43,769,394.7161
m/s
43,423,067.4147
m/s
0.14599899
0.14484376
1.010658
938.2753
MeV
43,769,394.7161
m/s
43,423,067.4147
m/s
0.14599899
0.14484376
1.010658
938.2753
MeV
The Particle Velocity Calculator determines the velocity of a nuclear or subatomic particle from its kinetic energy and mass, providing both classical and relativistic results for comparison. This is the inverse problem to energy calculation and is frequently needed in nuclear physics for computing time-of-flight, reaction kinematics, magnetic rigidity, and detector response.
In the classical approximation, velocity is \(v = \sqrt{2 KE / m}\). This can yield values exceeding the speed of light for high-energy particles, which is physically impossible—a clear signal that relativistic mechanics is required.
The relativistic velocity uses the Lorentz factor \(\gamma = 1 + KE/(mc^2)\) and then \(\beta = \sqrt{1 - 1/\gamma^2}\), giving \(v = \beta c\). This always yields \(v < c\) regardless of how large the kinetic energy becomes. The approach uses energy units throughout: the rest mass energy \(mc^2 = m_{amu} \times 931.494\) MeV.
Comparing classical and relativistic results reveals when relativity matters. For a proton with 10 MeV kinetic energy (about 1% of its rest mass energy), the classical velocity is 4.38×10⁷ m/s (β = 0.146) while the relativistic velocity is 4.35×10⁷ m/s—only 0.5% different. But for a 938 MeV proton (KE = rest mass energy), classical gives \(v = c\) while relativistic gives \(v = 0.866c\)—a 15% error.
This calculator is particularly useful for time-of-flight spectroscopy (measuring particle velocity to determine mass), designing beam transport systems in accelerators, computing Cherenkov radiation thresholds, and analyzing nuclear reaction products. The Lorentz factor and beta parameters are essential inputs for relativistic kinematics calculations.
Input the kinetic energy in MeV and the particle mass in amu for instant results. Common particle masses: proton (1.00728 amu), neutron (1.00866 amu), alpha (4.00260 amu), electron (0.000549 amu).
Classical velocity:
$$v_{class} = \sqrt{\frac{2 \cdot KE}{m}}$$
where KE is in joules and m in kg (converted from MeV and amu internally).
Relativistic velocity:
First compute the Lorentz factor from kinetic energy:
$$\gamma = 1 + \frac{KE}{mc^2} = 1 + \frac{KE_{MeV}}{m_{amu} \times 931.494}$$
Then:
$$\beta = \sqrt{1 - \frac{1}{\gamma^2}}, \quad v = \beta c$$
The rest mass energy is:
$$mc^2 = m_{amu} \times 931.494 \text{ MeV}$$
When classical and relativistic velocities agree closely (β < 0.1), the particle is non-relativistic and classical mechanics suffices. When they diverge significantly, or when classical β > 1 (impossible), relativity is essential. The Lorentz factor γ directly tells you the regime: γ ≈ 1 (non-relativistic), γ = 2 (KE = mc², moderately relativistic), γ ≫ 1 (ultra-relativistic, v ≈ c).
Inputs
Results
A 10 MeV proton has β ≈ 0.145—only mildly relativistic. Classical and relativistic velocities agree to within 0.6%, showing classical mechanics works well at this energy.
Inputs
Results
A 1 GeV electron is ultra-relativistic (γ ≈ 1957, β ≈ 0.9999999). Classical velocity exceeds c by a factor of 196—completely wrong. Relativistic velocity is 99.99999% of c.
The classical formula v = √(2KE/m) has no upper bound—it can give arbitrarily large velocities for high kinetic energies. This is a fundamental failure of Newtonian mechanics at high speeds. Special relativity corrects this by requiring the Lorentz factor, which ensures v < c for any finite kinetic energy.
The classical formula is accurate to better than 1% when KE < 0.01×mc² (or β < 0.14). For protons, this means KE < 9.4 MeV. For electrons (much lighter), it means KE < 5.1 keV. Most alpha particles from radioactive decay (≈4-9 MeV) are borderline, and electrons almost always require relativistic treatment.
Enter mass in atomic mass units (amu). Common values: proton = 1.00728, neutron = 1.00866, electron = 0.000549, alpha = 4.00260, deuteron = 2.01410, muon = 0.11343. The calculator internally converts to kg for classical and uses the amu→MeV/c² conversion (1 amu = 931.494 MeV/c²) for relativistic.
Common methods include: (1) Time-of-flight (TOF): measuring the time for a particle to traverse a known distance, (2) Cherenkov detectors: which detect light emitted when v > c/n, giving β directly, (3) Magnetic rigidity: the radius of curvature in a magnetic field gives momentum, from which velocity follows if mass is known.
The speed of light c = 2.998×10⁸ m/s is the universal speed limit for massive particles. They can approach it arbitrarily closely but never reach it. The most energetic cosmic rays have β = 1 - 10⁻²⁴, meaning they travel at (1 - 10⁻²⁴)×c—unimaginably close to c.
The de Broglie wavelength is λ = h/(mv) classically, or λ = h/(γmv) = h/p relativistically. Lower velocity (and mass) means longer wavelength. This determines whether a particle can resolve nuclear-scale structures: to probe a 1 fm (10⁻¹⁵ m) nucleus, you need λ < 1 fm, requiring hundreds of MeV for protons.
Roboculator Team
The Roboculator Team explains calculations, planning tools, and practical formulas in clear language for real-life situations.
How helpful was this calculator?
Be the first to rate!
Half-Life Calculator
Nuclear & Particle Physics Calculators
Carbon Dating Calculator
Nuclear & Particle Physics Calculators
Decay Constant Calculator
Nuclear & Particle Physics Calculators
Specific Activity Calculator
Nuclear & Particle Physics Calculators
Mean Life Calculator
Nuclear & Particle Physics Calculators
Nuclear Cross Section Calculator
Nuclear & Particle Physics Calculators