An electron moves through a region of uniform electric

Monochromatic light (that is, light of a single wavelength) is to be absorbed by a sheet of photographic film and thus recorded on the film. Photon absorption will occur if the photon energy equals or exceeds 0.6 eV, the smallest amount of energy needed to dissociate an AgBr molecule in the film. (a) What is the greatest wavelength of light that can be recorded by the film? (b) In what region of the electromagnetic spectrum is this wavelength located?

How fast must an electron move to have a kinetic energy equal to the photon energy of sodium light at wavelength 590 nm?

At what rate does the Sun emit photons? For simplicity, assume that the Suns entire emission at the rate of 3.9 " 1026 W is at the single wavelength of 550 nm

A heliumneon laser emits red light at wavelength l ! 633 nm in a beam of diameter 3.5 mm and at an energy-emission rate of 5.0 mW. A detector in the beams path totally absorbs the beam. At what rate per unit area does the detector absorb photons?

The meter was once defined as 1 650 763.73 wavelengths of the orange light emitted by a source containing krypton-86 atoms. What is the photon energy of that light?

What is the photon energy for yellow light from a highway sodium lamp at a wavelength of 589 nm?

A light detector (your eye) has an area of 2.00 " 10#6 m2 and absorbs 80% of the incident light, which is at wavelength 500 nm. The detector faces an isotropic source, 3.00 m from the source. If the detector absorbs photons at the rate of exactly 4.000 s#1 , at what power does the emitter emit light?

The beam emerging from a 1.5 W argon laser (l ! 515 nm) has a diameter d of 3.0 mm. The beam is focused by a lens system with an effective focal length fL of 2.5 mm. The focused beam strikes a totally absorbing screen, where it forms a circular diffraction pattern whose central disk has a radius R given by 1.22fLl/d. It can be shown that 84% of the incident energy ends up within this central disk. At what rate are photons absorbed by the screen in the central disk of the diffraction pattern?

A 100 W sodium lamp (l ! 589 nm) radiates energy uniformly in all directions. (a) At what rate are photons emitted by the lamp? (b) At what distance from the lamp will a totally absorbing screen absorb photons at the rate of 1.00 photon/cm2 $s? (c) What is the photon flux (photons per unit area per unit time) on a small screen 2.00 m from the lamp?

A satellite in Earth orbit maintains a panel of solar cells of area 2.60 m2 perpendicular to the direction of the Suns light rays. The intensity of the light at the panel is 1.39 kW/m2 . (a) At what rate does solar energy arrive at the panel? (b) At what rate are solar photons absorbed by the panel? Assume that the solar radiation is monochromatic, with a wavelength of 550 nm, and that all the solar radiation striking the panel is absorbed. (c) How long would it take for a mole of photons to be absorbed by the panel?

An ultraviolet lamp emits light of wavelength 400 nm at the rate of 400 W. An infrared lamp emits light of wavelength 700 nm, also at the rate of 400 W. (a) Which lamp emits photons at the greater rate and (b) what is that greater rate?

Under ideal conditions, a visual sensation can occur in the human visual system if light of wavelength 550 nm is absorbed by the eyes retina at a rate as low as 100 photons per second. What is the corresponding rate at which energy is absorbed by the retina?

A special kind of lightbulb emits monochromatic light of wavelength 630 nm. Electrical energy is supplied to it at the rate of 60 W, and the bulb is 93% efficient at converting that energy to light energy. How many photons are emitted by the bulb during its lifetime of 730 h?

A light detector has an absorbing area of m2 and absorbs 50% of the incident light, which is at wavelength 600 nm. The detector faces an isotropic source, 12.0 m from the source. The energy E emitted by the source versus time t is given in Fig. 38-26 (Es = 7.2 nJ, ts = 2.0 s). At what rate are photons absorbed by the detector?

Light strikes a sodium surface, causing photoelectric emission. The stopping potential for the ejected electrons is 5.0 V, and the work function of sodium is 2.2 eV. What is the wavelength of the incident light?

Find the maximum kinetic energy of electrons ejected from a certain material if the materials work function is 2.3 eV and the frequency of the incident radiation is 3.0 " 1015 Hz.

The work function of tungsten is 4.50 eV. Calculate the speed of the fastest electrons ejected from a tungsten surface when light whose photon energy is 5.80 eV shines on the surface.

You wish to pick an element for a photocell that will operate via the photoelectric effect with visible light. Which of the following are suitable (work functions are in parentheses): tantalum (4.2 eV), tungsten (4.5 eV), aluminum (4.2 eV), barium (2.5 eV), lithium (2.3 eV)?

(a) If the work function for a certain metal is 1.8 eV, what is the stopping potential for electrons ejected from the metal when light of wavelength 400 nm shines on the metal? (b) What is the maximum speed of the ejected electrons?

Suppose the fractional efficiency of a cesium surface (with work function 1.80 eV) is 1.0 " 10 #16; that is, on average one electron is ejected for every 1016 photons that reach the surface. What would be the current of electrons ejected from such a surface if it were illuminated with 600 nm light from a 2.00 mW laser and all the ejected electrons took part in the charge flow?

X rays with a wavelength of 71 pm are directed onto a gold foil and eject tightly bound electrons from the gold atoms.The ejected electrons then move in circular paths of radius r in a region of uniform magnetic field . For the fastest of the ejected electrons, the product Br is equal to 1.88 " 10 #4 T$m. Find (a) the maximum kinetic energy of those electrons and (b) the work done in removing them from the gold atoms

The wavelength associated with the cutoff frequency for silver is 325 nm. Find the maximum kinetic energy of electrons ejected from a silver surface by ultraviolet light of wavelength 254 nm

Light of wavelength 200 nm shines on an aluminum surface; 4.20 eV is required to eject an electron. What is the kinetic energy of (a) the fastest and (b) the slowest ejected electrons? (c) What is the stopping potential for this situation? (d) What is the cutoff wavelength for aluminum?

In a photoelectric experiment using a sodium surface, you find a stopping potential of 1.85 V for a wavelength of 300 nm and a stopping potential of 0.820 V for a wavelength of 400 nm. From these data find (a) a value for the Planck constant, (b) the work function 1 for sodium, and (c) the cutoff wavelength l0 for sodium.

The stopping potential for electrons emitted from a surface illuminated by light of wavelength 491 nm is 0.710 V. When the incident wavelength is changed to a new value, the stopping potential is 1.43 V. (a) What is this new wavelength? (b) What is the work function for the surface?

An orbiting satellite can become charged by the photoelectric effect when sunlight ejects electrons from its outer surface. Satellites must be designed to minimize such charging because it can ruin the sensitive microelectronics. Suppose a satellite is coated with platinum, a metal with a very large work function (1 ! 5.32 eV). Find the longest wavelength of incident sunlight that can eject an electron from the platinum.

Light of wavelength 2.40 pm is directed onto a target containing free electrons. (a) Find the wavelength of light scattered at 30.0 from the incident direction. (b) Do the same for a scattering angle of 120.

(a) In MeV/c, what is the magnitude of the momentum associated with a photon having an energy equal to the electron rest energy? What are the (b) wavelength and (c) frequency of the corresponding radiation?

What (a) frequency, (b) photon energy, and (c) photon momentum magnitude (in keV/c) are associated with x rays having wavelength 35.0 pm?

What is the maximum wavelength shift for a Compton collision between a photon and a free proton?

What percentage increase in wavelength leads to a 75% loss of photon energy in a photonfree electron collision?

X rays of wavelength 0.0100 nm are directed in the positive direction of an x axis onto a target containing loosely bound electrons. For Compton scattering from one of those electrons, at an angle of 180, what are (a) the Compton shift, (b) the corresponding change in photon energy, (c) the kinetic energy of the recoiling electron, and (d) the angle between the positive direction of the x axis and the electrons direction of motion?

Calculate the percentage change in photon energy during a collision like that in Fig. 38-5 for f ! 90 and for radiation in (a) the microwave range, with l ! 3.0 cm; (b) the visible range, with l ! 500 nm; (c) the x- ray range, with l ! 25 pm; and (d) the gamma-ray range, with a gamma photon energy of 1.0 MeV. (e) What are your conclusions about the feasibility of detecting the Compton shift in these various regions of the electromagnetic spectrum, judging solely by the criterion of energy loss in a single photonelectron encounter?

A photon undergoes Compton scattering off a stationary free electron. The photon scatters at 90.0 from its initial direction; its initial wavelength is 3.00 " 10#12 m. What is the electrons kinetic energy?

Calculate the Compton wavelength for (a) an electron and (b) a proton. What is the photon energy for an electromagnetic wave with a wavelength equal to the Compton wavelength of (c) the electron and (d) the proton?

Gamma rays of photon energy 0.511 MeV are directed onto an aluminum target and are scattered in various directions by loosely bound electrons there. (a) What is the wavelength of the incident gamma rays? (b) What is the wavelength of gamma rays scattered at 90.0 to the incident beam? (c) What is the photon energy of the rays scattered in this direction?

Consider a collision between an x-ray photon of initial energy 50.0 keV and an electron at rest, in which the photon is scattered backward and the electron is knocked forward. (a) What is the energy of the backscattered photon? (b) What is the kinetic energy of the electron?

Show that when a photon of energy E is scattered from a free electron at rest, the maximum kinetic energy of the recoiling electron is given by

Through what angle must a 200 keV photon be scattered by a free electron so that the photon loses 10% of its energy?

What is the maximum kinetic energy of electrons knocked out of a thin copper foil by Compton scattering of an incident beam of 17.5 keV x rays? Assume the work function is negligible.

What are (a) the Compton shift )l, (b) the fractional Compton shift )l/l, and (c) the change )E in photon energy for light of wavelength l ! 590 nm scattering from a free, initially stationary electron if the scattering is at 90 to the direction of the incident beam? What are (d) )l, (e) )l/l, and (f) )E for 90 scattering for photon energy 50.0 keV (x-ray range)?

The Sun is approximately an ideal blackbody radiator with a surface temperature of 5800 K. (a) Find the wavelength at which its spectral radiancy is maximum and (b) identify the type of electromagnetic wave corresponding to that wavelength. (See Fig. 33-1.) (c) As we shall discuss in Chapter 44, the universe is approximately an ideal blackbody radiator with radiation emitted when atoms first formed. Today the spectral radiancy of that radiation peaks at a wavelength of 1.06 mm (in the microwave region). What is the corresponding temperature of the universe?

Just after detonation, the fireball in a nuclear blast is approximately an ideal blackbody radiator with a surface temperature of about 1.0 " 107 K. (a) Find the wavelength at which the thermal radiation is maximum and (b) identify the type of electromagnetic wave corresponding to that wavelength. (See Fig. 33-1.) This radiation is almost immediately absorbed by the surrounding air molecules, which produces another ideal blackbody radiator with a surface temperature of about 1.0 " 105 K. (c) Find the wavelength at which the thermal radiation is maximum and (d) identify the type of electromagnetic wave corresponding to that wavelength

For the thermal radiation from an ideal blackbody radiator with a surface temperature of 2000 K, let Ic represent the intensity per unit wavelength according to the classical expression for the spectral radiancy and IP represent the corresponding intensity per unit wavelength according to the Planck expression. What is the ratio Ic/IP for a wavelength of (a) 400 nm (at the blue end of the visible spectrum) and (b) 200 mm (in the far infrared)? (c) Does the classical expression agree with the Planck expression in the shorter wavelength range or the longer wavelength range?

Assuming that your surface temperature is 98.6F and that you are an ideal blackbody radiator (you are close), find (a) the wavelength at which your spectral radiancy is maximum, (b) the power at which you emit thermal radiation in a wavelength range of 1.00 nm at that wavelength, from a surface area of 4.00 cm2 , and (c) the corresponding rate at which you emit photons from that area. Using a wavelength of 500 nm (in the visible range), (d) recalculate the power and (e) the rate of photon emission. (As you have noticed, you do not visibly glow in the dark.)

Calculate the de Broglie wavelength of (a) a 1.00 keV electron, (b) a 1.00 keV photon, and (c) a 1.00 keV neutron.

In an old-fashioned television set, electrons are accelerated through a potential difference of 25.0 kV. What is the de Broglie wavelength of such electrons? (Relativity is not needed.)

The smallest dimension (resolving power) that can be resolved by an electron microscope is equal to the de Broglie wavelength of its electrons.What accelerating voltage would be required for the electrons to have the same resolving power as could be obtained using 100 keV gamma rays?

Singly charged sodium ions are accelerated through a potential difference of 300 V. (a) What is the momentum acquired by such an ion? (b) What is its de Broglie wavelength?

Electrons accelerated to an energy of 50 GeV have a de Broglie wavelength l small enough for them to probe the structure within a target nucleus by scattering from the structure. Assume that the energy is so large that the extreme relativistic relation p ! E/c between momentum magnitude p and energy E applies. (In this extreme situation, the kinetic energy of an electron is much greater than its rest energy.) (a) What is l? (b) If the target nucleus has radius R ! 5.0 fm, what is the ratio R/l?

The wavelength of the yellow spectral emission line of sodium is 590 nm. At what kinetic energy would an electron have that wavelength as its de Broglie wavelength?

A stream of protons, each with a speed of 0.9900c, are directed into a two-slit experiment where the slit separation is 4.00 " 10#9 m. A two-slit interference pattern is built up on the viewing screen.What is the angle between the center of the pattern and the second minimum (to either side of the center)?

What is the wavelength of (a) a photon with energy 1.00 eV, (b) an electron with energy 1.00 eV, (c) a photon of energy 1.00 GeV, and (d) an electron with energy 1.00 GeV?

An electron and a photon each have a wavelength of 0.20 nm.What is the momentum (in kg $m/s) of the (a) electron and (b) photon? What is the energy (in eV) of the (c) electron and (d) photon?

The highest achievable resolving power of a microscope is limited only by the wavelength used; that is, the smallest item that can be distinguished has dimensions about equal to the wavelength. Suppose one wishes to see inside an atom. Assuming the atom to have a diameter of 100 pm, this means that one must be able to resolve a width of, say, 10 pm. (a) If an electron microscope is used, what minimum electron energy is required? (b) If a light microscope is used, what minimum photon energy is required? (c) Which microscope seems more practical? Why?

The existence of the atomic nucleus was discovered in 1911 by Ernest Rutherford, who properly interpreted some experiments in which a beam of alpha particles was scattered from a metal foil of atoms such as gold. (a) If the alpha particles had a kinetic energy of 7.5 MeV, what was their de Broglie wavelength? (b) Explain whether the wave nature of the incident alpha particles should have been taken into account in interpreting these experiments. The mass of an alpha particle is 4.00 u (atomic mass units), and its distance of closest approach to the nuclear center in these experiments was about 30 fm. (The wave nature of matter was not postulated until more than a decade after these crucial experiments were first performed.)

A nonrelativistic particle is moving three times as fast as an electron. The ratio of the de Broglie wavelength of the particle to that of the electron is 1.813 " 10 #4 . By calculating its mass, identify the particle.

What are (a) the energy of a photon corresponding to wavelength 1.00 nm, (b) the kinetic energy of an electron with de Broglie wavelength 1.00 nm, (c) the energy of a photon corresponding to wavelength 1.00 fm, and (d) the kinetic energy of an electron with de Broglie wavelength 1.00 fm?

If the de Broglie wavelength of a proton is 100 fm, (a) what is the speed of the proton and (b) through what electric potential would the proton have to be accelerated to acquire this speed?

Suppose we put A ! 0 in Eq. 38-24 and relabeled B as c0. (a) What would the resulting wave function then describe? (b) How, if at all, would Fig. 38-13 be altered?

The function c(x) displayed in Eq. 38-27 can describe a free particle, for which the potential energy is U(x) 0 in Schrdingers equation (Eq. 38-19).Assume now that U(x) ! U0 ! a constant in that equation. Show that Eq. 38-27 is a solution of Schrdingers equation, with giving the angular wave number k of the particle.

Show that Eq. 38-24 is indeed a solution of Eq. 38-22 by substituting c(x) and its second derivative into Eq. 38-22 and noting that an identity results

(a) Write the wave function c(x) displayed in Eq. 38-27 in the form c(x) ! a ' ib, where a and b are real quantities. (Assume that c0 is real.) (b) Write the time-dependent wave function &(x, t) that corresponds to c(x) written in this form.

Show that the angular wave number k for a nonrelativistic free particle of mass m can be written as in which K is the particles kinetic energy.

(a) Let n ! a ' ib be a complex number, where a and b are real (positive or negative) numbers. Show that the product nn* is always a positive real number. (b) Let m ! c ' id be another complex number. Show that |nm| ! |n| |m|.

In Eq. 38-25 keep both terms, putting A ! B ! c0. The equation then describes the superposition of two matter waves of equal amplitude, traveling in opposite directions. (Recall that this is the condition for a standing wave.) (a) Show that |&(x, t)|2 is then given by (b) Plot this function, and demonstrate that it describes the square of the amplitude of a standing matter wave. (c) Show that the nodes of this standing wave are located at and l is the de Broglie wavelength of the particle. (d) Write a similar expression for the most probable locations of the particle.

The uncertainty in the position of an electron along an x axis is given as 50 pm, which is about equal to the radius of a hydrogen atom. What is the least uncertainty in any simultaneous measurement of the momentum component px of this electron?

You will find in Chapter 39 that electrons cannot move in definite orbits within atoms, like the planets in our solar system. To see why, let us try to observe such an orbiting electron by using a light microscope to measure the electrons presumed orbital position with a precision of, say, 10 pm (a typical atom has a radius of about 100 pm). The wavelength of the light used in the microscope must then be about 10 pm. (a) What would be the photon energy of this light? (b) How much energy would such a photon impart to an electron in a head-on collision? (c) What do these results tell you about the possibility of viewing an atomic electron at two or more points along its presumed orbital path? (Hint: The outer electrons of atoms are bound to the atom by energies of only a few electron-volts.)

Figure 38-13 shows a case in which the momentum component px of a particle is fixed so that )px ! 0; then, from Heisenbergs uncertainty principle (Eq. 38-28), the position x of the particle is completely unknown. From the same principle it follows that the opposite is also true; that is, if the position of a particle is exactly known ()x ! 0), the uncertainty in its momentum is infinite. Consider an intermediate case, in which the position of a particle is measured, not to infinite precision, but to within a distance of l/2p, where l is the particles de Broglie wavelength. Show that the uncertainty in the (simultaneously measured) momentum component is then equal to the component itself; that is, )px ! p. Under these circumstances, would a measured momentum of zero surprise you? What about a measured momentum of 0.5p? Of 2p? Of 12p?

An electron moves through a region of uniform electric potential of #200 V with a (total) energy of 500 eV. What are its (a) kinetic energy (in electron-volts), (b) momentum, (c) speed, (d) de Broglie wavelength, and (e) angular wave number?

For the arrangement of Figs. 38-14 and 38-15, electrons in the incident beam in region 1 have energy E 800 eV and the potential step has a height of U1 ! 600 eV. What is the angular wave number in (a) region 1 and (b) region 2? (c) What is the reflection coefficient? (d) If the incident beam sends 5.00 " 105 electrons against the potential step, approximately how many will be reflected?

For the arrangement of Figs. 38-14 and 38-15, electrons in the incident beam in region 1 have a speed of 1.60 107 m/s and region 2 has an electric potential of V2 ! #500 V.What is the angular wave number in (a) region 1 and (b) region 2? (c) What is the reflection coefficient? (d) If the incident beam sends 3.00 " 109 electrons against the potential step, approximately how many will be reflected?

The current of a beam of electrons, each with a speed of 900 m/s, is 5.00 mA. At one point along its path, the beam encounters a potential step of height #1.25 mV. What is the current on the other side of the step boundary?

Consider a potential energy barrier like that of Fig. 38-17 but whose height Ub is 6.0 eV and whose thickness L is 0.70 nm. What is the energy of an incident electron whose transmission coefficient is 0.0010?

A 3.0 MeV proton is incident on a potential energy barrier of thickness 10 fm and height 10 MeV. What are (a) the transmission coefficient T, (b) the kinetic energy Kt the proton will have on the other side of the barrier if it tunnels through the barrier, and (c) the kinetic energy Kr it will have if it reflects from the barrier? A 3.0 MeV deuteron (the same charge but twice the mass as a proton) is incident on the same barrier. What are (d) T, (e) Kt , and (f) Kr?

(a) Suppose a beam of 5.0 eV protons strikes a potential energy barrier of height 6.0 eV and thickness 0.70 nm, at a rate equivalent to a current of 1000 A. How long would you have to waiton averagefor one proton to be transmitted? (b) How long would you have to wait if the beam consisted of electrons rather than protons?

An electron with total energy E 5.1 eV approaches a barrier of height Ub 6.8 eV and thickness L 750 pm. What percentage change in the transmission coefficient T occurs for a 1.0% change in (a) the barrier height, (b) the barrier thickness, and (c) the kinetic energy of the incident electron?

The current of a beam of electrons, each with a speed of 1.200 103 m/s, is 9.000 mA. At one point along its path, the beam encounters a potential barrier of height #4.719 mV and thickness 200.0 nm.What is the transmitted current?

Figure 38-13 shows that because of Heisenbergs uncertainty principle, it is not possible to assign an x coordinate to the position of a free electron moving along an x axis. (a) Can you assign a y or a z coordinate? (Hint: The momentum of the electron has no y or z component.) (b) Describe the extent of the matter wave in three dimensions.

A spectral emission line is electromagnetic radiation that is emitted in a wavelength range narrow enough to be taken as a sin-gle wavelength. One such emission line that is important in astronomy has a wavelength of 21 cm. What is the photon energy in the electromagnetic wave at that wavelength?

Using the classical equations for momentum and kinetic energy, show that an electrons de Broglie wavelength in nanometers can be written as , in which K is the electrons kinetic energy in electron- volts.

Derive Eq. 38-11, the equation for the Compton shift, from Eqs. 38-8, 38-9, and 38-10 by eliminating v and u.

Neutrons in thermal equilibrium with matter have an average kinetic energy of (3/2)kT, where k is the Boltzmann constant and T, which may be taken to be 300 K, is the temperature of the environment of the neutrons. (a) What is the average kinetic energy of such a neutron? (b) What is the corresponding de Broglie wavelength?

Consider a balloon filled with helium gas at room temperature and atmospheric pressure. Calculate (a) the average de Broglie wavelength of the helium atoms and (b) the average distance between atoms under these conditions. The average kinetic energy of an atom is equal to (3/2)kT, where k is the Boltzmann constant. (c) Can the atoms be treated as particles under these conditions? Explain

In about 1916, R. A. Millikan found the following stoppingpotential data for lithium in his photoelectric experiments: Wavelength (nm) 433.9 404.7 365.0 312.5 253.5 Stopping potential (V) 0.55 0.73 1.09 1.67 2.57 Use these data to make a plot like Fig. 38-2 (which is for sodium) and then use the plot to find (a) the Planck constant and (b) the work function for lithium

Show that |c| 2 ! |&| 2 , with c and & related as in Eq. 38-14. That is, show that the probability density does not depend on the time variable.

Show that )E/E, the fractional loss of energy of a photon during a collision with a particle of mass m, is given by where E is the energy of the incident photon, f4 is the frequency of the scattered photon, and f is defined as in Fig. 38-5

A bullet of mass 40 g travels at 1000 m/s. Although the bullet is clearly too large to be treated as a matter wave, determine what Eq. 38-17 predicts for the de Broglie wavelength of the bullet at that speed.

(a) The smallest amount of energy needed to eject an electron from metallic sodium is 2.28 eV. Does sodium show a photoelectric effect for red light, with l ! 680 nm? (That is, does the light cause electron emission?) (b) What is the cutoff wavelength for photoelectric emission from sodium? (c) To what color does that wavelength correspond?

Imagine playing baseball in a universe (not ours!) where the Planck constant is 0.60 J s and thus quantum physics affects macroscopic objects. What would be the uncertainty in the position of a 0.50 kg baseball that is moving at 20 m/s along an axis if the uncertainty in the speed is 1.0 m/s?