Pair Production Threshold Calculator

Find the threshold energy for two photons colliding to produce an electron-positron pair, γγ→e⁺e⁻.

✨ Pair Production Threshold Calculator
MeV
°
Threshold E₁
Total threshold (E₁+E₂)
Step-by-step working

✨ What is the Pair Production Threshold Calculator?

This pair production threshold calculator finds the minimum photon energy needed for two photons to collide and produce an electron-positron pair (γγ→e⁺e⁻). Enter the second photon's energy and the collision angle, and it returns the threshold energy of the first photon.

E₁E₂(1−cosθ) ≥ 2(m_ec²)² is the exact relativistic threshold condition, and this calculator solves it for E₁ given E₂ and θ.

The famous case of two equal-energy photons colliding head-on requires a total of exactly 1.022 MeV (twice the electron rest energy), the most efficient geometry for this process.

This calculator is useful for particle physics and gamma-ray astronomy students studying photon-photon interactions and the astrophysical gamma-ray horizon.

📐 Formula

E₁E₂(1−cosθ)  ≥  2(mec²)²
E₁, E₂ = the two photon energies
θ = angle between the photons' directions
me = 0.511 MeV, electron rest energy
Example: symmetric head-on (E₂=0.511 MeV, θ=180°): E₁=0.511 MeV, total=1.022 MeV exactly.

📖 How to Use This Calculator

Steps

1
Enter the second photon's energy.
2
Enter the collision angle.
3
Read the threshold energy.

💡 Example Calculations

Example 1 - Symmetric head-on collision (the famous 1.022 MeV case)

1
E₂=0.510999 MeV (=mec²), θ=180° (head-on)
2
E₁ = 0.510999 MeV exactly
3
Total threshold = 1.021998 MeV, the famous 1.022 MeV value
Total = 1.021998 MeV
Try this example →

Example 2 - Asymmetric head-on collision

1
E₂=1.0 MeV, θ=180° (head-on)
2
E₁ = 0.261120 MeV
3
A more energetic second photon lowers the required first-photon energy
E₁ = 0.261120 MeV
Try this example →

Example 3 - Perpendicular (90°) collision

1
E₂=0.510999 MeV, θ=90°
2
E₁ = 1.021998 MeV
3
Exactly double the head-on threshold, since (1−cos90°)=1 is half of (1−cos180°)=2
E₁ = 1.021998 MeV
Try this example →

❓ Frequently Asked Questions

What is pair production?+
Pair production is the creation of a particle-antiparticle pair, most commonly an electron and a positron, from pure energy. In the photon-photon process (γγ→e⁺e⁻) calculated here, two photons collide and convert their energy directly into the rest mass and kinetic energy of the new electron-positron pair.
What is the formula for the pair production threshold?+
E₁E₂(1−cosθ) ≥ 2(m_ec²)², where E₁ and E₂ are the two photon energies, θ is the angle between their directions of travel, and m_ec² is the electron rest energy (0.511 MeV). This calculator solves for the minimum E₁ given E₂ and θ.
Why is 1.022 MeV such a famous number in this context?+
1.022 MeV is exactly twice the electron rest energy (2 × 0.511 MeV), and it is the minimum TOTAL photon energy needed for pair production in the special, most efficient case: two photons of equal energy colliding exactly head-on (θ=180°). This is one of the most quoted numbers in particle physics.
Why does a single photon never pair-produce on its own in a vacuum?+
A single photon cannot simultaneously conserve both energy and momentum while converting into two massive particles in a vacuum, there is always a reference frame where the photon's energy is insufficient, or momentum fails to balance. A second photon (or a nearby nucleus to absorb recoil momentum) is required.
Why does a head-on collision require the least energy?+
The (1−cosθ) term is maximized (equal to 2) exactly at θ=180° (head-on), meaning the same product E₁E₂ is most "efficient" at producing pairs in this geometry. At smaller angles, (1−cosθ) shrinks, so a larger E₁E₂ product (and therefore more total energy) is needed to reach the same threshold.
What is the "gamma-ray horizon" and how does this relate to pair production?+
Very-high-energy gamma rays traveling across cosmological distances can pair-produce against the diffuse extragalactic background light (starlight and infrared light filling the universe), effectively absorbing the gamma ray. This creates a "horizon" beyond which the highest-energy gamma rays from distant sources cannot reach us, a major consideration in gamma-ray astronomy.
Does this calculator apply to particle pairs other than electron-positron?+
As written, this calculator uses the electron rest energy specifically, since electron-positron pair production is by far the most common and lowest-threshold case (electrons being the lightest charged particle). The same formula structure applies to heavier pairs (like muon-antimuon) by substituting the appropriate rest energy, though that isn't what this specific calculator computes.
What angle gives the highest pair production threshold?+
As θ approaches 0° (photons traveling in nearly the same direction), (1−cosθ) approaches zero, driving the required threshold energy toward infinity, physically meaning two photons traveling almost parallel essentially never pair-produce, matching the intuition that they need to genuinely collide, not just travel alongside each other.
Is pair production the reverse of electron-positron annihilation?+
Yes, exactly, electron-positron annihilation (e⁺e⁻→γγ) converts a particle-antiparticle pair into two photons, while pair production (γγ→e⁺e⁻) runs this process in reverse, converting photon energy back into a particle-antiparticle pair. Both processes obey the same underlying conservation laws.
Why must the products be a particle and its antiparticle?+
Photons carry zero net electric charge, and since charge must be conserved, they can only produce a particle-antiparticle pair (equal and opposite charge, summing to zero) rather than any arbitrary pair of massive particles. This is why the process specifically produces electron-positron pairs, not, say, two electrons.

What is pair production?

Pair production is the creation of a particle-antiparticle pair, most commonly an electron and a positron, from pure energy. In the photon-photon process (γγ→e⁺e⁻) calculated here, two photons collide and convert their energy directly into the rest mass and kinetic energy of the new electron-positron pair.

What is the formula for the pair production threshold?

E₁E₂(1−cosθ) ≥ 2(m_ec²)², where E₁ and E₂ are the two photon energies, θ is the angle between their directions of travel, and m_ec² is the electron rest energy (0.511 MeV). This calculator solves for the minimum E₁ given E₂ and θ.

Why is 1.022 MeV such a famous number in this context?

1.022 MeV is exactly twice the electron rest energy (2 × 0.511 MeV), and it is the minimum TOTAL photon energy needed for pair production in the special, most efficient case: two photons of equal energy colliding exactly head-on (θ=180°). This is one of the most quoted numbers in particle physics.

Why does a single photon never pair-produce on its own in a vacuum?

A single photon cannot simultaneously conserve both energy and momentum while converting into two massive particles in a vacuum, there is always a reference frame where the photon's energy is insufficient, or momentum fails to balance. A second photon (or a nearby nucleus to absorb recoil momentum) is required.

Why does a head-on collision require the least energy?

The (1−cosθ) term is maximized (equal to 2) exactly at θ=180° (head-on), meaning the same product E₁E₂ is most 'efficient' at producing pairs in this geometry. At smaller angles, (1−cosθ) shrinks, so a larger E₁E₂ product (and therefore more total energy) is needed to reach the same threshold.

What is the 'gamma-ray horizon' and how does this relate to pair production?

Very-high-energy gamma rays traveling across cosmological distances can pair-produce against the diffuse extragalactic background light (starlight and infrared light filling the universe), effectively absorbing the gamma ray. This creates a 'horizon' beyond which the highest-energy gamma rays from distant sources cannot reach us, a major consideration in gamma-ray astronomy.

Does this calculator apply to particle pairs other than electron-positron?

As written, this calculator uses the electron rest energy specifically, since electron-positron pair production is by far the most common and lowest-threshold case (electrons being the lightest charged particle). The same formula structure applies to heavier pairs (like muon-antimuon) by substituting the appropriate rest energy, though that isn't what this specific calculator computes.

What angle gives the highest pair production threshold?

As θ approaches 0° (photons traveling in nearly the same direction), (1−cosθ) approaches zero, driving the required threshold energy toward infinity, physically meaning two photons traveling almost parallel essentially never pair-produce, matching the intuition that they need to genuinely collide, not just travel alongside each other.

Is pair production the reverse of electron-positron annihilation?

Yes, exactly, electron-positron annihilation (e⁺e⁻→γγ) converts a particle-antiparticle pair into two photons, while pair production (γγ→e⁺e⁻) runs this process in reverse, converting photon energy back into a particle-antiparticle pair. Both processes obey the same underlying conservation laws.

Why must the products be a particle and its antiparticle?

Photons carry zero net electric charge, and since charge must be conserved, they can only produce a particle-antiparticle pair (equal and opposite charge, summing to zero) rather than any arbitrary pair of massive particles. This is why the process specifically produces electron-positron pairs, not, say, two electrons.