Mandelstam Variables Calculator

Calculate the Mandelstam variables s, t, and u for massless 2-to-2 particle scattering from the center-of-mass energy and angle.

📐 Mandelstam Variables Calculator
GeV
Scattering angle (θ)90°
degrees
180°
s (Mandelstam s)
t (Mandelstam t)
u (Mandelstam u)
Check: s + t + u
Step-by-step working

📐 What is the Mandelstam Variables Calculator?

This Mandelstam variables calculator computes the three Lorentz-invariant kinematic variables s, t, and u for a massless 2-to-2 particle scattering process, given the center-of-mass energy √s and the scattering angle θ.

Mandelstam variables are the standard language for describing scattering kinematics in particle physics. s (the square of the total center-of-mass energy) sets the energy scale of a collision, resonances in s-channel processes appear as peaks when s equals the square of an intermediate particle's mass. t and u describe momentum transfer in forward and backward exchange (t-channel and u-channel) processes, and are the natural variables in which differential cross sections dσ/dt are written.

A useful sanity check is the identity s + t + u = Σm² (the sum of the squares of all four particle masses in the process). For massless particles, that sum is exactly zero, so a correct calculation always returns s + t + u = 0 up to floating-point rounding.

This calculator is useful for particle physics students working through scattering kinematics problems, and for anyone verifying a hand calculation of s, t, and u for a collider process.

📐 Formula

t  =  −s/2 × (1 − cosθ)     u  =  −s/2 × (1 + cosθ)
s = (√s)², the square of the center-of-mass energy (GeV²)
θ = center-of-mass scattering angle (degrees)
Identity: s + t + u = 0 for massless particles
Example: √s=100 GeV, θ=90°: s=10,000, t=u=−5,000 GeV².

📖 How to Use This Calculator

Steps

1
Enter the center-of-mass energy, √s, in GeV.
2
Enter the scattering angle, θ, between 0° and 180°.
3
Read s, t, and u, the massless-invariant check, and the t/u vs angle chart.

💡 Example Calculations

Example 1 - Symmetric 90° scattering

1
√s = 100 GeV, θ = 90°
2
s = (100)² = 10,000 GeV²
3
t = −10,000/2 × (1−0) = −5,000 GeV², u = −10,000/2 × (1+0) = −5,000 GeV² (equal at 90°, as expected)
s = 10,000 GeV², t = u = −5,000 GeV²
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Example 2 - LHC-scale collision at small angle

1
√s = 13,000 GeV (LHC design energy), θ = 30°
2
s = (13,000)² = 169,000,000 GeV²
3
t ≈ −1.1321×10⁵ GeV², u ≈ −1.5768×10⁹ GeV² (small angle means small |t|, large |u|)
s = 1.6900×10⁸ GeV²
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Example 3 - Full backscattering

1
√s = 200 GeV, θ = 180° (the outgoing particle scatters straight backward)
2
s = (200)² = 40,000 GeV²
3
t = −40,000/2 × (1−(−1)) = −40,000 GeV², u = −40,000/2 × (1+(−1)) ≈ 0 GeV² (the backscattering limit)
t = −40,000 GeV², u ≈ 0 GeV²
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❓ Frequently Asked Questions

What are the Mandelstam variables?+
The Mandelstam variables s, t, and u are three Lorentz-invariant quantities used to describe the kinematics of a 2-to-2 particle scattering or decay process. s is the square of the total center-of-mass energy, while t and u are squared momentum transfers between the incoming and outgoing particles.
What is the formula for s, t, and u in massless 2-to-2 scattering?+
For massless particles, s=(√s)², t=−s/2×(1−cosθ), and u=−s/2×(1+cosθ), where √s is the center-of-mass energy and θ is the scattering angle in the center-of-mass frame.
Why does s + t + u always equal zero for massless particles?+
In general, s+t+u equals the sum of the squares of all four particle masses involved in the scattering. For massless particles that sum is zero, so s+t+u=0 exactly, a useful identity for checking a calculation.
What do s, t, and u physically represent?+
s is the square of the total energy available in the center-of-mass frame (relevant for resonance production). t is the squared momentum transfer in the forward-scattering direction (relevant for t-channel exchange processes). u is the squared momentum transfer in the backward direction (relevant for u-channel exchange processes).
What happens to t and u at forward and backward scattering angles?+
At θ=0° (the outgoing particle continues forward, no deflection), t=0 and u=−s. At θ=180° (the outgoing particle is scattered straight back), t=−s and u=0. These are the two extreme kinematic limits.
Why are t and u negative?+
By convention, t and u represent squared four-momentum transfers for physical (spacelike) exchanges in 2-to-2 scattering, which are negative or zero. Only s, the squared total energy, is positive for a physical process.
Does this calculator work for massive particles?+
This calculator uses the massless approximation, which is highly accurate whenever √s is much larger than all four particle masses, as is typical at high-energy colliders. For scattering near threshold, where masses are comparable to √s, the full mass-dependent Mandelstam formulas are needed instead.
What is a real example use of Mandelstam variables?+
At the LHC, proton-proton collisions at √s=13,000 GeV probe parton-level scattering processes described by s, t, and u. The differential cross section dσ/dt for many QCD and electroweak processes is written directly in terms of these variables.
How is the scattering angle θ defined?+
θ is the polar scattering angle measured in the center-of-mass frame, between the direction of one incoming particle and the direction of one outgoing particle. It ranges from 0° (no deflection) to 180° (full backscattering).
Are s, t, and u independent of each other?+
No, for a 2-to-2 process with fixed masses, only two of the three variables are independent, the third is fixed by the identity s+t+u=Σm². Once you know √s and the scattering angle, all three are determined.

What are the Mandelstam variables?

The Mandelstam variables s, t, and u are three Lorentz-invariant quantities used to describe the kinematics of a 2-to-2 particle scattering or decay process. s is the square of the total center-of-mass energy, while t and u are squared momentum transfers between the incoming and outgoing particles.

What is the formula for s, t, and u in massless 2-to-2 scattering?

For massless particles, s=(√s)², t=−s/2×(1−cosθ), and u=−s/2×(1+cosθ), where √s is the center-of-mass energy and θ is the scattering angle in the center-of-mass frame.

Why does s + t + u always equal zero for massless particles?

In general, s+t+u equals the sum of the squares of all four particle masses involved in the scattering. For massless particles that sum is zero, so s+t+u=0 exactly, a useful identity for checking a calculation.

What do s, t, and u physically represent?

s is the square of the total energy available in the center-of-mass frame (relevant for resonance production). t is the squared momentum transfer in the forward-scattering direction (relevant for t-channel exchange processes). u is the squared momentum transfer in the backward direction (relevant for u-channel exchange processes).

What happens to t and u at forward and backward scattering angles?

At θ=0° (the outgoing particle continues forward, no deflection), t=0 and u=−s. At θ=180° (the outgoing particle is scattered straight back), t=−s and u=0. These are the two extreme kinematic limits.

Why are t and u negative?

By convention, t and u represent squared four-momentum transfers for physical (spacelike) exchanges in 2-to-2 scattering, which are negative or zero. Only s, the squared total energy, is positive for a physical process.

Does this calculator work for massive particles?

This calculator uses the massless approximation, which is highly accurate whenever √s is much larger than all four particle masses, as is typical at high-energy colliders. For scattering near threshold, where masses are comparable to √s, the full mass-dependent Mandelstam formulas are needed instead.

What is a real example use of Mandelstam variables?

At the LHC, proton-proton collisions at √s=13,000 GeV probe parton-level scattering processes described by s, t, and u. The differential cross section dσ/dt for many QCD and electroweak processes is written directly in terms of these variables.

How is the scattering angle θ defined?

θ is the polar scattering angle measured in the center-of-mass frame, between the direction of one incoming particle and the direction of one outgoing particle. It ranges from 0° (no deflection) to 180° (full backscattering).

Are s, t, and u independent of each other?

No, for a 2-to-2 process with fixed masses, only two of the three variables are independent, the third is fixed by the identity s+t+u=Σm². Once you know √s and the scattering angle, all three are determined.