Chapter 3
Endoplasmic Reticulum- and Plasma-Membrane-Driven Calcium Oscillations
Arthur Sherman
Laboratory of Biological Modeling, NIDDK, National Institutes of Health, USA
3.1 Introduction
Calcium () is of great importance throughout biology because it regulates many processes. In neuroendocrine cells, it plays a central role as the main trigger of hormone and peptide secretion. In the experimental literature, one often finds statements along the lines of “Agent X increases concentration (), which increases secretion”. However, secretion is generally not controlled by a mere rise and fall of concentration, but rather by oscillations, and “Agent X” works by changing the pattern of those oscillations.
One of the key contributions of theorists has been to develop models that explain the mechanisms behind such oscillations and how they are regulated. Indeed, there are multiple mechanisms, so it is helpful to distinguish their origins and how they are regulated. In particular, we find oscillations that reflect variation in influx and arise from ion channels at the plasma membrane (PM), as well as oscillations that reflect release from internal stores and arise from ion channels in the membrane of the endoplasmic reticulum (ER). A particularly interesting scenario, where the analytical power of models really shines, is when both mechanisms are present in the same cell and interact with each other.
Our objectives are limited. We will consider simplified examples that illustrate the basic principles rather than aim to model in detail any particular system. An understanding of these principles will provide good preparation to tackle particular problems in the future. Our focus is cellular; other chapters will address systems level models that involve multiple cell types and organs. We also limit ourselves to temporal phenomena, modeling cells as spatially homogeneous. This is often adequate, sometimes not. Mathematically, this means that we only need to deal with ordinary differential equations (a single independent variable, time), rather than partial differential equations (time plus one or more spatial dimensions.) We also treat only deterministic systems, which leaves out the sometimes important effects of noise, but allows us to make good use of dynamical systems tools, such as phase planes and bifurcation diagrams (BDs).
3.2 Calcium balance equations
3.2.1 Derivation
The fundamental physical principle needed to model calcium dynamics in cells is the conservation of mass, which is determined by flux across boundaries. In physics, flux is the rate of flow of some quantity per unit area (http://en.wikipedia.org/wiki/Flux). As we will be dealing with small round cells with a fixed boundary, it is convenient to multiply implicitly by the cell surface area, giving just quantity per time, symbolized by . Our goal is to calculate the changes in the cytoplasmic or intracellular concentration, , denoted here more simply as , which means that we must divide by the cytosol volume to convert the rate of flux to the rate of change of concentration. The cytosol volume can be taken to be fixed, so that we can further simplify by absorbing the volume into the flux; we denote this scaled flux by .
Cells can often (but not always) be well approximated with two compartments: one for the cytosol and one for the ER, as shown in Figure 3.1. The cytosolic , , then satisfies the equation
where we are using the volume-scaled fluxes.
The factor accounts for the fact that most of the that enters a cell is buffered, that is, complexed with -binding proteins. Typically, only about 1% of the ions that enter remain free, which means that the rate of increase of the free concentration is only 1% of what it would be in the absence of buffering. This keeps the free concentration low and prevents runaway activation of the many reactions that are regulated by . This form of the equation is valid only because the buffering reactions are much faster than fluxes, so that it is safe to assume that free and bound are in the quasi-steady state. (A more complete derivation of this can be found in Sherman et al. (2002)).
The equation for ER , , can be similarly written as
Note that the ER gets its own fraction of free , which may differ from that in the cytosol. Also, because we absorbed the cytosolic volume into the fluxes, we have to multiply by the cytosolic-ER volume ratio to get the correct effect of the flux on . The ER volume is much smaller than that of the cytosol, so that the concentration change due to the flux will be much greater in the ER. However, the ER concentration is much greater, so the most typical case is small relative changes in the ER that result in large relative changes in the cytosol. We can make Equation (3.2) look much better, and reduce the number of parameters from 4 to 2, by multiplying the right-hand side by :
where
3.2.2 Applications
We will flesh out the equations (3.1) and (3.3) and incorporate them into more complex models shortly, but pause here to show that even these simple equations can be used to draw nontrivial conclusions.
We choose the following expressions for the fluxes:
where PMCA is the “plasma-membrane calcium ATPase,” which pumps out of the cell, and SERCA is the “sarco-endoplasmic reticulum calcium ATPase,” which pumps into the ER. We assume that flux out of the ER is a passive, diffusive leak. Equations (3.4) and (3.5) correspond to Equation (2.15), Chapter 2, this volume, for bulk cytosolic , except that the plasma-membrane calcium current is for the moment constant, not voltage dependent. In general, the pump expressions are not linear, but rather saturating Hill functions, but these are not needed for the moment. There may also be multiple plasma-membrane currents (e.g., L-type and T-type currents, as described in Chapter 2, Equations (2.6) and (2.7)), multiple ER channels (e.g., IP3 and Ryanodine receptors), and more than one efflux component (e.g., the – exchanger in addition to PMCA).
In Figure 3.2, the black curves show the effect of partial (50%) block of the SERCA pump, such as with thapsigargin, by cutting in half. For simplicity, we assume that the block becomes fully effective instantaneously at min. Then, rises to a peak and then recovers to baseline. One often hears or reads something like “thapsigargin was used to increase ,” but the simulation shows that such an increase is only transient because the released from the ER to the cytosol is pumped out of the cell, leaving the ER depleted (in proportion to the inhibition of SERCA) but the cytosol at its original level once equilibrium is re-established. It is simple to show that the rise in must be transient: setting Equation (3.3) to steady state gives
and substituting this into Equation (3.1) and setting to the steady state implies that
Thus, the ER terms drop out of the equation, and the steady-state value of depends only on the parameters of and . We conclude that cannot be affected by the change in . The same would be true if we had emptied the ER by increasing efflux, which could correspond to the activation of IP3 or Ryanodine receptors. This is in general enough that it is worth stating as a theorem that holds independent of our choices for the fluxes:
A maintained change in is illustrated by the red curve in Figure 3.2. In that simulation, is increased in magnitude at the same time that the PMCA is inhibited; this could correspond, for example, to a store-operated current (SOC) activated by the reduction in (Hogan et al., 2010). The combination of the two effects results in an increase in at the steady state. Conversely, if one observes a steady state increase in when SERCA is inhibited in an experiment, one can be sure that a plasma-membrane ion current was affected (though not necessarily SOC).
The inability of to affect steady state is not due to the depletion of the ER (indeed, we deliberately only depleted it partially in Figure 3.2 to emphasize this point), but to the fact that is constant. The reader may check this explicitly by solving for in terms of in Equations (3.1) and (3.3) using the expressions in Equations (3.4)–(3.7).
We now illustrate that Theorem 3.2.1 does not hold when the system is not in steady state. In Figure 3.3, the black curves show the response to a train of square pulses of ; this represents roughly the effect of a train of action potentials. The red curves show the response when SERCA is partially inhibited. The pulses of are larger in amplitude. This happens because more of the that enters with each pulse stays in the cytosol instead of going into the ER. Theorem 3.2.1 does not apply because fluctuates too rapidly for the system to reach steady state during each pulse.
Note that there are two time constants evident in Figure 3.3: with each pulse, jumps up rapidly and then rises slowly. The rapid jumps reflect the fast intrinsic kinetics of , whereas the slow rise reflects the slow kinetics of , which pushes up slightly with each pulse as the ER fills. The slow kinetics of the ER are also manifest in the slow rise (black) and slow fall (red) of the envelope of as the ER fills or empties. The mean trend of , however, averaged over the rapid fluctuations, does approach approximately the same level irrespective of the fact whether the pump is inhibited or not. That is, Theorem 3.2.1 applies approximately to the averaged system.
3.3 ER-driven calcium oscillations
3.3.1 Closed cell
The model we have considered so far has a very limited repertoire because it is linear. There is a unique steady state, and the most the system can do is relax to that steady state exponentially or as a sum of exponentials. Put in other terms, the model has only negative feedback, embodied in the SERCA and PMCA pumps, which suppresses any fluctuation of away from rest. There is a strongimperative to keep stable, but some cells have evolved the ability to generate and profit from controlled large excursions away from rest. In order to obtain more dynamic responses, we need to make the model nonlinear, specifically to add positive feedback. We do this by postulating that increases the flux out of the ER, often referred to as “calcium-induced calcium release” (CICR). Moreover, the negative feedback, which is needed to limit and terminate the excursions, has to develop slowly enough that it does not cancel out the rise in too soon. We have already encountered examples of oscillations mediated by fast positive feedback combined with slow negative feedback in Chapter 1, McCobb and Zeeman, and Chapter 2, Bertram et al., where they were the bases of action potentials. Indeed, the model we introduce here has much in common with those electrical oscillators, though it works via rather than the membrane potential.
IP3 regulation of ER
A simple example of cytosolic oscillations is the model of Li and Rinzel (1994), which is a simplification of the model of DeYoung and Keizer (1992). This will serve as an exemplar of a wide class of models based on the IP3 receptor (IP3R), an internal receptor located on the ER membrane, which opens in response to the second messenger IP3. IP3 in turn is produced by the activation of a G-protein-coupled receptor (GPCR) on the plasma membrane that responds to an external signal, such as acetylcholine or GnRH; the GPCR is coupled to phospholipase C via G, which forms IP3 from phosphatidylinositol 4,5-bisphosphate (PIP2). The IP3R is moreover a ligand-gated channel; IP3 opens the channel and allows to flow down its concentration gradient from the ER to the cytosol. Thus, one way to introduce positive feedback is to assume that IP3 production is stimulated by rises in . This was the basis of the earliest models for oscillations (Meyer and Stryer, 1988; Swillens and Mercan, 1990). DeYoung and Keizer, in contrast, motivated by reports that could oscillate even when IP3 is held fixed, proposed that enhanced the activity of the IP3R directly. Both effects of are known to exist, and there has been a long, yet unresolved debate about which is more important, or whether they each occur in different types of oscillations. We will not enter that debate here, but simply use the hypothesis of DeYoung and Keizer as a learning tool.
Modeling the role of IP3
Bezprozvanny et al. (1991) showed that the steady state open probability of the IP3R was a bell-shaped function of , which suggested that in high concentrations inactivates the channel. DeYoung and Keizer proposed that this inactivation provides negative feedback beyond that of SERCA to terminate the spike, and that its time scale controls the period of the oscillation. They developed a model with eight states, for all the combinations of activating , activating IP3 and inactivating , bound or unbound.
Li and Rinzel (1994) simplified this in the following formula:
where
is the concentration of IP3, treated as a parameter; and is the fraction of available IP3 receptors, that is, the fraction not inactivated by binding . satisfies the differential equation
where
Equations (3.8) and (3.9) together say that the IP3R open probability is for fixed an increasing function of [IP3] and , but decreases over time as receptors inactivate. This was deliberately formulated to highlight its similarity to the conductance of the voltage-dependent channel, described in Chapter 2, Equation (2.1), which increases with the membrane potential but inactivates over time.
We can now assemble the pieces to specify the Li–Rinzel model, taking Equations (3.1) and (3.3) with Equation (3.8) in place of Equation (3.7) and
in place of Equation (3.6) (not strictly necessary but customary and more accurate). The equations for and then become
Finally, we add Equation (3.9) for receptor inactivation.
This system with three dependent variables (, , and ) can be simplified by assuming that the cell is closed, that is, that the fluxes across the plasma membrane, and are 0. This serves two purposes. First, it emphasizes that the oscillations only require flux in and out of the ER. Second, it reduces the number of equations to 2. The total content of the cell is
where takes into account the differences in ER and cytosolic volume and buffering. This quantity is constant when the cell is closed: its time derivative is 0, as can be verified by multiplying Equation (3.3) by and adding to Equation (3.1). This reduction to two equations now allows us to use phase planes, shown in Figure 3.4, to understand the behaviors. (The concept and usage of phase planes are explained in Chapter 1, McCobb and Zeeman.)
We solve the model equations for and (but can recover from Equation (3.12) should the need arise; see Figure 3.6). The left column shows the phase planes for three values of [IP3], and the right column shows the corresponding timecourses. The nullcline (blue) is obtained by setting the right-hand side of Equation (3.9) to 0 and solving for as a function of . It decreases monotonically, reflecting the increase of inactivation with (see Equation (3.9)).
The nullcline (red) is obtained by setting the right-hand side of Equation (3.1) to 0. Conceptually, we want to solve for as a function of , but that equation can have up to three solutions for some values of , so it is easier to solve for as a function of . The nullcline is, thus, defined by
where we have neglected the small terms and in the second line (the latter is valid as long as is not too small). The resulting curve has a distorted N shape, increasing for small , then decreasing, and then increasing again. The left branch of the nullcline has a steep slope because as . The N shape results from the competition between activation, , of the receptor, which increases , and SERCA, , which refills the ER. The general trend is for to increase due to SERCA, but in the range where the IP3R is strongly activated, turns down. This is typical for activator–inhibitor systems, where the positive feedback mechanism creates a kink in the activator variable nullcline and thereby creating instability and oscillations. In Hodgkin–Huxley-type systems, the activation of the current plays the same role. In that context, it creates a dip in the current–voltage relation, which translates to a negative resistance and gives away its role as the source of dynamism.
The intersection of the two nullclines is the steady state, and in each row there is only one. Increasing IP3 pulls down the nullcline because is an increasing function of and moves the steady state along the nullcline. In the top row, M, the steady state is on the rising left branch of the nullcline, and is therefore stable. The trajectory (black) swings around from the upper right to end at the steady state, producing a single transient spike and then steady , as shown in the right panel. In this state, the system is not oscillatory but is said to be excitable, meaning that a suitable perturbation away from the rest state is amplified into a spike rather than returning immediately to rest.
For M, the steady state is on the rising right branch of the nullcline and is again stable, but the approach to rest is a damped oscillation. In order to get sustained oscillations, the steady state must be destabilized, which is guaranteed if it lies on the falling middle branch of the nullcline. This is the case for M, shown in the middle panels. The trajectory now takes the form of a closed curve (a limit cycle, see Chapter 1, McCobb and Zeeman) that orbits around the steady state.
The phase plane also explains a characteristic feature of the oscillation, namely that the spikes are narrow and the interspike intervals are long. This happens because the trajectory is closer to the unstable steady state during the interspike portion, and the flow is therefore slow. The period decreases markedly as IP3 is increased within the oscillatory range because the steady state moves to the right, away from the low values traversed during the interspike period (compare M to M in Figure 3.4). Thus, it is not difficult for models like this to capture the frequency encoding observed experimentally as the IP3-generating stimulus is varied (Goldbeter et al., 1990).
If we stack a series of phase planes like those in Figure 3.4 and plot the values of (the steady states as well as the minima and maxima of the periodic orbits when those are present), we get Figure 3.5. A similar picture would be obtained if were plotted against IP3, so we omit the third dimension. The line shows the steady states, solid and black for stable, dashed and red for unstable. The green dotted line shows the average during spiking, and the filled circles the amplitude of the oscillations, which exist for a range of values of IP3, or between lower and upper thresholds. Those thresholds are labeled “HB” for Hopf bifurcation, which indicates the particular way in which the steady state goes unstable (see Chapter 1, McCobb and Zeeman). The existence of upper and lower thresholds, dividing the system behaviors into off, oscillating and fully on, is a ubiquitous feature of activator–inhibitor systems.
The peak of the oscillation is in most cases higher than the steady level when is above the upper threshold, but the average is lower. The model thus suggests that if one could measure experimentally but not IP3, then the average would be a better indicator of the IP3 level (or “activity”) than the peak.
3.3.2 Open cell
Suppose now that the cell is open. Now during each spike, some of the will be pumped out of the cell rather than back into the ER. Unless there is some influx to balance the efflux, the ER would eventually empty out and oscillations would cease. We restore the plasma-membrane fluxes, setting to a constant and introducing a saturating PMCA pump: