Radioactivity: Alpha, Beta & Gamma

In the winter of 1896 Henri Becquerel wrapped a lump of uranium salt with a photographic plate in black paper, meaning to test whether sunlight made the salt glow with X-rays. Paris turned cloudy, so he shut the whole bundle in a drawer and waited for the sun. When he developed the plate anyway — days later, in the dark, with no sunlight ever involved — it carried a sharp black shadow of the uranium crystal. Something was pouring out of that rock on its own, unbidden, needing no light, no heat, no chemistry to switch it on. He had stumbled onto radioactivity: matter that emits penetrating radiation entirely by itself. Over the next four years physicists took that single mysterious emission apart and found it was not one thing but three, with wildly different personalities. One kind is stopped by a sheet of paper yet ionises the air ferociously; one punches through millimetres of aluminium; one sails through centimetres of lead and is barely dented. Put them in a magnetic field and one swings left, one swings right, and one flies dead straight. Rutherford named the first two alpha and beta rays by how far they penetrate; Villard found the third and it was later called gamma. This article is the map of those three radiations — what each one is (a helium nucleus, an electron, a photon), the charge and mass it carries, how deeply it penetrates, how fiercely it ionises, and which way a magnetic field bends it. Underneath all of it sits one deep fact Becquerel's drawer already hinted at: radioactivity comes from the nucleus, is random, and no oven or freezer can speed it up or slow it down.

Key takeaways
  • Radioactivity is a nuclear process: an unstable nucleus spontaneously throws out radiation. It is random (you cannot say which nucleus decays when), and its rate is untouched by temperature, pressure, or chemical state — because nuclear energies are MeV while heat and chemistry act at eV.
  • Three radiations, three identities: an alpha particle is a helium-4 nucleus (2 protons + 2 neutrons, charge +2e); a beta-minus particle is an electron (charge −e); a gamma ray is a high-energy photon (no charge, no rest mass, travels at c).
  • Penetration ranks γ > β > α: alpha is stopped by paper or skin, beta by a few millimetres of aluminium, gamma is only reduced — never fully stopped — by centimetres of lead.
  • Ionising power is the reverse, α > β > γ: roughly 10⁴ : 10² : 1. The ray that stops soonest dumps its energy fastest, so it ionises hardest over its short range.
  • A magnetic field separates them: the heavy positive alpha bends gently one way, the light negative beta bends sharply the opposite way, the neutral gamma is undeflected — the classic experiment that fixed each ray's charge.
  • Key idea: radioactivity is the spontaneous, random emission from an unstable nucleus of one of three radiations — a +2e helium nucleus (α), a −e electron (β), or an uncharged photon (γ) — distinguished at a glance by charge, mass, penetration, and the way a field deflects them.
The core insight

An unstable nucleus spontaneously and randomly emits radiation that comes in three kinds — the alpha particle (a +2e helium-4 nucleus, heavy, intensely ionising, stopped by paper), the beta particle (a −e electron, light, moderately penetrating), and the gamma ray (an uncharged, massless photon, weakly ionising but hugely penetrating) — and a magnetic field bends α and β oppositely while leaving γ straight.

Where this lives today

The three rays Becquerel and Rutherford sorted out are the working tools of a dozen modern fields. In medicine, gamma rays from cobalt-60 and technetium-99m image the body and destroy tumours; beta emitters are used in targeted radiotherapy; and the intensely local energy deposit of alpha particles makes alpha-emitting isotopes precision cancer weapons that spare the tissue a millimetre away. Smoke detectors in most homes contain a tiny americium-241 alpha source whose ionised air a whisper of smoke disrupts. Radiocarbon dating reads the beta activity of carbon-14 to date ancient wood and bone. Industry uses beta and gamma gauges to measure the thickness of paper, foil and plastic on the production line without touching them, and gamma radiography to X-ray welds and castings too thick for ordinary X-rays. Every one of these applications rests on exactly the properties this article compared — that alpha stops in tissue, beta penetrates a controlled few millimetres, and gamma passes through the body — and on the nuclear, temperature-proof constancy of the decay itself. The same penetration ranking dictates radiation shielding on spacecraft, in reactors, and around every hospital gamma source.

The physical picture

Start from what the previous article established: an atom's mass and all its positive charge live in a tiny central nucleus of protons and neutrons, bound by the strong nuclear force. Most nuclei are perfectly stable and sit there forever. But some combinations of protons and neutrons are unstable — the internal bookkeeping of energy and force does not quite balance — and such a nucleus will, sooner or later, rearrange itself into a more stable configuration and shed the excess as radiation. That spontaneous emission is radioactivity, and the rearrangement is a radioactive decay. Becquerel's uranium was doing exactly this in his drawer, and it had been doing it, and will keep doing it, for billions of years regardless of what anyone does to it. The single most important word here is nuclear. Ordinary chemistry — burning, dissolving, bonding — rearranges the outer electrons, and those processes trade energies of a few electronvolts. Radioactive decay reshuffles the nucleus itself, and nuclear energies are measured in millions of electronvolts (MeV), a factor of about a million larger. Heating a sample to red heat, cooling it in liquid nitrogen, crushing it, or locking its atoms into a compound changes the eV-scale electron cloud and leaves the MeV-scale nucleus completely indifferent. This is why the decay rate of a radioactive source is a fixed property of the nucleus, immovable by any everyday means — a fact we will turn into the exponential decay law two articles from now. The second key word is random. Radioactivity is genuinely probabilistic: identical nuclei, prepared the same way, decay at different, unpredictable moments. You cannot point at one uranium nucleus and say when it will go; you can only say what fraction of a large collection will have gone after a given time. The individual event is a roll of the quantum dice; only the statistics are lawful.

Figure
A radioactive source in a lead block sends a beam through a magnetic field pointing into the page — the heavy positive alpha ray bends gently one way, the light negative beta ray bends sharply the other way, and the uncharged gamma ray passes straight through
A magnetic field into the page splits the three radiations ××××× ××××× B into page lead block source γ · neutral · straight α · +2e · heavy · gentle bend β⁻ · −e · light · sharp bend opposite charges bend opposite ways · the neutral ray does not bend

The very first thing early physicists did with Becquerel's radiation was pass it through a magnetic field, and it split into three beams. That single picture — reproduced above — already tells you almost everything: two of the rays are charged (they bend) and of opposite sign (they bend opposite ways), while the third is uncharged (it does not bend). The one that bends only slightly is heavy; the one that bends sharply is light. Reading those clues off, physicists worked out that the three rays are a helium nucleus, an electron, and a photon. The rest of this article is that identification, made quantitative.

What each ray actually is

Three particles, three identities. It is worth stating them plainly before comparing them, because every other property — charge, penetration, deflection — follows from what the thing is.

Alpha (α): a helium-4 nucleus, written 24He^{4}_{2}\text{He} — two protons and two neutrons bound tightly together. Its charge is +2e+2e and its mass is about 4 u4\,u, roughly four times a proton and nearly 7300 times an electron. Because it is a whole, tightly-bound nucleus, an alpha particle is emitted as a single compact projectile: slow (a few per cent of the speed of light), massive, and doubly charged.

Beta-minus (β⁻): an ordinary electron, charge −e-e, mass mem_e — the same electron you meet in circuits and atoms, but created in and flung out of the nucleus at the instant of decay (it was not orbiting there beforehand). Being nearly 7300 times lighter than an alpha, a beta particle of comparable energy travels far faster, up to 99%99\% of the speed of light, and carries far less momentum.

Gamma (γ): a photon — a quantum of electromagnetic radiation, the same kind of thing as light or an X-ray but of much higher energy. It has no charge and no rest mass, always travels at the speed of light c=3.0×108 m s−1c = 3.0\times10^{8}\ \mathrm{m\,s^{-1}}, and carries away energy in the MeV range. A gamma ray is emitted when a nucleus that is left in an excited state after an alpha or beta decay drops to a lower state, exactly as an atom emits a light photon when an electron falls between levels — but at nuclear, million-fold, energies. These three identities immediately fix the charges you will use in every deflection problem:

qα=+2e=+3.2×10−19 C,qβ=−e=−1.6×10−19 C,qγ=0.(1)q_\alpha = +2e = +3.2\times10^{-19}\ \text{C}, \qquad q_\beta = -e = -1.6\times10^{-19}\ \text{C}, \qquad q_\gamma = 0. \qquad (1)

where: e=1.6×10−19 Ce = 1.6\times10^{-19}\ \text{C} is the elementary charge. The physical reading is the whole story of the field experiment in one line: the alpha is doubly positive, the beta is singly negative, and the gamma is neutral. Opposite signs bend opposite ways; zero charge does not bend at all.

Penetration and ionisation — a mirror-image pair

The three rays differ enormously in how far they travel through matter, and — crucially — the ranking of penetration is the exact reverse of the ranking of ionising power. Understanding why they are mirror images is the single most useful idea in this whole comparison. When a charged particle ploughs through matter it loses energy by knocking electrons off atoms — ionising them — and each such collision costs it a little energy. A slow, heavy, doubly-charged alpha interacts violently and constantly: it rips electrons off atoms thousands of times per millimetre, dumps all its energy within a very short distance, and so is stopped almost at once — a sheet of paper, the dead outer layer of your skin, or a few centimetres of air will halt it. But over that short path it creates a dense trail of ionisation, so alpha is by far the most ionising and the least penetrating. A beta particle, light and singly charged, interacts more gently. It ionises perhaps a hundred times less densely than an alpha, so it travels much further before it is spent — up to a few metres of air, and it takes a few millimetres of aluminium to stop it. Moderate ionisation, moderate penetration. A gamma ray carries no charge at all, so it does not steadily ionise as it goes; it interacts only in occasional, abrupt photon events. It therefore ionises very weakly but penetrates enormously — a gamma beam is attenuated by centimetres of lead or metres of concrete but, being absorbed statistically photon-by-photon, is never brought completely to zero, only reduced. Weakest ioniser, deepest penetrator.

ionising power:  α:β:γ ≈ 104:102:1,penetration:  γ>β>α.(2)\text{ionising power:}\ \ \alpha : \beta : \gamma \ \approx\ 10^{4} : 10^{2} : 1, \qquad\qquad \text{penetration:}\ \ \gamma > \beta > \alpha. \qquad (2)

where: the numbers are order-of-magnitude ratios of how many ion pairs each ray makes per unit path. The physical reading: penetration and ionisation are two sides of one coin. A ray that ionises fiercely spends its energy fast and so stops soon; a ray that barely ionises coasts a long way. That is why the danger ranking flips with geometry: outside the body gamma is the hazard (it reaches your organs while alpha is stopped by skin), but if an alpha emitter is inhaled or swallowed, alpha becomes the most dangerous, depositing all its energy in a tiny volume of tissue.

Figure
Three absorbers in a row — a sheet of paper stops the alpha ray, a few millimetres of aluminium stops the beta ray, and a thick slab of lead only reduces the gamma ray which passes partly through
Penetration — paper stops α, aluminium stops β, lead only cuts γ source α β γ paper few mm Al cm of Pb reduced, not stopped penetration γ > β > α · ionising power α > β > γ (the reverse)

Separating the rays in a magnetic field

The experiment that unmasked the three rays was to fire the beam across a magnetic field and watch it fan out. A magnetic field exerts a force on a moving charge — and only on a moving charge — of magnitude F=qvBF = qvB when the velocity is perpendicular to the field, directed sideways (by the right-hand or Fleming rule) so that it always pushes the particle in a circle. Setting that magnetic force equal to the centripetal force mv2/rmv^2/r needed to hold the particle on a circle of radius rr gives the master relation of the whole experiment. Since gamma has q=0q = 0, it feels no force and goes straight; the two charged rays curve, and because their charges have opposite sign they curve to opposite sides.

qvB=mv2r⟹r=mvqB=pqB.(3)qvB = \frac{mv^2}{r} \quad\Longrightarrow\quad r = \frac{mv}{qB} = \frac{p}{qB}. \qquad (3)

where: qq is the particle's charge magnitude, vv its speed, mm its mass, BB the field strength, p=mvp = mv its momentum, and rr the radius of the circular arc it follows. The physical reading: the radius measures momentum per unit charge. A big, heavy, fast particle (large pp) curves in a big lazy arc; a light particle of the same energy has much less momentum and curls up tightly. This is precisely why the heavy alpha bends only gently while the light beta bends sharply — and, with the sign of qq, why they bend to opposite sides.

Derivation AWhy a magnetic field bends α and β oppositely and leaves γ straight

The goal is to show, from the single fact that a magnetic field pushes a moving charge sideways with force F=qvBF = qvB, both the direction each of the three rays curves and the radius of the arc it follows, and to compute a concrete alpha-particle radius for a realistic energy and field using nothing beyond algebra and a square root. The strategy is to balance the magnetic force against the centripetal requirement to get the radius formula, read the direction off the sign of the charge, and then plug in numbers for a 5 MeV alpha in a half-tesla field.

Step 1. The magnetic force on a charge qq moving at speed vv perpendicular to a field BB has magnitude F=qvBF = qvB and points perpendicular to the velocity. A force that is always perpendicular to the motion does no work and changes only the direction of vv, not its size — it bends the path into a circle. For that circle of radius rr the required centripetal force is mv2/rmv^2/r, so qvB=mv2/rqvB = mv^2/r, which rearranges to r=mv/(qB)r = mv/(qB): equation (3).

Step 2. Direction. For the gamma ray q=0q = 0, so F=0F = 0 and it travels in a perfectly straight line — undeflected. For the alpha (q=+2eq = +2e) and the beta (q=−eq = -e) the forces point in opposite directions because the charges have opposite sign, so the two rays swing to opposite sides of the gamma's straight track. This opposite deflection is the signature that alpha and beta carry opposite charge, and it is exactly what the fan-out picture at the top of the article shows.

Step 3. Now a number. Take a typical alpha of kinetic energy KE=5 MeVKE = 5\ \text{MeV} in a field B=0.5 TB = 0.5\ \text{T}. First convert the energy: KE=5×1.602×10−13 J=8.01×10−13 JKE = 5\times1.602\times10^{-13}\ \text{J} = 8.01\times10^{-13}\ \text{J} (using 1 MeV=1.602×10−13 J1\ \text{MeV} = 1.602\times10^{-13}\ \text{J}). The alpha's mass is mα≈4 u=4×1.66×10−27=6.64×10−27 kgm_\alpha \approx 4\,u = 4\times1.66\times10^{-27} = 6.64\times10^{-27}\ \text{kg}.

Step 4. Since 5 MeV5\ \text{MeV} is small compared with the alpha's rest energy (about 3700 MeV3700\ \text{MeV}), the motion is non-relativistic and KE=12mv2KE = \tfrac12 m v^2, so v=2 KE/m=2×8.01×10−13/6.64×10−27=1.55×107 m s−1v = \sqrt{2\,KE/m} = \sqrt{2\times8.01\times10^{-13}/6.64\times10^{-27}} = 1.55\times10^{7}\ \mathrm{m\,s^{-1}} — about 5%5\% of the speed of light, confirming the non-relativistic step. The charge magnitude is q=2e=3.2×10−19 Cq = 2e = 3.2\times10^{-19}\ \text{C}, so

r=mvqB=(6.64×10−27)(1.55×107)(3.2×10−19)(0.5)=0.64 m.r = \frac{mv}{qB} = \frac{(6.64\times10^{-27})(1.55\times10^{7})}{(3.2\times10^{-19})(0.5)} = 0.64\ \text{m}.

Step 5. Contrast with the beta. A beta of comparable energy has the same charge magnitude to within a factor of two but a mass nearly 73007300 times smaller, hence a far smaller momentum p=mvp = mv, hence — by r=p/(qB)r = p/(qB) — a much smaller radius: it curls up tightly where the alpha sweeps a gentle arc, and to the opposite side. (Real MeV betas move at nearly cc and need relativistic momentum, but the conclusion — small radius, opposite side — stands.) The gamma, feeling no force, rules the straight line down the middle. Verified: rα=mv/(qB)=0.64 mr_\alpha = mv/(qB) = 0.64\ \text{m} for a 5 MeV alpha in 0.5 T, with vα=1.55×107 m s−1≈0.05cv_\alpha = 1.55\times10^{7}\ \mathrm{m\,s^{-1}} \approx 0.05c and qα=3.2×10−19 Cq_\alpha = 3.2\times10^{-19}\ \text{C}; opposite deflection for β follows from the opposite sign of qq — recomputed in verify_hs2-radioactivity-alpha-beta-gamma.py.

Limiting cases

caseresultmeaning
gamma in a magnetic fieldno deflection, straight lineq=0q = 0 so F=qvB=0F = qvB = 0 — the neutral ray is unmoved
very strong field BBradius r=mv/(qB)r = mv/(qB) shrinksmore field, tighter curve for the charged rays; γ still straight
alpha vs beta, same energyrα≫rβr_\alpha \gg r_\beta, opposite sidesthe heavy α has far more momentum, so a much gentler arc, opposite sign to β
absorber = a sheet of paperα stopped, β and γ passranks the rays by penetration in one move
absorber = few mm aluminiumα and β stopped, γ passesthe standard way to tell a β source from a γ source
sample heated, cooled, or bondeddecay rate unchangedthe emission is nuclear (MeV); temperature and chemistry act at eV

Worked examples

Board level — identify the three rays (CBSE and ICSE pattern)

A radioactive source is placed behind a slit so it emits a narrow beam. Three separate tests are run. (a) A sheet of paper placed in the beam removes one component entirely. (b) After the paper, a 4 mm aluminium plate removes a second component. (c) What remains passes through and is only cut down by a thick lead block. When a magnetic field is switched on, one component bends up, one bends down, one does not bend. Name each of the three rays and give its charge.

Step 1. The component stopped by mere paper is the least penetrating — the alpha ray, a helium nucleus of charge +2e+2e. Alphas are halted by paper or the dead layer of skin.

Step 2. The component that survives paper but is stopped by a few millimetres of aluminium is the beta ray, an electron of charge −e-e. This aluminium test is the standard way to separate a beta emitter from a gamma emitter.

Step 3. The component that passes even the aluminium and is only reduced — never fully stopped — by centimetres of lead is the gamma ray, an uncharged photon.

Step 4. In the magnetic field the two charged rays bend to opposite sides because their charges have opposite sign; the alpha (heavy, +2e+2e) bends only gently, the beta (light, −e-e) bends sharply the other way, and the uncharged gamma is undeflected, going straight. So the ray that does not bend is confirmed as gamma. Answer: α (+2e, stopped by paper), β (−e, stopped by aluminium), γ (0, only reduced by lead).

Competitive level — radius of an alpha's path in a magnetic field (JEE and NEET pattern)

A 5 MeV alpha particle enters a uniform magnetic field of 0.5 T at right angles to the field. Take the alpha's mass as 4 u = 6.64×10⁻²⁷ kg and its charge as +2e = 3.2×10⁻¹⁹ C. Find (a) its speed, and (b) the radius of its circular path. (c) State, without a full calculation, how a beta particle of the same energy would differ.

Step 1. Convert the energy: KE=5 MeV=5×1.602×10−13=8.01×10−13 JKE = 5\ \text{MeV} = 5\times1.602\times10^{-13} = 8.01\times10^{-13}\ \text{J}.

Step 2. The alpha's rest energy is about 3700 MeV3700\ \text{MeV}, hugely more than 5 MeV5\ \text{MeV}, so it is non-relativistic and KE=12mv2KE = \tfrac12 m v^2. Solve for the speed: v=2 KE/m=2×8.01×10−13/6.64×10−27=1.55×107 m s−1v = \sqrt{2\,KE/m} = \sqrt{2\times8.01\times10^{-13}/6.64\times10^{-27}} = \boxed{1.55\times10^{7}\ \mathrm{m\,s^{-1}}}, about 5%5\% of cc — comfortably non-relativistic, as assumed.

Step 3. Apply r=mv/(qB)r = mv/(qB): r=(6.64×10−27)(1.55×107)/[(3.2×10−19)(0.5)]=0.64 mr = (6.64\times10^{-27})(1.55\times10^{7}) / \left[(3.2\times10^{-19})(0.5)\right] = \boxed{0.64\ \text{m}}.

Step 4. A beta of the same 5 MeV has almost the same charge magnitude (within a factor of two) but a mass nearly 73007300 times smaller, so far less momentum p=mvp = mv; by r=p/(qB)r = p/(qB) its radius is much smaller, and its negative charge curves it to the opposite side. So on the same photograph the alpha traces a broad gentle arc and the beta a tight opposite curl — the fingerprint that told the first experimenters they were seeing two different, oppositely-charged particles. Timing note: about 90 seconds. The one gate is remembering r=mv/(qB)r = mv/(qB) and that vv comes from 12mv2=KE\tfrac12 mv^2 = KE — do the energy conversion first, then the square root, then one division. Do not reach for a relativistic formula on the alpha: a quick "5 MeV≪5\ \text{MeV} \ll rest energy" check licenses the clean non-relativistic route and saves you minutes. The part-(c) comparison needs no arithmetic at all — it is worth full marks for the two words "smaller, opposite".

Exam traps

Penetration ranked backwards. The order is γ>β>α\gamma > \beta > \alpha for penetration and the reverse, α>β>γ\alpha > \beta > \gamma, for ionising power. Writing "alpha penetrates most because it is most energetic" is the classic slip — alpha is stopped by paper. Anchor it: paper stops α, a few mm of aluminium stops β, centimetres of lead only reduce γ. Tested on CBSE, ICSE, IGCSE, AP-2 and A-Level every year.

Saying gamma is "never stopped, so infinitely penetrating" or "completely blocked by lead". Neither. A gamma beam is attenuated exponentially — each thickness of lead cuts it by the same factor, so it is steadily reduced but, mathematically, never brought exactly to zero. Lead does not "stop" gamma; it thins it. (The exponential form is the decay-law article's job.)

The beta electron "was orbiting in the nucleus". No — the emitted electron is created at the moment of decay when a neutron turns into a proton; it was not sitting inside the nucleus beforehand. Do not describe beta decay as the nucleus "losing one of its orbital electrons".

Getting the deflection directions wrong, or bending the gamma. Alpha (+2e+2e) and beta (−e-e) bend to opposite sides; gamma (q=0q=0) does not bend at all. A diagram that curves the gamma, or bends α and β the same way, throws away easy marks. And the alpha bends less than the beta despite its larger charge, because it is so much heavier (bigger momentum, bigger radius).

Claiming temperature, pressure or chemistry changes the decay rate. They do not — radioactivity is nuclear (MeV) and untouched by eV-scale conditions. "Heating the sample speeds up decay" is always wrong.

Board scope. The qualitative comparison here — the three rays, their charges, penetration, and magnetic deflection — is on every board including IGCSE 0625, which carries this half of nuclear physics. The quantitative pieces (the MeV-to-joule conversion, r=mv/(qB)r = mv/(qB) radius calculations, and the exponential attenuation of gamma) are for CBSE, ICSE (ISC), JEE Main and Advanced, NEET, AP-2, IB HL and A-Level 9702 — IGCSE and IB SL keep the description but not the algebra.

Origins · 1 minHenri Becquerel and how this was discovered
HB
Henri Becquerel
1852–1908 · Paris

Antoine Henri Becquerel was a French physicist, the third generation of a Paris dynasty of physicists, whose 1896 discovery opened the entire field of nuclear physics. Investigating whether the phosphorescence of uranium salts could produce the newly-found X-rays, he found instead that uranium fogged a wrapped photographic plate in total darkness, needing no external light — a penetrating radiation the element emitted spontaneously and endlessly. He showed the effect depended only on the presence of uranium, not on its chemical form, temperature or illumination, pinning it to the atom itself. Marie Curie, who took Becquerel's uranium rays as her doctoral subject, and her husband Pierre took up the phenomenon, named it radioactivity, and isolated far stronger new sources. Becquerel shared the 1903 Nobel Prize in Physics with the Curies; the SI unit of radioactivity, the becquerel (one decay per second), carries his name.

History
1896
— Henri Becquerel finds that uranium salts fog a wrapped photographic plate in the dark, discovering spontaneous radioactivity.
1898
— Marie and Pierre Curie isolate polonium and radium and Marie Curie coins the word "radioactivity".
1899
— Ernest Rutherford distinguishes two components by their penetration and names them alpha and beta rays.
1900
— Paul Villard identifies a third, far more penetrating and uncharged ray, later named the gamma ray.
1903
— Rutherford shows the alpha ray is deflected by strong magnetic and electric fields and is positively charged.
1909
— Rutherford and Thomas Royds collect the gas from an alpha source and see helium's spectrum, proving the alpha particle is a helium nucleus.

Going further

Texts. NCERT Physics Class 12, Chapter 13 ("Nuclei"), the radioactivity sections · H. C. Verma, Concepts of Physics Vol. 2, "The Nucleus" · Halliday, Resnick and Walker, "Nuclear Physics" · Krane, Introductory Nuclear Physics, for the historical route and the deflection experiments.

Provenance. Standard nuclear constants (e=1.6×10−19 Ce = 1.6\times10^{-19}\ \text{C}, u=1.66×10−27 kgu = 1.66\times10^{-27}\ \text{kg}, me=9.11×10−31 kgm_e = 9.11\times10^{-31}\ \text{kg}, c=3.0×108 m s−1c = 3.0\times10^{8}\ \mathrm{m\,s^{-1}}, 1 MeV=1.602×10−13 J1\ \text{MeV} = 1.602\times10^{-13}\ \text{J}). Recompute: qα=+2e=3.2×10−19 Cq_\alpha = +2e = 3.2\times10^{-19}\ \text{C}, qβ=−e=−1.6×10−19 Cq_\beta = -e = -1.6\times10^{-19}\ \text{C}, qγ=0q_\gamma = 0; alpha mass 4 u=6.64×10−27 kg4\,u = 6.64\times10^{-27}\ \text{kg}, mass ratio α/β≈7300\alpha/\beta \approx 7300; ionising ratio α:β:γ≈104:102:1\alpha:\beta:\gamma \approx 10^{4}:10^{2}:1; 5 MeV =8.01×10−13 J= 8.01\times10^{-13}\ \text{J}, vα=2KE/m=1.55×107 m s−1≈0.05cv_\alpha = \sqrt{2KE/m} = 1.55\times10^{7}\ \mathrm{m\,s^{-1}} \approx 0.05c, rα=mv/(qB)=0.64 mr_\alpha = mv/(qB) = 0.64\ \text{m} at B=0.5 TB = 0.5\ \text{T}; equal-momentum radius ratio rα/rβ=qβ/qα=1/2r_\alpha/r_\beta = q_\beta/q_\alpha = 1/2 — all recomputed in verify_hs2-radioactivity-alpha-beta-gamma.py.

Prerequisites. Inside the Nucleus: Protons, Neutrons & Isotopes — what the nucleus is made of and why some combinations are unstable. Leads to. Alpha Decay & the Q-Value, which takes the alpha ray apart in energy detail (the Q-value, why a whole helium nucleus, and Gamow tunnelling by name); and, further on, Beta Decay & the Neutrino, Gamma Decay & Nuclear Energy Levels, and The Radioactive Decay Law, which turns the "random, nuclear" nature established here into the exponential N=N0e−λtN = N_0 e^{-\lambda t}. For enrichment, the university seam on particle-decay kinematics (go-deeper only, never an exam dependency here).

Why is radioactivity not affected by temperature, pressure, or chemical reactions?

Because it happens in the nucleus, not in the electron cloud. Heating, cooling, squeezing, and chemical bonding all act on the outer electrons, and the energies involved are a few electronvolts. A radioactive decay reshuffles protons and neutrons in the nucleus, where the energies are millions of electronvolts — about a million times larger. On that scale the eV-sized nudges of everyday physics and chemistry are utterly negligible, like trying to change the orbit of a planet by blowing on it. This is why the decay rate of a given isotope is a fixed constant of nature, the same in a flame or in liquid nitrogen, in the pure metal or locked in a compound — a constancy we will build the exponential decay law on.

If a beta particle is just an electron, where was it hiding inside the nucleus?

It was not hiding anywhere — it is created at the instant of decay. The nucleus contains protons and neutrons, not electrons. In beta-minus decay a neutron transforms into a proton, and the process manufactures a brand-new electron (plus an antineutrino) which is immediately ejected. So the emitted electron did not pre-exist inside the nucleus and is certainly not one of the atom's orbiting electrons. This is exactly parallel to a photon being created when an atom de-excites: the photon was not stored in the atom beforehand. The detailed mechanism — why a neutron turns into a proton and what the antineutrino is for — is the subject of the beta-decay article.

Which type of radiation is the most dangerous?

It depends entirely on whether the source is outside or inside your body, which is why the question has no single answer. Outside the body, alpha is nearly harmless — the dead outer layer of your skin stops it — while gamma is the real hazard because it penetrates to your internal organs. But if an alpha emitter is inhaled or swallowed, alpha becomes the most dangerous of the three, because it dumps all its energy, ionising ferociously, into a tiny volume of living tissue with no dead skin to shield it. Beta sits in between in both cases. So "most dangerous" is a two-part answer: gamma outside, alpha inside.

Why does an alpha particle bend less than a beta particle in a magnetic field, even though it has more charge?

Because the radius of the curve is set by momentum divided by charge, r=mv/(qB)r = mv/(qB), and the alpha's mass wins overwhelmingly. An alpha is nearly 7300 times heavier than a beta. Even though its charge is twice as large (which alone would tighten its curve), its momentum mvmv is so much greater that the net radius is far bigger — a gentle sweep rather than a tight curl. Charge decides the direction of the bend (opposite signs, opposite sides); mass and speed, through the momentum, decide how sharply it bends. The heavy alpha therefore traces a broad arc and the light beta a tight one, to opposite sides of the undeflected gamma.

Can gamma rays ever be completely stopped by shielding?

Not completely, only reduced. Unlike alpha and beta, which have a definite finite range and are truly stopped, gamma rays are attenuated exponentially: each equal thickness of lead cuts the beam by the same fraction (a "half-value layer" halves it), so ten such layers reduce it by a factor of about a thousand, but never mathematically to zero. In practice you add enough lead or concrete to bring the intensity below a safe level, not to eliminate it. This is why shielding a gamma source is always quoted as a thickness that reduces the dose by some factor, never as a thickness that "blocks" it — a distinction examiners like to test, and the reason the exponential law matters so much for radiation safety.

Is a gamma ray the same thing as an X-ray?

They are the same kind of thing — high-energy photons of electromagnetic radiation — and their energy ranges overlap, so the only rigorous distinction is where they come from, not how energetic they are. A gamma ray is emitted by a nucleus dropping from an excited state to a lower one; an X-ray is emitted by electrons (either braking in a target or falling between inner atomic levels). Historically gammas were the more energetic, but the categories are defined by origin. For this article the key point is that a gamma is a photon: no charge, no rest mass, travelling at the speed of light, and therefore undeflected by fields and only weakly ionising.

Why is an alpha particle emitted as a whole helium nucleus rather than as separate protons and neutrons?

Because the helium-4 nucleus is exceptionally tightly bound — two protons and two neutrons lock together into an unusually stable little package with a large binding energy per nucleon. Ejecting that ready-made, tightly-bound unit releases energy, whereas prying out separate protons would cost energy the nucleus does not have to spare. Nature takes the energetically favourable route, and for many heavy nuclei that route is to spit out a whole alpha rather than individual nucleons. The energy bookkeeping of exactly why an alpha, and the tunnelling mechanism that lets it escape, are the subject of the alpha-decay article that follows this one.

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