Large Extra Dimension Planck Scale
Introduction: What this calculator does
In the Arkani-Hamed–Dimopoulos–Dvali (ADD) scenario, gravity propagates in 4 + n spacetime dimensions while Standard Model fields remain confined to a 3+1 dimensional brane. The observed (effective) weakness of gravity in four dimensions can then arise from the fact that gravitational flux “spreads out” into the extra-dimensional volume.
This calculator connects the higher-dimensional fundamental Planck scale (often written M★, entered here in TeV) to the common compactification radius R of n equal-size, flat, compact extra dimensions. It returns R in meters (and typically also millimeters if your results panel supports it).
Core relation (ADD with an n-torus)
For n extra dimensions compactified on an n-torus with common radius R, a commonly used convention relates the reduced 4D Planck mass () to the fundamental (4+n)-dimensional scale () through the extra-dimensional volume factor:
In this convention: .
Written in MathML:
Solving for R gives: .
Units, constants, and conventions
- The input M★ is entered in TeV for convenience (collider-scale intuition). Internally it must be converted to GeV using 1 TeV = 10^3 GeV.
- The calculation uses the reduced Planck mass . (This differs from the non-reduced Planck mass by a factor of .)
- The intermediate result for R from the formula is in GeV−1. Convert to meters using 1 GeV−1 = 1.97327 × 10−16 m.
- Different papers sometimes place factors of differently depending on how the higher-dimensional action is normalized. This page follows the widely used convention shown above.
Interpreting the radius R
The value of R tells you the approximate size of each compact extra dimension in this simplified ADD setup:
- Large R (e.g., microns to sub-millimeter): potentially testable via short-range gravity experiments that look for deviations from Newton’s inverse-square law at small distances.
- Intermediate/small R (e.g., nanometers and below): direct tabletop gravity tests become difficult; constraints typically come from astrophysics/cosmology and high-energy processes (model-dependent).
- Very tiny R: extra dimensions are effectively invisible at accessible distances/energies; the model resembles ordinary 4D gravity over macroscopic scales.
As you increase n at fixed M★, the required R generally decreases quickly. Conversely, lowering M★ (toward the TeV scale) tends to increase R.
Worked example
Example inputs: M★ = 10 TeV, n = 2.
- Convert: .
- Compute the dimensionless ratio inside the parentheses: .
- Take the power (here square root) and divide by to get in GeV−1, then multiply by to get meters.
Numerically, this lands in the neighborhood of (tens of microns) for this specific convention—squarely in the regime where short-distance gravity tests are relevant. Your exact displayed value depends on rounding and the constants used.
Quick comparison table (how R changes)
The table below summarizes the qualitative trend at fixed : increasing n reduces the required radius for a given fundamental scale.
| n (extra dimensions) | If M★ is fixed | Typical effect on R | What it often implies |
|---|---|---|---|
| 2 | TeV-scale M★ | Largest R among common n | Most accessible to sub-mm gravity tests |
| 3–4 | TeV-scale M★ | Smaller R (rapidly shrinking) | Constraints become more model/astrophysics driven |
| 5–7 | TeV-scale M★ | Very small R | Hard to probe directly at distances; relies on high-energy signatures |
Limitations and assumptions
- Geometry: assumes n flat extra dimensions compactified on an n-torus with a single common radius R. Realistic models can have different radii, shapes, curvature, or warping.
- Convention dependence: the factor and the use of the reduced Planck mass are conventional choices. Other normalizations shift the numerical value of R by order-one factors.
- No phenomenology: this is an algebraic back-of-the-envelope mapping between scales; it does not compute collider cross sections, KK spectra details, astrophysical bounds, or cosmological constraints.
- Effective theory: treating gravity in 4+n dimensions with a sharp compactification radius is an effective description; UV completion details (string scale, strong coupling, brane effects) are not included.
- Input ranges: extremely small M★ or very large n can push the calculation into regimes where the simple ADD picture may be inconsistent with existing constraints or with the underlying assumptions.
Tip
If you are comparing to a paper, verify whether it uses or , and whether the volume factor is written as or . Those choices can change the quoted radius by factors of and .
How to use this calculator
- Enter Fundamental scale M★ (TeV) using the unit or time period shown by the field.
- Enter Number of extra dimensions n using the unit or time period shown by the field.
- Run the calculation and compare the output with a second scenario before acting on it.
Formula: how the estimate is built
The result can be read as result = f(a, b), where those inputs represent Fundamental scale M★ (TeV), Number of extra dimensions n. Keep money, time, distance, percentage, and count fields in the units requested by the form.
Arcade Mini-Game: Large Extra Dimension Planck Scale Calibration Run
Use this quick arcade run to practice separating useful scenario inputs from common planning mistakes before you rely on the calculator output.
Start the game, then use your pointer or arrow keys to catch useful inputs and avoid bad assumptions.
