1. 10. 7. 20031 I-4 Simple Electrostatic Fields

2. 10. 7. 20032 Main Topics Relation of the Potential and Intensity The Gradient Electric Field Lines and Equipotential Surfaces. Motion of Charged Particles in Electrostatic Fields.

3. 10. 7. 20033 A Spherically Symmetric Field I A spherically symmetric field e.g. a field of a point charge is another important field where the relation between  and E can easily be calculated. Let’s have a single point charge Q in the origin. We already know that the field lines are radial and have a spherical symmetry:

4. 10. 7. 20034 A Spherically Symmetric Field II The magnitude of E depends only on r Let’s move a “test” charge q equal to unity from some point A to another point B. We study directly the potential! Its change actually depends only on changes of the radius. This is because during the shifts at a constant radius work is not done.radius

5. 10. 7. 20035 A Spherically Symmetric Field III The conclusion: potential  of a spherically symmetric field depends only on r and it decreases as 1/r If we move a non-unity charge q we have again to deal with its potential energy

6. 10. 7. 20036 The General Formula of The general formula is very simple Gradient of a scalar function in some point is a vector : Gradient It points to the direction of the fastest growth of the function f. Its magnitude is equal to the change of the function f, if we move a unit length into this particular direction.

7. 10. 7. 20037 in Uniform Fields In a uniform field the potential can change only in the direction along the field lines. If we identify this direction with the x-axis of our coordinate system the general formula simplifies to:

8. 10. 7. 20038 in Centrosymmetric Fields When the field has a spherical symmetry the general formulas simplify to: and This can for instance be used to illustrate the general shape of potential energy and its impact to forces between particles in matter.

9. 10. 7. 20039 The Equipotential Surfaces Equipotential surfaces are surfaces on which the potential is constant. If a charged particle moves on a equipotential surface the work done by the field as well as by the external agent is zero. This is possible only in the direction perpendicular to the field lines.

10. 10. 7. 200310 Equipotentials and the Field Lines We can visualize every electric field by a set of equipotential surfaces and field lines. In uniform fields equipotentials are planes perpendicular to the field lines. In spherically symmetric fields equipotentials are spherical surfaces centered on the center of symmetry. Real and imaginary parts of an ordinary complex function has the same relations.

11. 10. 7. 200311 Motion of Charged Particles in Electrostatic Fields I Free charged particles tend to move along the field lines in the direction in which their potential energy decreases. From the second Newton’s law: In non-relativistic case:

12. 10. 7. 200312 Motion of Charged Particles in Electrostatic Fields II The ratio q/m, called the specific charge is an important property of a particle. 1. electron, positron |q/m| = 1.76 10 11 C/kg 2. proton, antiproton |q/m| = 9.58 10 7 C/kg (1836 x) 3.  -particle (He core) |q/m| = 4.79 10 7 C/kg (2 x) 4. other ions … Accelerations of elementary particles can be enormous! enormous

13. 10. 7. 200313 Motion of Charged Particles in Electrostatic Fields III Either the force or the energetic approach is employed. Usually, the energetic approach is more convenient. It uses the law of conservation of energy and takes the advantage of the existence of the potential energy.

14. 10. 7. 200314 Motion IV – Energetic Approach If in the electrostatic field a free charged particle is at a certain time in a point A and after some time we find it in a point B and work has not been done on it by an external agent, then the total energy in both points must be the same, regardless of the time, path and complexity of the field : E KA + U A = E KB + U B

15. 10. 7. 200315 Motion V – Energetic Approach We can also say that changes in potential energy must be compensated by changes in kinetic energy and vice versa : In high energy physics 1eV is used as a unit of energy 1eV = 1.6 10 -19 J.

16. 10. 7. 200316 Motion of Charged Particles in Electrostatic Fields II It is simple to calculate the gain in kinetic energy of accelerated particles from : When accelerating electrons by few tens of volts we can neglect the original speed.few tens But relativistic speeds can be reached at easily reached voltages!relativistic

17. 10. 7. 200317 Homework The homework from yesterday is due Monday!

18. 10. 7. 200318 Things to read This lecture covers : Chapter 21-10, 23-5, 23-8 Advance reading : The rest of chapters 21, 22, 23

19. Potential of the Spherically Symmetric Field A->B We just substitute for E(r) and integrate: We see that  decreases with 1/r ! ^

20. The Gradient I It is a vector constructed from differentials of the function f into the directions of each coordinate axis. It is used to estimate change of the function f if we make an elementary shift.

21. The Gradient II The change is the last term. It is a dot product. It is the biggest if the elementary shift is parallel to the grad. In other words the grad has the direction of the biggest change of the function f ! ^

22. The Acceleration of an e and p I What is the acceleration of an electron and a proton in the electric field E = 2 10 4 V/m ? a e = E q/m = 2 10 4 1.76 10 11 = 3.5 10 15 ms -2 a p = 2 10 4 9.58 10 7 = 1.92 10 12 ms -2 [J/Cm C/kg = N/kg = m/s 2 ] ^

23. The Acceleration of an Electron II What would be the speed of an electron, if accelerated from zero speed by a voltage (potential difference) of 200 V? Thermal motion speed ~ 10 3 m/s can be neglected even in the case of protons (v p = 1.97 10 5 m/s)! ^

24. Relativistic Effects When Accelerating an Electron Relativistic effects start to be important when the speed reaches about 10% of the speed of light ~ c/10 = 3 10 7 ms -1. What is the accelerating voltage to reach this speed? Conservation of energy: mv 2 /2 = q V V = mv 2 /2e = 9 10 14 /4 10 11 = 2.5 kV ! A proton would need V = 4.7 MV!

25. Relativistic Approach I If we know the speeds will be relativistic we have to use the famous Einstein’s formula: E is the total and E K is the kinetic energy, m is the relativistic and m 0 is the rest mass ^

26. Relativistic Approach II The speed is usually expressed in multiples of the c by means of  = v/c. Since  is very close to 1 a trick has to be done not to overload the calculator. So for  we have : ^

27. Example of Relativistic Approach Electrons in the X-ray ring of the NSLS have kinetic energy E k = 2.8 GeV. What is their speed. What would be their delay in arriving to  -Centauri after light? E 0 = 0.51 MeV for electrons. So  = 5491 and v = 0.999 999 983 c. The delay to make 4 ly is dt = 2.1 s ! Not bad and the particle would find the time even shorter!! ^