Nature of (Strong) Nuclear Force

Nature of (Strong) Nuclear Force

Understanding the Strong Nuclear Force

Overview of Fundamental Forces

  • The strong nuclear force is one of the four fundamental forces in the universe, alongside gravitational, electromagnetic, and weak nuclear forces.
  • It is characterized as the strongest among these forces but operates over extremely short distances (around a few femtometers).

Functionality of the Strong Nuclear Force

  • The strong nuclear force acts between neutrons and protons to create stable nuclear structures and also within individual neutrons and protons.
  • When acting outside a neutron or proton to stabilize nuclei, it is referred to as the residual or mostly nuclear force.

Magnitude and Distance Relationship

  • At a distance of approximately 150 meters, two protons experience a repulsive Coulomb force of about 230 Newtons due to their positive charges. This highlights the significant repulsion at this range.
  • In contrast, at around 1 femtometer, the attractive nuclear force between two protons can reach approximately 25,000 Newtons, indicating its immense strength compared to Coulomb repulsion.

Nature of Strong Nuclear Force with Distance

  • The strong nuclear force decreases exponentially from around 150 meters down to negligible levels beyond 2.5 to 3 femtometers; it becomes attractive at maximum strength near 1 femtometer.
  • Interestingly, below about 0.8 femtometers, this force flips from attractive to repulsive; this prevents neutrons and protons from collapsing into each other under extreme attraction.

Mechanism Behind Strong Nuclear Force

  • Hideki Yukawa proposed that the strong nuclear force results from continuous exchange of particles (pions) between neutrons and protons in his theory established in 1935. This exchange mechanism explains how nucleons interact effectively despite their charge-induced repulsion.

Understanding Nuclear Forces

The Concept of Interaction in Physics

  • When observing two individuals, Harry and John, playing catch, an external observer may deduce that they are connected by an unseen force rather than just seeing them throw a ball back and forth.
  • This analogy is used to explain the attractive force between neutrons and protons within an atomic nucleus, which involves the exchange of particles known as pions.

The Standard Model of Physics

  • Modern physics utilizes the Standard Model to describe forces as results of particle exchanges between different systems, providing a framework for understanding fundamental interactions.

Composition of Neutrons and Protons

  • Neutrons and protons are not elementary particles; they are composed of quarks. A proton consists of two up quarks and one down quark, while a neutron has one up quark and two down quarks.
  • The strong nuclear interaction binds these quarks together through the exchange of gluons, which creates stable structures for both neutrons and protons.

Residual Effects in Nuclear Forces

  • The strong nuclear interaction extends beyond individual neutrons and protons; it influences their collective behavior when they come close together.
  • This leads to what is termed as residual effects—interactions between collections of quarks from different nucleons (neutrons or protons)—resulting in what we recognize as the nuclear force.

Complexity of Nuclear Forces

Playlists: Nuclear Physics
Video description

What is the (Strong) Nuclear Force? The Nuclear force is the force that holds nucleus of an atom together. It can act between both neutrons and protons. It is the strongest among all the fundamental forces in nature. Yet, it only works at extremely short distances. Protons and neutrons are made up of further fundamental particles known as Quarks. The force that exists between such quarks to create stable neutron and proton structures is known as Strong Nuclear Force/Interaction, while the force that exists between such neutrons and protons to create stable nuclear configurations is known as Nuclear force or Residual nuclear force. So how does the nuclear force vary with distance? It is most powerful at distances of around 1 fm. From distances of around 1 - 2.5 fm, it decreases exponentially. For distances greater than 2.5 fm, it is almost negligible. And, finally, for distances less than 0.8 fm, it reverses in sign and suddenly becomes repulsive in nature. This is necessary to avoid collapse of the nuclei. If the nuclear force was not repulsive at extremely short distances, the particles would collapse into themselves. One of the first successful models to explain the mechanism of how such a force works was first given by Hideki Yukawa, in what is now known as the Meson Theory of Nuclear Forces. ▱▱▱▱▱▱▱▱▱▱▱▱▱▱▱▱▱▱▱ Support💖https://www.patreon.com/dibyajyotidas Donate🤝🏻https://paypal.me/FortheLoveofPhysics Telegram - https://t.me/FortheLoveofPhysicsYT ▱▱▱▱▱▱▱▱▱▱▱▱▱▱▱▱▱▱▱ NUCLEAR AND PARTICLE PHYSICS - Series : •••••••••••••••••••••••••••••••••••••••••• 1) What is Nuclear Physics? ► https://youtu.be/6joildn5lqY 2) Nuclear Size / Radius ► https://youtu.be/1keKrGoqUAg 3) Quantization of Angular Momentum ► https://youtu.be/QHYJ4VpqAvs 4) Nuclear Spin and Angular Momentum ► https://youtu.be/LPYPhyioDfs 5) Nuclear Magnetic Moment ► https://youtu.be/3QniicZuVnc 6) Binding Energy of Nucleus & BE Curve ► https://youtu.be/BYRz_9wvJzA 7) Parity of Wave function ► https://youtu.be/BSTRJjElDdI 8) Symmetric & Anti symmetric Wave func ► https://youtu.be/wvnWCY9TKgw 9) Liquid Drop Model of Nucleus ► https://youtu.be/4q1i7yTcQmA 10) Corrections to Liquid Drop Model ► https://youtu.be/GeLC1AUC0W8 11) NZ Graph (& Maximizing BE) ► https://youtu.be/MHYrv_1VJdI 12) Fermi Energy of Nucleus ► https://youtu.be/aUPLjIjgYGk 13) Fermi Gas Model of Nucleus ► https://youtu.be/emSekijh7XI 14) Shell Model of Nucleus ► https://youtu.be/Rd0CJje59bE 15) Nature of (Strong) Nuclear Force) ► https://youtu.be/43AyN24jZw8 16) Alpha, Beta & Gamma Decay ► https://youtu.be/eUEgpcQHzIA 17) Gamow's Theory of Alpha Decay ► https://youtu.be/suj5MTLGAUU 18) Gamow's Theory (DERIVATION) ► https://youtu.be/QwT4tbA8UvI 19) Q Value and KE of Alpha Decay ► https://youtu.be/w0eEGiOYvus 20) Beta Decay & Neutrino Hypothesis ► https://youtu.be/avKic7oiwvA 21) Radioactive Decay Law ► https://youtu.be/fOMvJj39eTU 22) Nuclear Cross Section ► https://youtu.be/R0tdsaFJ4vg 23) Interaction of Nuclear Radiation with Matter ► https://youtu.be/Ara0eTv02No 24) What is Cherenkov Radiaton? ► https://youtu.be/AkR2daFw45U 25) Nuclear Detectors ► https://youtu.be/avvXftiyBEs 26) Geiger Muller Counter ► https://youtu.be/jxY6RC52Cf0 27) Scintillation Detector ► https://youtu.be/rjuFrk0-AOw 28) Semiconductor Detectors ► https://youtu.be/c1boCCYs77Q 29) What are Accelerators? ► https://youtu.be/-KslGjXEtKk 30) Van de Graaff Generator ► https://youtu.be/Q9bijrQfS6E 31) Linear Accelerator ► https://youtu.be/C79838wtRZo 32) Cyclotron ► https://youtu.be/L5zhpLfnqGc 33) Synchrotron ► https://youtu.be/rOXfm6EezeA 34) Betatron ► https://youtu.be/rOXfm6EezeA 35) Fission & Fusion ► https://youtu.be/L7_oi9zChqE 36) Proton-Proton & CNO Cycle ► https://youtu.be/aqnCfDqQlzA 37) Meson Theory of Nuclear Forces ► https://youtu.be/Wvjci2gP7eg ••••••••••••••••••••••••••••••••••••••••••• NUCLEAR PHYSICS - PLAYLIST https://www.youtube.com/playlist?list=PLRN3HroZGu2n_j3Snd_fSYNLvCkao8HIx ••••••••••••••••••••••••••••••••••••••••••• #NuclearPhysics mage Attribution : 1) Nucleus Marekich [CC BY-SA 3.0 (https://creativecommons.org/licenses/by-sa/3.0)], from Wikimedia Commons 2) Quark structure - neutron No machine-readable author provided. Harp assumed (based on copyright claims). [CC BY-SA 2.5 (https://creativecommons.org/licenses/by-sa/2.5)], via Wikimedia Commons 3) Quark structure - proton Jacek rybak [CC BY-SA 4.0 (https://creativecommons.org/licenses/by-sa/4.0)], from Wikimedia Commons 4) Nuclear Force - Graph Bdushaw [CC BY-SA 4.0 (https://creativecommons.org/licenses/by-sa/4.0)], from Wikimedia Commons 5) Strong Nuclear Force - among Quarks Manishearth [CC BY-SA 3.0 (https://creativecommons.org/licenses/by-sa/3.0) or GFDL (http://www.gnu.org/copyleft/fdl.html)], from Wikimedia Commons 6) Residual nuclear interaction Manishearth [CC BY-SA 3.0 (https://creativecommons.org/licenses/by-sa/3.0) or GFDL (http://www.gnu.org/copyleft/fdl.html)], from Wikimedia Commons