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Laser Physics - P. Milonni, J. Eberly (Wiley, 2010)


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- The award of the 1964 Nobel Prize in physics to C.
- The temperature of the sun is about T ¼ 5800K 20(300K).
- The electric field should vanish at both ends of the cavity.
- for the z component of the wave vector.
- In the most favorable situation the lower level (level 1) of the laser transition is empty.
- These factors are reflected in the size of the ampli- fication or gain coefficient a.
- (1.5.1) nor (1.5.2) can be solved independently of the other.
- However, several consequences of the quantum theory are essential.
- In the Coulomb field of the.
- In the Bohr model a state of the electron is characterized by the quantum number n..
- there are n possible values of the orbital angular momentum quantum number.
- The origin of the binding.
- In terms of the reduced mass.
- The ground level of the oscillator corresponds to n ¼ 0.
- in (2.3.11), that is, by the shape of the potential function V(x).
- The vibrational spectra of the two isotopic molecules for the same electronic transition E e ! E e 0.
- This was before the quantum mechanical derivation by Heisenberg (1925) of the formula (2.3.8) for the energy.
- It is found that the rotational energy (2.4.2) of the molecule has the allowed values.
- This is a general feature of the quantum theory of angular momentum.
- Figure 2.10 The first few vibrational energy levels of the CO 2 molecule..
- E g , where hn is the frequency of the radiation).
- Specifically, an electron to the right of the hole indicated in Fig.
- 2.16) as the current of the electrons in the conduction band.
- In particular, the energy of the lowest energy state should be.
- According to these relations, the product N n N p is the same for the two sides of the junction..
- c (x) ¼ u(x)e ikx , (2:A:5a) with k a real number and u(x) now not a constant, but a function with the periodicity of the potential:.
- This is the limit of the potential of Fig.
- Figure 2.33 Plot of the left side of Eq.
- this is implicit in the assumption of the periodicity of the potential.
- The rate of change of the electron energy as a result of this force is.
- Now the force equals the rate of change of the momentum p ¼ h k:.
- The acceleration of the electron is therefore.
- Thus, m arises from the proportionality of the electron acceleration to the external force.
- gives the Balmer series of the hydrogen spectrum.
- In what region of the spectrum are these wavelengths?.
- p , where n is the refractive index of the LED, and estimate this factor for GaAs.
- The binding energy of the ion H 2 þ.
- (a) What is the contribution to the energy from the Coulomb repulsion of the nuclei?.
- (b) What is the contribution to the energy from the Coulomb attraction of the electron to the nuclei?.
- Figure 3.1 Absorption lines of the sun’s atmosphere.
- F ¼ e(E þ v B where e and v are the charge and velocity, respectively, of the particle..
- Figure 3.3 The position vectors r e and r n of the electron and nucleus, measured from some origin O..
- is the reduced mass of the electron – nucleus system..
- The vector analog of the Taylor series is.
- is the electric dipole moment of the electron – nucleus pair.
- In the Appendix we show that the electron oscillator model can be regarded as a good approximation to the quantum theory of the interaction of an atom with light..
- dt ¼ 0, i.e., the total number of atoms N 1 þ N 2 in the upper and lower states of the transition stays the same..
- The peak value of the absorption rate is.
- Far out in the wings of the Lorentzian, where jn n 0 j d n 0 , there is very little absorption.
- (3.4.35) for absorption in terms of the spontaneous emission rate A 21 for the E 2 ! E 1 transition.
- The narrower the width of S(n), the easier it is to satisfy (3.5.4).
- The historical significance of the Planck spectrum in the development of quantum.
- “classical limit” of the Planck spectrum..
- 3.13, how- ever, only a small part of the radiation from the heated filament lies in the visible..
- (3.7.5) are the foundation for a considerable part of the theory of lasers..
- 3pe 0 h c 3 jx m 1 m 2 j where x m 1 m 2 is the matrix element between states m 1 and m 2 of the electron coordinate x.
- (For a multielectron atom, x is the sum of the position vectors of all the electrons.) In the case of g 2.
- and will examine the solution of the S equation, d.
- under the following interpretation of the effect of collisions..
- (3.8.4) for the collisionless displacement, except for the appearance of the new g c term.
- The linewidth of the collision-broadened lineshape is [Eq.
- Collisions completely interrupt the phase of the oscillation.
- It is convenient to express this in terms of the atomic (or molecular) weights M X and M Y.
- e 4(nn 0 ) 2 ln 2=dn 2 D , (3:9:9) and we recognize that d n D is the width (FWHM) of the Doppler absorption curve, since (Fig.
- (3:9:12) for the ratio of the Doppler width to the resonance frequency is also useful..
- Each peak falls in the remote wing of the other function (see Fig.
- will result in a (homogeneous) linewidth of the form (3.11.2).
- populations are independent of the field intensity.
- Figure 3.20 Absorption cross section of the sodium D 2 line [Eq.
- (3.13.9)] for different values of the temperature T.
- (3.14.6) in which the field frequency v is very large compared to any of the transition frequencies v j.
- where 1 b ¼ n 2 b e 0 is the dielectric permittivity of the background.
- and introducing the oscillator strength f of the resonant transition, we have.
- while the expectation value of the electron coordinate is.
- h z 2 12 E, (3 : A : 22) where k z l ¼ k x l ^ z is the component of k x l along the direction of the electric field.
- Does your estimate indicate that molecular vibrations lie in the infrared region of the spectrum?.
- (1.5.2)? What is the physical meaning of the differences in the form of these two equations?.
- where I n (0) is the spectral brightness of the radiation input to the cell..
- [Note that the spectrum of the emitted radiation is identical to the absorption lineshape S(n.
- I n (L) 2hn 3 =c 2 e hn=k B T 1 , where T is the temperature of the medium..
- In Chapter 1 the growth rate of the number of laser photons in the cavity was described by an amplification coefficient a.
- Each of the mirrors of Fig.
- number of atoms in level 2 is n 2 ¼ N 2 V g , where V g is the volume of the gain medium..
- Likewise the total number of atoms in the lower level of the laser transition is n 1 ¼ N 1 V g .
- ¼ PN as a result of the pumping process.
- 2 hn 31 N T G which, because of the approximation DN t N T , is the same as (4.7.15).
- We further assume that the intensity I n of the field is constant in time.
- where we have used A s 2 1 for the spontaneous emission rate of the sodium D 2 line (Section 3.13).
- The FWHM radiative linewidth of the sodium D 2 line is [Eq.
- The electromagnetic energy density u is proportional to the square of the electric field: 3.
- sin 2 kz or, in terms of the intensity I n .
- interference of the two traveling-wave fields.
- Thus, g(n) varies with z on the scale of the laser wavelength..
- Saturation of the absorption or gain coefficient is more complicated in the case of inhomogeneous broadening.
- Consider the saturation of the gain coefficient when there is Doppler broadening.
- (b) Determine the steady-state values of the three level populations..
- Usually, only one of the mirrors is transmitting (Fig.
- This ratio is called the quantum efficiency of the three-level laser.
- Similarly n 0 / n 30 is the quantum efficiency of the ideal four-level laser.
- (t þ s)I (þ) ¼ 1 2 (t þ s)I ¼ g t lI: (5:4:5) Note that the one-way intensity I n (þ) ¼ I = 2 in the direction of the output mirror is inde- pendent of z