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🔒 Start your 14-day free trial to unlock the full solution →Concept understanding — Nuclear Reaction Balancing
Nuclear Reaction Balancing: The Intuition
Think of a nuclear reaction like a game of atomic Lego. You start with a certain set of blocks (the reactants), and after the reaction, you end up with a different set of blocks (the products). The fundamental rule is: you cannot lose or gain any Lego pieces. You can rearrange them, break some apart, or fuse them together, but the total number of each type of piece must stay the same.
In the atomic world, the "pieces" are:
- Protons (positive charge, found in the nucleus)
- Neutrons (neutral charge, also in the nucleus)
- Energy (which can appear or disappear, but that's a separate story)
The nucleus of an atom is made of protons and neutrons. When a nuclear reaction happens, the nuclei change. But the total number of protons and the total number of neutrons must be conserved — they cannot be created or destroyed.
This is different from chemical reactions, where atoms themselves are conserved. In nuclear reactions, atoms can change into different elements, but the nucleons (protons + neutrons) are conserved.
The Precise Statement
A nuclear reaction is balanced when two quantities are equal on both sides of the reaction arrow:
- Mass number (A) — the total number of nucleons (protons + neutrons). This is the superscript number.
- Atomic number (Z) — the total number of protons. This is the subscript number.
For any nuclear reaction:
Reactant1+Reactant2→Product1+Product2+…
The balancing conditions are:
∑Areactants=∑Aproducts
∑Zreactants=∑Zproducts
Nuclear Reaction Balancing Rules
Total mass number (A) on left=Total mass number (A) on right
Total atomic number (Z) on left=Total atomic number (Z) on right
How to Write a Nuclear Equation
Every nuclear particle is written as:
ZAX
Where:
- X = chemical symbol of the element
- A = mass number (top left)
- Z = atomic number (bottom left)
Common particles you'll encounter:
| Particle | Symbol | A | Z |
|---|---|---|---|
| Alpha particle | α or 24He | 4 | 2 |
| Beta particle | β− or −10e | 0 | -1 |
| Gamma ray | γ or 00γ | 0 | 0 |
| Neutron | n or 01n | 1 | 0 |
| Proton | p or 11p | 1 | 1 |
| Positron | β+ or +10e | 0 | +1 |
A common mistake: forgetting that beta particles have Z=−1 (for β−) or Z=+1 (for β+). This is because a neutron turns into a proton (or vice versa), and the beta particle carries away the "missing" charge.
Worked Example
Problem: Balance the following alpha decay reaction:
92238U→90234Th+?
Step 1: Identify what's missing. We have an unknown particle on the right.
Step 2: Balance mass numbers (A).
Left: A=238
Right: A=234+Aunknown
So 238=234+Aunknown⟹Aunknown=4
Step 3: Balance atomic numbers (Z).
Left: Z=92
Right: Z=90+Zunknown …
Why this formula?
Why Nuclear Reaction Balancing Works
Nuclear reaction balancing rests on a single, non-negotiable principle: conservation laws are absolute. In every nuclear reaction — whether natural decay, artificial transmutation, or fission/fusion — two quantities never change:
- Total mass number (A) — the sum of protons + neutrons
- Total atomic number (Z) — the sum of protons
These aren't arbitrary rules. They follow from deeper physics: baryon number conservation (protons and neutrons are baryons, and their total count is fixed) and charge conservation (electric charge cannot be created or destroyed). A nuclear reaction is just a rearrangement of nucleons; the number of nucleons stays constant, and the total charge stays constant.
For a reaction Z1A1X+Z2A2Y→Z3A3W+Z4A4Z:
A1+A2=A3+A4
Z1+Z2=Z3+Z4
The Reasoning Behind Each Conservation Law
Mass number conservation (A conserved):
A nucleon (proton or neutron) can change identity — a neutron can beta-decay into a proton, or a proton can capture an electron and become a neutron — but it cannot vanish or appear from nothing. The total count of nucleons before the reaction equals the total count after. This is why, for example, in alpha decay:
92238U→90234Th+24He
The left side has A=238; the right side has 234+4=238. The alpha particle carries away exactly 4 nucleons.
Atomic number conservation (Z conserved):
Charge is strictly conserved. The total positive charge (proton count) before equals the total after. In the same alpha decay, Z goes from 92 to 90+2=92. If charge weren't conserved, atoms would spontaneously change their chemical identity — which never happens in a closed system.
A common mistake is to think mass number conservation means mass is conserved. It does not. Mass-energy is conserved, but the rest mass can change (and usually does, releasing energy). The mass number A is a count of nucleons, not a measure of mass in kilograms.
How to Apply It: A Worked Example
Suppose you see: 92235U+01n→56141Ba+??Kr+301n
You know the total A on the left: 235+1=236.
On the right, you have 141+AKr+3(1)=144+AKr. …
(a) Balancing of nuclear vs. chemical equations
A chemical equation balances atoms — the same number of each element on both sides. A nuclear reaction equation balances nucleons (protons + neutrons) and charge (proton number). It does not balance the number of atoms or molecules; instead, it shows the transformation of one nucleus into another.
In a nuclear equation, the mass number (top) and atomic number (bottom) must each sum to the same total on both sides. This is nucleon and charge conservation, not atom conservation.
(b) How mass converts to energy if nucleons are conserved
Even though the total number of nucleons is conserved, the total mass of the products is slightly less than the total mass of the reactants. This mass difference (Δm) is converted into energy via E=Δmc2. The missing mass appears as kinetic energy of the products or as gamma radiation.
Nucleon count is conserved, but the binding energy per nucleon differs between parent and daughter nuclei, causing a net mass defect that releases energy.
(c) Mass-energy conversion in chemical reactions …
Nuclear reactions balance nucleon number and charge, not chemical species; mass-energy equivalence (E=mc2) accounts for the tiny mass defect that appears as energy, and this same principle applies — though far less noticeably — to chemical reactions as well.
(a) Balancing in nuclear vs. chemical equations
A chemical equation like 2H2+O2→2H2O balances atoms and charge — the same number of each element appears on both sides. The molecules themselves rearrange, but the atoms are conserved.
A nuclear reaction equation, such as
714N+24He→817O+11H
does not balance in the chemical sense — the elements on the left and right are different. Nitrogen and helium become oxygen and hydrogen. What is conserved are two quantities:
- Mass number (nucleon number) — the superscripts: 14+4=17+1
- Atomic number (proton number / charge) — the subscripts: 7+2=8+1
So a nuclear equation is balanced in terms of total nucleons and total charge, not in terms of chemical species. The identity of the nucleus changes, but the building blocks (protons and neutrons) are simply rearranged.
A common mistake is to think that "mass" is conserved in nuclear reactions. The mass number (nucleon count) is conserved, but the actual mass (in kg or u) is not — the mass defect is the source of the released energy.
(b) If nucleons are conserved, where does the energy come from?
If the number of protons and neutrons is the same on both sides, you might wonder: how can mass be converted into energy? The key is that the total mass of the separated nucleons is not the same as the mass of the nucleus they form.
A nucleus is held together by the strong nuclear force. To pull it apart into individual protons and neutrons, you must supply energy — this energy is stored as the binding energy of the nucleus. Conversely, when nucleons fuse, they release that binding energy.
Because of Einstein’s relation E=mc2, this binding energy corresponds to a mass defect:
Δm=Zmp+Nmn−mnucleus
where Δm>0 for a stable nucleus. The mass of the nucleus is less than the sum of the masses of its constituents.
In a nuclear reaction, the total number of nucleons is conserved, but the binding energy per nucleon differs between the reactants and products. If the products have a higher binding energy per nucleon (i.e., they are more tightly bound), the total mass of the products is slightly less than that of the reactants. The missing mass appears as kinetic energy of the products (or as gamma radiation), according to E=Δmc2.
Q=(mass of reactants−mass of products)c2
The Q-value of a nuclear reaction is the energy released (positive for exothermic reactions).
So mass is not "destroyed" — it is converted into energy, and the nucleon count remains unchanged. The mass defect is a measure of the binding energy difference.
(c) Mass-energy interconversion in chemical reactions
It is a widespread misconception that E=mc2 only matters in nuclear physics. In truth, every exothermic chemical reaction also involves a tiny mass decrease.
When hydrogen burns:
2H2+O2→2H2O+energy …
Method: Conservation Laws in Nuclear Reaction Balancing
The method is Conservation of Nucleon Number and Charge. Unlike chemical equations, nuclear reactions are not balanced by conserving atoms or molecules — they are balanced by conserving two fundamental quantities on each side of the arrow.
Steps
- Check conservation of mass number (A) — the total number of nucleons (protons + neutrons) must be the same on both sides.
- Check conservation of atomic number (Z) — the total charge (number of protons) must be the same on both sides.
- Check that the resulting nuclide is physically possible — the product must have a known isotope with the calculated Z and A.
For any nuclear reaction:
∑Areactants=∑Aproducts
∑Zreactants=∑Zproducts
(a) How are nuclear equations "balanced"?
No, nuclear equations are not balanced in the chemical sense. A chemical equation like 2H2+O2→2H2O is balanced by conserving the number of atoms of each element — the same atoms rearrange, nothing changes identity at the nuclear level.
A nuclear equation is balanced by conserving nucleon count and charge. The identities of elements can change completely. For example, in alpha decay:
92238U→90234Th+24He
Left: A = 238, Z = 92. Right: A = 234 + 4 = 238, Z = 90 + 2 = 92. The numbers match, but uranium has become thorium plus helium — atoms are not "preserved" the way they are in chemistry.
In chemical balancing, you conserve atoms. In nuclear balancing, you conserve nucleons and charge — the particles themselves can transform.
(b) If nucleons are conserved, where does the mass-energy conversion come from?
The number of nucleons is conserved, but the total mass of the products is slightly less than the total mass of the reactants. This mass difference (Δm) is converted into energy via E=Δmc2.
Why does mass decrease even though the count of protons and neutrons stays the same? Because the binding energy per nucleon differs between the initial and final nuclei. A nucleus with higher binding energy per nucleon is more tightly bound and has less mass per nucleon. The "missing" mass is the mass equivalent of the binding energy released.
Nucleon count is conserved. Mass is not conserved — the mass defect is converted to kinetic energy of the products (or to gamma radiation).
(c) Mass-energy conversion also occurs in chemical reactions — why the impression is incorrect …
Common Mistakes in Nuclear Reaction Balancing
Mistake 1: Treating nuclear equations like chemical equations
Students often try to balance nuclear reactions by matching the number of atoms of each element on both sides, just as they would for 2H2+O2→2H2O.
Why this fails: In a chemical equation, atoms are conserved — the same elements appear on both sides. In a nuclear reaction, elements can change because the nucleus itself transforms. A uranium nucleus splitting into barium and krypton doesn't have "equal uranium atoms" on both sides.
How to avoid: Instead of looking at elements, look at two numbers only:
- Mass number (A) — the superscript (total protons + neutrons)
- Atomic number (Z) — the subscript (number of protons)
Both A and Z must sum to the same total on left and right. That's the only balancing that matters.
In chemical equations, atoms are conserved. In nuclear equations, nucleons (protons + neutrons) are conserved, and charge (proton number) is conserved. Elements themselves are not conserved.
Mistake 2: Forgetting that mass-energy conversion happens within conserved totals
This connects directly to part (b) of your question. Students see that the total number of protons and neutrons is conserved and then wonder: where does the energy come from?
The confusion: If 92 protons and 143 neutrons go in, and 92 protons and 143 neutrons come out, how can mass have been converted to energy?
The resolution: The count of nucleons is conserved, but the total mass of the nucleus is not equal to the sum of the masses of its individual protons and neutrons. The mass of a nucleus is less than the sum of its parts — that difference is the mass defect, which corresponds to binding energy.
When a nuclear reaction releases energy, the total mass of the products is slightly less than the total mass of the reactants, even though the number of protons and neutrons is identical. That missing mass has become energy via E=mc2.
Conservation of nucleon count does not mean conservation of nucleon mass. The mass of a bound nucleus is less than the sum of the masses of its free nucleons.
Mistake 3: Believing mass-energy conversion is exclusive to nuclear reactions
This addresses part (c). Many students think chemical reactions involve only energy rearrangement, with no mass change at all.
The error: Chemical reactions do involve mass-energy conversion — the effect is just too tiny to measure. When hydrogen burns:
2H2+O2→2H2O
The reaction releases about 286 kJ/mol of energy. Using E=mc2, the corresponding mass change is:
Δm=c2E=(3×108)2286×103≈3.2×10−12 kg per mole
That's roughly one part in 1010 of the total mass — far below the sensitivity of any chemical balance. …
- AP EAPCET 2026Set eng-2026-05-13-FN1 markMCQQ.Binding energy per nucleon of deuteron and Helium nuclei are 1.1 MeV and 7 MeV respectively. If a single Helium nucleus was formed by adding two Deuterons, the energy released is (A) 23.6 MeV (B) 32.4 MeV (C) 28.6 MeV (D) 13.6 MeV
›Reveal solutionSolution
This tests fusion energetics via total binding energy (not BE per nucleon directly). Two deuterons fusing to helium release 23.6 MeV — this is exactly the classic D-D fusion energy release figure.
Concept and Intuition
Binding energy per nucleon measures how tightly bound, on average, each nucleon is. To get the total binding energy of a nucleus you must multiply by the mass number A (the total nucleon count), because binding energy is an extensive (whole-nucleus) quantity while BE/nucleon is an intensive (per-particle) one. When lighter nuclei fuse into a more tightly-bound heavier nucleus, the difference in total binding energy is released as energy (mass converts to energy per E=mc2, already baked into the BE values).
Step-by-Step Solution
- Deuteron (12H) has mass number A=2 and BE/nucleon =1.1 MeV. Total BE of one deuteron =2×1.1=2.2 MeV.
- Two deuterons together carry total BE =2×2.2=4.4 MeV.
- Helium (24He) has mass number A=4 and BE/nucleon =7 MeV. …
- AP EAPCET 2026Set eng-2026-05-15-AN1 markMCQQ.During the decay of an unstable nucleus, if its neutron number and mass number decrease by 5 and 12 respectively, then the particles released in the decay are (A) One alpha particle and six positrons (B) One alpha particle and six electrons (C) Three alpha particles and one positron (D) Three alpha particles and one electron
›Reveal solutionSolution
Matching the mass-number and neutron-number decreases uniquely picks three α particles plus one positron.
Concept and Intuition
An α particle (24He) removes 2 protons and 2 neutrons, so it always changes A by −4, Z by −2, N by −2. A β− (electron) emission converts a neutron to a proton: Z by +1, N by −1, A unchanged. A β+ (positron) emission does the reverse: Z by −1, N by +1, A unchanged. We're told the overall changes are N down by 5 and A down by 12, so ΔZdecrease=ΔA−ΔN=12−5=7.
Step-by-Step Solution
- Only α particles change A, each by −4. To get a total A decrease of 12 we need exactly 3 α particles.
- Three α particles alone give a Z decrease of 6 and an N decrease of 6.
- We still need one more unit of Z-decrease (to reach 7) while N's decrease must come back up from 6 to 5 (i.e., N needs +1 relative to the 3-alpha result).
- A positron emission does exactly that: Z decreases by 1 more (reaching 7 total) and N increases by 1 (bringing the N-decrease from 6 down to 5). …
- AP EAPCET 2025Set ap-2025-05-19-FN1 markMCQQ.The equation for 10Ne23 nucleus which decays by β-emission is (A) 10Ne23β-decay10Ne22+νˉ+e+ (B) 10Ne23β-decay10Ne23+ν+e− (C) 10Ne23β-decay11Na22+e−+νˉ (D) 10Ne23β-decay11Na23+e−+νˉ
›Reveal solutionSolution
This tests the mass/charge bookkeeping of β−-decay. In β−-decay a neutron becomes a proton, so Z increases by 1 while A is unchanged; the correct daughter is 11Na23.
Concept and Intuition
In β− (negatron) decay, one neutron inside the nucleus transforms into a proton, emitting an electron (e−) and an electron-antineutrino (νˉ):
n→p+e−+νˉ
Since a neutron is replaced by a proton, the mass number A stays the same but the atomic number Z increases by 1. The daughter nucleus therefore sits one place to the right in the periodic table.
Step-by-Step Solution
- Parent nucleus: 10Ne23 (Z = 10, A = 23).
- β−-decay converts one neutron to a proton: Z→Z+1=11, A unchanged =23.
- Element with Z = 11 is sodium (Na). So the daughter is 11Na23.
- Conservation of charge and lepton number requires the emitted particles to be e− and νˉ (not a positron, which would occur in β+-decay and would decrease Z).
- Full equation: 10Ne23→11Na23+e−+νˉ.
Common Mistakes …
- AP EAPCET 2025Set eng-2025-05-27-FN1 markMCQQ.If the binding energy per nucleon of deuteron (1H2) is 1.15 MeV and an α-particle has a binding energy of 7.1 MeV per nucleon, then the energy released per nucleon in the given reaction is 1H2+1H2→2He4+Q (A) 23.8 MeV (B) 26.1 MeV (C) 5.95 MeV (D) 28.9 MeV
›Reveal solutionSolution
This tests binding-energy bookkeeping for a fusion reaction; the total Q is 23.8 MeV, which works out to 5.95 MeV per nucleon.
Concept and Intuition
In any nuclear reaction, the energy released equals the increase in total binding energy: reactants with less total binding energy fuse into a product with more total binding energy, and the difference is released as Q. Binding energy per nucleon must first be converted to total binding energy (multiply by mass number) before adding/subtracting, since binding energy is an extensive (additive) quantity, not per-nucleon directly comparable across different nuclei.
Step-by-Step Solution
- Each deuteron 1H2 has mass number 2 and BE/nucleon =1.15MeV, so total BE per deuteron =2×1.15=2.3MeV.
- Two deuterons together: total initial BE =2×2.3=4.6MeV.
- The product 2He4 has mass number 4 and BE/nucleon =7.1MeV, so total BE =4×7.1=28.4MeV. …
- AP EAPCET 2023Set ap-2023-05-22-AN1 markMCQQ.Among the following the possible nuclear reaction is (A) 510B+24He→713N+11H (B) 1124Na+01n→1020Ne+24He (C) 93239Np→94239Pu+e−+υˉ (D) 711N+11H→612C+e−+υˉ
›Reveal solutionSolution
A nuclear reaction is physically possible only if both mass number and atomic number balance on both sides; checking each option, only the Np-239 → Pu-239 beta decay balances.
Concept and Intuition
Every nuclear reaction must independently conserve total mass number A (nucleon count) and total charge/atomic number Z on both sides of the arrow (along with energy/momentum, but those aren't testable from the symbolic equation alone). This is a quick, purely bookkeeping check that instantly rules out fabricated-looking reactions.
Step-by-Step Solution
- Option (A): A: 10+4=14, 13+1=14 — matches. Z: 5+2=7, but 7+1=8 — mismatch. Not possible as written (correct version would emit a neutron, not a proton).
- Option (B): A: 24+1=25 vs 20+4=24 — mismatch. Not possible.
- Option (C): A: 239 vs 239+0+0=239 — matches. Z: 93 vs 94+(−1)+0=93 — matches. This is the well-known genuine β− decay 93239Np→94239Pu+e−+υˉ. …
- AP EAPCET 2023Set eng-2023-05-18-FN1 markMCQQ.A radioactive decay forms an isotope of the original nucleus with the emission of the following particles (A) one α- and four β- particles (B) one α- and one β- particles (C) one α- and two β- particles (D) four α- and one β- particles
›Reveal solutionSolution
Restoring the original atomic number (needed for an isotope) after one α decay requires exactly two β− decays to compensate.
Concept and Intuition
An isotope of the original nucleus has the same atomic number Z (same element) but generally a different mass number A. In radioactive decay: an α particle emission reduces Z by 2 and A by 4; a β− particle emission (electron emission, a neutron converting to a proton) increases Z by 1 while leaving A unchanged.
Step-by-Step Solution
- Let the decay chain involve nα alpha particles and nβ beta particles.
- Net change in atomic number: ΔZ=−2nα+nβ.
- For the final nucleus to be an isotope (same Z, so ΔZ=0, but with A reduced due to the alpha decays, so genuinely a different isotope, not the identical nuclide): nβ=2nα. …
- AP EAPCET 2022Set ap-2022-07-11-AN1 markMCQQ.Consider a radioactive isotope 92U238 decays into 82Pb206 in a series by emission of nα number of alpha particles and nβ number of beta particles. Then the values of nα and nβ? (A) nα=8, nβ=8 (B) nα=6, nβ=6 (C) nα=8, nβ=6 (D) nα=6, nβ=8
›Reveal solutionSolution
This tests radioactive-decay-series bookkeeping: the mass-number drop fixes the alpha count, and the atomic-number drop (after accounting for the alphas) fixes the beta count. Answer: nα=8, nβ=6.
Concept and Intuition
In a decay series, mass number (A) changes only because of α-emission — each α is a 24He nucleus, so it reduces A by 4. β−-emission (an electron ejected when a neutron converts to a proton inside the nucleus) changes Z but leaves A unchanged. So the total mass-number drop alone tells us how many alphas were emitted; once that is known, the atomic-number drop tells us how many betas were needed to make the numbers balance.
Step-by-Step Solution
- Mass-number change: 238−206=32. Since each α reduces A by 4: nα=32/4=8.
- Atomic-number change: 92−82=10 (a net decrease of 10 over the whole series). …
- AP EAPCET 2022Set eng-2022-07-07-FN1 markMCQQ.The correct statement of the following is (A) The Q – value of a nuclear process is the difference between final and initial kinetic energies. (B) The nuclear mass is always higher than the total mass of its constituents (C) Nuclides with same number of neutrons in the nucleus are known as isotopes. (D) In nuclear fusion, a heavy nucleus breaks into two smaller fragments.
›Reveal solutionSolution
This tests precise nuclear-physics vocabulary: Q-value, mass defect, isotopes/isotones, and fission vs fusion. Only the Q-value statement (A) is accurate.
Concept and Intuition
Nuclear reactions release or absorb energy according to the mass difference between reactants and products (Q=Δmc2). Equivalently, since total energy is conserved, this same Q shows up as the difference between the total kinetic energy carried away by the products and the total kinetic energy the reactants had — this equivalence is exactly what statement (A) states. The other statements test whether you can distinguish related-but-different ideas: mass defect (binding energy) vs. constituent mass, isotopes vs. isotones, and fission vs. fusion.
Step-by-Step Solution
- (A) By definition, Q=(KE of products)−(KE of reactants), which equals [∑mreactants−∑mproducts]c2. This is the standard textbook definition — true.
- (B) Because of the mass defect (binding energy), a nucleus's mass is always less than the sum of the masses of its free constituent nucleons, not higher — false.
- (C) Nuclides with the same number of protons (atomic number Z) are isotopes; nuclides with the same number of neutrons are isotones. The statement swaps these — false. …
- AP EAPCET 2021Set ap-2021-09-03-FN1 markMCQQ.The binding energy per nucleon of 3Li7 and 2He4 nuclei are 5.60 MeV and 7.06 MeV, respectively. Then, in the nuclear reaction 3Li7+1H1⟶2He4+2He4+Q, the value of Q, the energy released, is (A) 19.6 MeV (B) −2.4 MeV (C) 8.4 MeV (D) 17.3 MeV
›Reveal solutionSolution
This tests computing the Q-value of a nuclear reaction from binding energies per nucleon, using Q=(total BE of products)−(total BE of reactants). The answer is 17.3 MeV.
Concept and Intuition
In a nuclear reaction, the energy released, Q, equals the increase in total binding energy going from reactants to products — because a more tightly bound (higher total BE) final configuration corresponds to a lower rest-mass total, and that mass difference is released as kinetic energy/radiation by E=mc2. So instead of tracking individual masses, we can directly use Q=∑(BE)products−∑(BE)reactants, taking care to multiply each binding energy per nucleon by the number of nucleons in that nucleus to get the total binding energy.
Step-by-Step Solution
- Reaction: 3Li7+1H1→2He4+2He4+Q.
- Total BE of 3Li7 (7 nucleons, 5.60 MeV/nucleon): 7×5.60=39.2 MeV.
- Total BE of 1H1: a single proton has no binding energy (there's nothing to bind to itself), so BE =0. …
- AP EAPCET 2021Set eng-2021-08-20-AN1 markMCQQ.Which of the following nuclear reactions is possible? (A) 5B10+2He4⟶7N13+1H1 (B) 11Na24+1H1⟶10Ne20+2He4 (C) 93Np239⟶94Pu239+β−+γ− (D) 7N11+1H1⟶6C12+β−+γ−
›Reveal solutionSolution
A real nuclear reaction must conserve both mass number (A) and charge/atomic number (Z) on both sides; only option (C) does.
Concept and Intuition
In any nuclear reaction (or decay), the total mass number A (nucleons) and the total charge Z (protons, counting β− as charge −1 and mass number 0, and γ as carrying neither charge nor mass number) must each be conserved separately. Checking these two simple bookkeeping sums is the fastest way to spot an impossible reaction.
Step-by-Step Solution
- (A) 5B10+2He4→7N13+1H1: mass numbers 10+4=14=13+1 ✓, but charges 5+2=7 on the left vs 7+1=8 on the right ✗ — charge not conserved, impossible as written (the real reaction actually produces a neutron, 7N13+0n1).
- (B) 11Na24+1H1→10Ne20+2He4: charges 11+1=12=10+2 ✓, but mass numbers 24+1=25=20+4=24 ✗ — mass number not conserved, impossible. …
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