المرجع الالكتروني للمعلوماتية
المرجع الألكتروني للمعلوماتية

علم الفيزياء
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الفيزياء الكلاسيكية
الفيزياء الحديثة
الفيزياء والعلوم الأخرى
مواضيع عامة في الفيزياء

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The mean free path  
  
684   01:32 صباحاً   التاريخ: 2024-06-05
المؤلف : Richard Feynman, Robert Leighton and Matthew Sands
الكتاب أو المصدر : The Feynman Lectures on Physics
الجزء والصفحة : Volume I, Chapter 43
القسم : علم الفيزياء / الفيزياء الحديثة / الفيزياء الجزيئية /


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Another way of describing the molecular collisions is to talk not about the time between collisions, but about how far the particle moves between collisions. If we say that the average time between collisions is τ, and that the molecules have a mean velocity v, we can expect that the average distance between collisions, which we shall call l, is just the product of τ and v. This distance between collisions is usually called the mean free path:

Mean free path l=τv.                                        (43.9)

In this chapter we shall be a little careless about what kind of average we mean in any particular case. The various possible averages—the mean, the root-mean-square, etc.—are all nearly equal and differ by factors which are near to one. Since a detailed analysis is required to obtain the correct numerical factors anyway, we need not worry about which average is required at any particular point. We may also warn the reader that the algebraic symbols we are using for some of the physical quantities (e.g., l for the mean free path) do not follow a generally accepted convention, mainly because there is no general agreement.

Just as the chance that a molecule will have a collision in a short time dt is equal to dt/τ, the chance that it will have a collision in going a distance dx is dx/l. Following the same line of argument used above, the reader can show that the probability that a molecule will go at least the distance x before having its next collision is e−x/l.

The average distance a molecule goes before colliding with another molecule—the mean free path l—will depend on how many molecules there are around and on the “size” of the molecules, i.e., how big a target they represent. The effective “size” of a target in a collision we usually describe by a “collision cross section,” the same idea that is used in nuclear physics, or in light-scattering problems.

Fig. 43–1. Collision cross section.

 

Consider a moving particle which travels a distance dx through a gas which has n0 scatterers (molecules) per unit volume (Fig. 43–1). If we look at each unit of area perpendicular to the direction of motion of our selected particle, we will find there n0dx molecules. If each one presents an effective collision area or, as it is usually called, “collision cross section,” σc, then the total area covered by the scatterers is σcn0dx.

By “collision cross section” we mean the area within which the center of our particle must be located if it is to collide with a particular molecule. If molecules were little spheres (a classical picture) we would expect that σc=π(r1+r2)2, where r1 and r2 are the radii of the two colliding objects. The chance that our particle will have a collision is the ratio of the area covered by scattering molecules to the total area, which we have taken to be one. So the probability of a collision in going a distance dx is just σcn0dx:

Chance of a collision in dx = σcn0dx.                                  (43.10)

We have seen above that the chance of a collision in dx can also be written in terms of the mean free path l as dx/l. Comparing this with (43.10), we can relate the mean free path to the collision cross section:

This formula can be thought of as saying that there should be one collision, on the average, when the particle goes through a distance l in which the scattering molecules could just cover the total area. In a cylindrical volume of length l and a base of unit area, there are n0l scatterers; if each one has an area σc the total area covered is n0c, which is just one unit of area. The whole area is not covered, of course, because some molecules are partly hidden behind others. That is why some molecules go farther than l before having a collision. It is only on the average that the molecules have a collision by the time they go the distance l. From measurements of the mean free path l we can determine the scattering cross section σc, and compare the result with calculations based on a detailed theory of atomic structure. But that is a different subject! So we return to the problem of nonequilibrium states.




هو مجموعة نظريات فيزيائية ظهرت في القرن العشرين، الهدف منها تفسير عدة ظواهر تختص بالجسيمات والذرة ، وقد قامت هذه النظريات بدمج الخاصية الموجية بالخاصية الجسيمية، مكونة ما يعرف بازدواجية الموجة والجسيم. ونظرا لأهميّة الكم في بناء ميكانيكا الكم ، يعود سبب تسميتها ، وهو ما يعرف بأنه مصطلح فيزيائي ، استخدم لوصف الكمية الأصغر من الطاقة التي يمكن أن يتم تبادلها فيما بين الجسيمات.



جاءت تسمية كلمة ليزر LASER من الأحرف الأولى لفكرة عمل الليزر والمتمثلة في الجملة التالية: Light Amplification by Stimulated Emission of Radiation وتعني تضخيم الضوء Light Amplification بواسطة الانبعاث المحفز Stimulated Emission للإشعاع الكهرومغناطيسي.Radiation وقد تنبأ بوجود الليزر العالم البرت انشتاين في 1917 حيث وضع الأساس النظري لعملية الانبعاث المحفز .stimulated emission



الفيزياء النووية هي أحد أقسام علم الفيزياء الذي يهتم بدراسة نواة الذرة التي تحوي البروتونات والنيوترونات والترابط فيما بينهما, بالإضافة إلى تفسير وتصنيف خصائص النواة.يظن الكثير أن الفيزياء النووية ظهرت مع بداية الفيزياء الحديثة ولكن في الحقيقة أنها ظهرت منذ اكتشاف الذرة و لكنها بدأت تتضح أكثر مع بداية ظهور عصر الفيزياء الحديثة. أصبحت الفيزياء النووية في هذه الأيام ضرورة من ضروريات العالم المتطور.