To and Janda et al. formally equivalent expressions for the jamming probability are found. This reinforces the conclusion that the avalanche size does not diverge and there is no critical outlet. However, one must consider i) that there are underlying asumptions in the theoretical considerations, and ii) that the available data can be well fit with diverging ex- pressions. More (difficult to obtain) data for ori- fices similar to the putative critical size would be necessary to make a strong statement. It is worth mentioning that the theoretical derivation of the jamming probability in Ref. [6] leads, when applied to a 3D silo, to an expression that does not fit the corresponding experimental data. This could be due to some assumption being valid in 2D but not in 3D. Or, one can also con- sider the possibility that there is no transition in two dimensions, and a critical outlet size appears in three dimensions. This is a perfectly possible scenario, as we know from other phase transitions whose existence depends on the dimensionality of the system. Magalhães et al. propose an analogous study in a radically modified geometry. One can imagine that removes the lateral walls of a 2D silo, then the col- umn of particles collapses and ends up in a pile of certain width. Under these conditions, there is 060008-3 Papers in Physics, vol. 6, art. 060008 (2014) / R. Arévalo no Janssen effect, the pressure is not homogeneous and the dynamics could be very different from that of a silo. In any case, as mentioned in the intro- duction, the probability of arch formation could be drastically affected. Thus, it is not obvious that the conclusions reached for silos should hold in the case of piles. Actually, the conclusion in the previous work, Ref. [8], is that there exists a critical outlet for the flow from piles. The obtained value Rc = 5 is far below to Rc = 8.5, reported by Janda el al. for the 2D silo. Without taking into account the existence or not of a critical outlet, this could be an indication that the two setups are not comparable. In their present contribution, Magalhães et al. report a correction to Rc = 5.3 for a contact model that includes rolling resistance (RR). This is rea- sonable, since particles interacting with RR should interlock more easily, leading to more stable arches. Nevertheless, this new Rc value is still much smaller than the one found for the 2D silo. IV. Avalanche size and flow It may seem difficult to imagine the formation of an arch stable enough to arrest the flow in a silo with a large aperture. Effectively, it appears that the flow will sweep any incipient arch and will continue undisturbed. However, the flow is a tunable feature of the silo, known to vary with the square root of gravity, as manifested in experiments [9–11] and simulations [12]. Gravity can be modified in experiments up to a certain point, and it is always possible in simula- tions, so let us call Γ to the imposed body force on the particles. One can imagine, then, that reduces Γ, thus making the flow slower, even for large aper- tures. Under these conditions, molecular dynamics simulations [12] lead to the conclusion that the size of the avalanches increases with the kinetic energy of the system. This is so because, when reducing the driving force, the particles in the outlet region have more time to dissipate their kinetic energy and form a stable structure that blocks the flow. It is then conceivable that one can have a Γ small enough to allow the particles form a stable arch before being swept by the flow. Should this picture be correct, there would not be a critical outlet size. Arches would simply be less likely to be stabilize as the flow was increased by increasing R. The observation of arches would be limited by the time window allowed by the ex- periments or simulations. In order to shed some light in the process of arching a low Γ, additional simulations with a variable outlet size are currently under way. V. Conclusions In this brief commentary, I have tried to give a per- spective on recent results on the jamming of parti- cle flows in silos and its relation with Magalhães et al. contribution to this volume. It is commonplace that silos get jammed. When the size of the aper- ture is not much larger than that of the particles, arches appear to block the flow. Upon increasing the size of the outlet, arches become scarcer. And for large orifices, they are not seen at all at ac- cessible time scales. The observation of power-law relations between the size of the avalanches and the outlet size sparked the interest in considering a critical-like transition between two regimes: a jamming regime in which arches are bound to ap- pear and block the flow, and a continuous regime in which there are no arches. Both regimes would be separated by a critical outlet size. Magalhães et al. undertake an analogous re- search changing the conditions of the reservoir from which the particles flow. They use piles, which have open boundaries, and introduce new complications to be considered. If not transferable from one an- other, the results in piles and silos will widen our perspective on the clogging of granular particles. Let me, very briefly, summarize my opinion on the existence of a critical outlet: • Experimental data in 3D silos are compatible with a transition from a jammed to a contin- uos flow regime at a certain value of the out- let. However, descriptions not involving a di- vergence are also possible. So far, we lack a theoretical frame that justifies one view over the other. • Experimental data in 2D silos are also compat- ible with both the existence and the absence of a critical outlet. Some theoretical insights may point toward a picture without a critical 060008-4 Papers in Physics, vol. 6, art. 060008 (2014) / R. Arévalo outlet. However, one should take into account that: - These theoretical insights contain under- lying assumptions. - They are not always based on a complete understanding of the arching process. • Simulations in Refs. [1, 8] on the flow from 2D piles are compatible with the existence of a critical outlet. There is not a theoretical pic- ture in which to understand the results yet. • Due to the disparities in the conditions of the reservoir, it is not a priori clear that results in 2D silos and 2D piles should be comparable. • Based on results of recent simulations in 2D, one can speculate that an arch can always block the outlet irrespective of the flow rate and, hence of R. For large R, these arches are just extremely unlikely. Possible ideas to advance in the future could be: • Obtain more experimental data for R close to the transition in silos and piles. This could eliminate alternative expresions for the avalanche size. • Carry out experiments in inclined silos to mimic reduced gravity. • Investigate the dynamics of particles in the region close to the outlet. Here, simulations should be extremely useful, given that one has access to all the variables involved. • Extend the study of piles to three dimensions and diverse conditions, as reduced gravity. 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