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The energy-momentum relation is a crucial concept in relativistic mechanics. It links the energy of a particle with its momentum and mass, allowing us to derive quantities like energy when momentum and mass are known. Given as:

• \( E = \sqrt{(m c^2)^2 + (pc)^2} \)

This equation stems from Einstein’s theory of relativity. It shows how energy is not merely dependent on mass but also momentum, especially significant at high speeds.
For our case with particle \( a \) and \( b \), using this relation helps us find their respective energies knowing their masses and momenta.
Knowing the energy of the final state particles is key as it helps find the initial state quantities such as total energy and momentum, later used to find the invariant mass.

Invariant mass, often denoted as \( M \), is a scalar quantity that remains the same, irrespective of the reference frame. It's sometimes called rest mass and provides a direct measure of a particle system's "weight".
The invariant mass can be determined using the total energy and momentum of the system through:

• \( M c^2 = \sqrt{E^2 - (pc)^2} \)

Here, \( E \) is the total energy, and \( p \) is the total momentum.
This formula tells us that even though the energy and momentum can vary based on the observer's frame of reference, the invariant mass is constant.
In our particle decay example, knowing the decay products' energies and momenta helps compute the original particle's mass.

Particle decay refers to a process where a particle transforms into other particles. It's a common phenomenon in high-energy physics and is governed by conservation laws.
In the decay process considered in the problem, a particle of unknown mass decays into two particles with known masses and measurable momenta.
Important points to remember about particle decay:

• Conservation of Energy: Total energy before decay equals total energy after.
• Conservation of Momentum: Total momentum before decay equals total momentum after.

By applying these conservation laws, you can find the energy and momentum of the decayed particles and use them to compute unknown quantities, such as the original particle's invariant mass and its speed, using relativistic equations.

Relativistic speed occurs when a particle moves at speeds close to the speed of light, \( c \). At these speeds, traditional velocity calculations using Newtonian mechanics break down, as relativistic effects become significant.
The speed of a particle can be found using the relation:

• \( E = \gamma M c^2 \)
• \( p = \gamma M v \)

Here, \( \gamma \) is the Lorentz factor given by \( \gamma = \frac{1}{\sqrt{1 - (v/c)^2}} \), reflecting how time and length distort at high velocities.
In our calculation, the unknown particle's speed approximates to 0.660c, indicating significant relativistic effects due to its high velocity.
Understanding relativistic speed ensures accurate analysis of a particle's behavior at speeds nearing that of light, crucial in high-energy physics experiments.