Ekpyrotic Cycle Duration Calculator

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Brane Collisions and the Cyclic Quest for a Smooth Cosmos

The ekpyrotic scenario is an audacious alternative to the inflationary big bang. Instead of a singular explosive birth, our universe may be one slice of a higher-dimensional stack of membranes—branes—that periodically drift together and collide. Each collision unleashes a fireworks display of radiation and matter, re-sculpting the cosmos before the branes rebound and drift apart again. This repeated drama of approach, impact, and recession gives rise to a cyclic universe in which time extends infinitely into the past and future, with each cycle smoothing the universe and seeding new structures.

Key to this tale is the strange behavior of the brane world just before collision. In the ekpyrotic phase, the universe is dominated by a stiff form of energy with an equation-of-state parameter \(w\gg1\). Rather than ballooning like inflation, space contracts gently. Yet this contraction is special: anisotropies and spatial curvature are suppressed because their energy densities scale more quickly than the ekpyrotic field. When the branes finally meet, the universe emerges astonishingly flat and homogeneous despite the absence of an inflationary blast. Our calculator provides a tiny sandbox for exploring this imaginative model. By specifying the initial separation between branes, their relative speed, and the value of \(w\), you can estimate how long a full cycle lasts and how potent the smoothing effect becomes.

The setup imagines two parallel three-dimensional branes separated by a minuscule gap in a higher-dimensional bulk. They creep toward each other with relative speed \(v\), measured as a fraction of the speed of light \(c\). If their initial separation is \(D\), the time until impact in the bulk frame is simply \(t_{\text{coll}} = D/(v c)\). In many ekpyrotic models the branes bounce after collision, retreating to their starting positions before the dance begins anew. A full cycle—from one collision to the next—therefore lasts approximately \(T_{\text{cycle}} = 2D/(v c)\). Converting these intervals into years provides a sense of how languid the cosmological rhythm can be. Even for separations measured in micrometers the cycle spans far longer than a human lifetime, underscoring how gentle the brane motion must be to avoid catastrophic tidal distortions.

While timekeeping is straightforward, quantifying the smoothing power of ekpyrotic contraction is subtler. The suppression of spatial curvature, anisotropy, and relics depends on the number of e-folds of ekpyrotic contraction experienced before the crunch. In simple models this is tied to the equation-of-state parameter \(w\) and the duration of contraction. A rough estimate treats the Hubble parameter during contraction as \(H \approx v c / D\). The number of e-folds is then \(N \approx |H| t_{\text{coll}} = v c / D \times D/(v c) = 1\): even a single e-fold in this toy model provides significant smoothing when \(w\) is large. More realistically, we account for the stiff equation of state by amplifying this result, defining a smoothing factor \(S = \exp[3(1+w)N]\). This captures how rapidly anisotropies are diluted relative to the ekpyrotic field. Because \(w\) can reach values of a hundred or more, \(S\) becomes enormous, signaling a dramatic flattening of the universe.

The calculator implements this cartoon by taking the user-provided \(w\) and multiplying the base e-fold count by \(3(1+w)/2\), recognizing that contraction spans half a full cycle. We also anchor the scale using the Planck length \(\ell_P \approx 1.616\times10^{-35}\) m. The resulting expression for the effective smoothing e-folds is \(N_{\text{eff}} = \frac{3}{2}(1+w)\ln(D/\ell_P)\). Although this relation is heuristic, it reproduces the qualitative expectation that greater separations and larger \(w\) dramatically heighten smoothing. Feeding this into \(S = e^{N_{\text{eff}}}\) yields fantastically large numbers even for modest inputs, emphasizing how the ekpyrotic phase can erase primordial wrinkles without inflation.

From these quantities we can infer a residual curvature parameter \(\Omega_k \sim e^{-2N_{\text{eff}}}\). This dimensionless number gauges how close the post-bounce universe is to perfect spatial flatness. Values far below unity imply an exceedingly smooth cosmos. The calculator reports \(N_{\text{eff}}\), the smoothing factor \(S\), and the estimated curvature parameter to show how sensitive each is to the chosen inputs. While the formulas are simplistic, they highlight the conceptual mechanism: lengthy contraction with a very stiff equation of state suffices to iron out the universe before each fiery rebirth.

To make the toy model more tangible, consider an initial separation of one micrometer and a relative speed of \(0.1c\). The collision occurs after roughly \(3.3\times10^{-14}\) seconds. Doubling this to account for the rebound yields a full cycle of \(6.6\times10^{-14}\) seconds—astonishingly brief on human scales yet ages to microscopic branes. Plugging \(w=100\) into the smoothing formula gives \(N_{\text{eff}}\approx 124\). The corresponding smoothing factor is about \(e^{124}\), an immense number near \(10^{53}\). The curvature parameter becomes \(e^{-248}\), effectively zero. Tweaking the separation or \(w\) quickly sends these quantities to extremes.

The table below enumerates three sample scenarios. The first uses the default values just discussed. The second explores a slower approach with \(v=0.01c\), extending the cycle time. The third considers a larger separation of ten micrometers while maintaining \(w=50\). The table lists the computed half-cycle time, full period, effective e-folds, and residual curvature parameter. Because the numbers span many orders of magnitude, scientific notation is employed for clarity.

D (μm)v/cwtcoll (s)Tcycle (s)NeffΩk
10.1100
10.01100
100.0550

Critics of ekpyrotic cosmology note that rendering these ideas concrete requires a complete theory of the bounce—the moment when the branes pass through each other and re-emerge. Issues like entropy production, relic generation, and the stability of the extra dimension demand sophisticated mathematics beyond this playful calculator. Nevertheless the exercise illuminates a curious possibility: our universe may have been born not from a unique big bang but from an endless series of collisions in a hidden dimension. If so, calculating the cycle time and smoothing power becomes more than a parlor trick—it hints at the heartbeat of a cosmos without beginning or end.

The calculator is intentionally speculative. The formulas mix heuristic reasoning with dimensional analysis and should not be taken as definitive predictions. Their purpose is to spark curiosity about alternative cosmologies and to highlight the remarkable creativity of theoretical physics. Whether inflation, ekpyrosis, or some other mechanism describes the earliest moments, exploring these models expands our imagination about the ultimate origin of space and time.

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