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नाभिक का संघटन (Composition of Nucleus)|...

नाभिक का संघटन (Composition of Nucleus)|प्रोटॉन (Proton)|परमाणु द्रव्यमान मात्रक (Atomic Mass Unit)|आइंस्टाइन का द्रव्यमान-ऊर्जा समतुल्यता संबंध (Einstein's mass-energy equivalence relation)|द्रव्यमान क्षति (Mass Defect)|नाभिकीय बंधन ऊर्जा (Nuclear Binding Energy)|प्रति न्यूक्लियॉन बंधन ऊर्जा (Binding Energy per Nucleon)|नाभिकीय बल (Nuclear Forces)|नाभिकीय विखंडन (Nuclear Fission)|नाभिकीय संलयन (Nuclear Fusion)|OMR

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Q-Value in Terms OF Mass||Binding Energy||Kinetic Energy||Binding Energy Per Nucleon and Stability||Nuclear Fusion and Fission||Alpha-decay

Q Value in Terms OF Mass|| Binding Energy||Kinetic Energy|| Binding Energy Per Nucleon and Stability|| Nuclear Fusion and Fission|| Alpha-decay

Nuclear physics:Nucleus||Fission||Fusion||Mass defect||Binding energy||Binding energy per nucleons||Examples

नाभिक-परिचय|नाभिकीय बल|द्रव्यमान क्षति|बंधन ऊर्जा तथा बंधन ऊर्जा प्रति न्यूक्लिऑन|रेडियो सक्रियता|रेडियोएक्टिविटी क्षय का नियम|नाभिकीय विखंडण तथा नाभिकीय संलयन|नाभिकीय रिएक्टर

Atom(परमाणु)|Atomic Mass(परमाणु भार)|Nuclear Force(नाभिकीय बल)|Questions(प्रश्न )|OMR|Summary

The binding energy per nucleon, for nuclei with atomic mass number A gt 100 , decreases with A . The nuclear forces are weak for heavier nuclei.

Assertion: The nuclear energy can be obtained by the nuclear fission of heavier nuclei as well as by fusion of lighter nuclei. Reason: As the mass number increases, the binding energy per nucleon, first increases and then decreases.