# Multiple-Electron Atoms

All atoms except hydrogen are multiple-electron atoms. The physical and chemical properties of elements are directly related to the number of electrons a neutral atom has. The periodic table of the elements groups elements with similar properties into columns. This systematic organization is related to the number of electrons in a neutral atom, called the atomic number, $Z$. We shall see in this section that the exclusion principle is key to the underlying explanations, and that it applies far beyond the realm of atomic physics.

In 1925, the Austrian physicist Wolfgang Pauli (see [link]) proposed the following rule: No two electrons can have the same set of quantum numbers. That is, no two electrons can be in the same state. This statement is known as the Pauli exclusion principle, because it excludes electrons from being in the same state. The Pauli exclusion principle is extremely powerful and very broadly applicable. It applies to any identical particles with half-integral intrinsic spin—that is, having $s=\mathrm{1/2,\; 3/2,\; ...}$ Thus no two electrons can have the same set of quantum numbers.

Let us examine how the exclusion principle applies to electrons in atoms. The quantum numbers involved were defined in Quantum Numbers and Rules as $\mathrm{n,\; l,}\phantom{\rule{0.25em}{0ex}}{m}_{l}\mathrm{,\; s}$, and ${m}_{s}$. Since $s$ is always $1/2$ for electrons, it is redundant to list $s$, and so we omit it and specify the state of an electron by a set of four numbers $\left(n,\phantom{\rule{0.25em}{0ex}}l,\phantom{\rule{0.25em}{0ex}}{m}_{l},\phantom{\rule{0.25em}{0ex}}{m}_{s}\right)$. For example, the quantum numbers $\left(\mathrm{2,\; 1,\; 0,}\phantom{\rule{0.25em}{0ex}}-1/2\right)$ completely specify the state of an electron in an atom.

Since no two electrons can have the same set of quantum numbers, there are limits to how many of them can be in the same energy state. Note that $n$ determines the energy state in the absence of a magnetic field. So we first choose $n$, and then we see how many electrons can be in this energy state or energy level. Consider the $n=1$ level, for example. The only value $l$ can have is 0 (see [link] for a list of possible values once $n$ is known), and thus ${m}_{l}$ can only be 0. The spin projection ${m}_{s}$ can be either $+1/2$ or $-1/2$, and so there can be two electrons in the $n=1$ state. One has quantum numbers $\left(\mathrm{1,\; 0,\; 0,}\phantom{\rule{0.25em}{0ex}}+\mathrm{1/2}\right)$, and the other has $\left(\mathrm{1,\; 0,\; 0,}\phantom{\rule{0.25em}{0ex}}-\mathrm{1/2}\right)$. [link] illustrates that there can be one or two electrons having $n=1$, but not three.

# Shells and Subshells

Because of the Pauli exclusion principle, only hydrogen and helium can have all of their electrons in the $n=1$ state. Lithium (see the periodic table) has three electrons, and so one must be in the $n=2$ level. This leads to the concept of shells and shell filling. As we progress up in the number of electrons, we go from hydrogen to helium, lithium, beryllium, boron, and so on, and we see that there are limits to the number of electrons for each value of $n$. Higher values of the shell $n$ correspond to higher energies, and they can allow more electrons because of the various combinations of $l,\phantom{\rule{0.25em}{0ex}}{m}_{l}$, and ${m}_{s}$ that are possible. Each value of the principal quantum number $n$ thus corresponds to an atomic shell into which a limited number of electrons can go. Shells and the number of electrons in them determine the physical and chemical properties of atoms, since it is the outermost electrons that interact most with anything outside the atom.

The probability clouds of electrons with the lowest value of $l$ are closest to the nucleus and, thus, more tightly bound. Thus when shells fill, they start with $l=0$, progress to $l=1$, and so on. Each value of $l$ thus corresponds to a subshell.

The table given below lists symbols traditionally used to denote shells and subshells.

Shell | Subshell | |

$$n$$ | $$l$$ | Symbol |

1 | 0 | $$s$$ |

2 | 1 | $$p$$ |

3 | 2 | $$d$$ |

4 | 3 | $$f$$ |

5 | 4 | $$g$$ |

5 | $$h$$ | |

6 It is unusual to deal with subshells having $l$ greater than 6, but when encountered, they continue to be labeled in alphabetical order. |
$$i$$ |

To denote shells and subshells, we write $\text{nl}$ with a number for $n$ and a letter for $l$. For example, an electron in the $n=1$ state must have $l=0$, and it is denoted as a $1s$ electron. Two electrons in the *$n=1$* state is denoted as $1{s}^{2}$. Another example is an electron in the $n=2$ state with $l=1$, written as $2p$. The case of three electrons with these quantum numbers is written $2{p}^{3}$. This notation, called spectroscopic notation, is generalized as shown in [link].

Counting the number of possible combinations of quantum numbers allowed by the exclusion principle, we can determine how many electrons it takes to fill each subshell and shell.

List all the possible sets of quantum numbers for the $n=2$ shell, and determine the number of electrons that can be in the shell and each of its subshells.

**Strategy**

Given $n=2$ for the shell, the rules for quantum numbers limit $l$ to be 0 or 1. The shell therefore has two subshells, labeled $2s$ and $2p$. Since the lowest $l$ subshell fills first, we start with the $2s$ subshell possibilities and then proceed with the $2p$ subshell.

**Solution**

It is convenient to list the possible quantum numbers in a table, as shown below.

**Discussion**

It is laborious to make a table like this every time we want to know how many electrons can be in a shell or subshell. There exist general rules that are easy to apply, as we shall now see.

The number of electrons that can be in a subshell depends entirely on the value of $l$. Once $l$ is known, there are a fixed number of values of ${m}_{l}$, each of which can have two values for ${m}_{s}$ First, since ${m}_{l}$ goes from *$-l$* to *l* in steps of 1, there are $2l+1$ possibilities. This number is multiplied by 2, since each electron can be spin up or spin down. Thus the *maximum number of electrons that can be in a subshell* is $2\left(2l+1\right)$.

For example, the $2s$ subshell in [link] has a maximum of 2 electrons in it, since $2\left(2l+1\right)=2\left(0+1\right)=2$ for this subshell. Similarly, the $2p$ subshell has a maximum of 6 electrons, since $2\left(2l+1\right)=2\left(2+1\right)=6$. For a shell, the maximum number is the sum of what can fit in the subshells. Some algebra shows that the *maximum number of electrons that can be in a shell* is $2{n}^{2}$.

For example, for the first shell $n=1$, and so $2{n}^{2}=2$. We have already seen that only two electrons can be in the $n=1$ shell. Similarly, for the second shell, $n=2$, and so $2{n}^{2}=8$. As found in [link], the total number of electrons in the $n=2$ shell is 8.

How many subshells are in the $n=3$ shell? Identify each subshell, calculate the maximum number of electrons that will fit into each, and verify that the total is $2{n}^{2}$.

**Strategy**

Subshells are determined by the value of $l$; thus, we first determine which values of $\text{l}$ are allowed, and then we apply the equation “maximum number of electrons that can be in a subshell $=2\left(2l+1\right)$” to find the number of electrons in each subshell.

**Solution**

Since $n=3$, we know that $l$ can be $\mathrm{0,\; 1}$, or $2$; thus, there are three possible subshells. In standard notation, they are labeled the $3s$, $3p$, and $3d$ subshells. We have already seen that 2 electrons can be in an $s$ state, and 6 in a $p$ state, but let us use the equation “maximum number of electrons that can be in a subshell = $2\left(2l+1\right)$” to calculate the maximum number in each:

The equation “maximum number of electrons that can be in a shell = $2{n}^{2}$” gives the maximum number in the $n=3$ shell to be

**Discussion**

The total number of electrons in the three possible subshells is thus the same as the formula $2{n}^{2}$. In standard (spectroscopic) notation, a filled $n=3$ shell is denoted as $3{s}^{2}3{p}^{6}3{d}^{\text{10}}$. Shells do not fill in a simple manner. Before the $n=3$ shell is completely filled, for example, we begin to find electrons in the $n=4$ shell.

# Shell Filling and the Periodic Table

[link] shows electron configurations for the first 20 elements in the periodic table, starting with hydrogen and its single electron and ending with calcium. The Pauli exclusion principle determines the maximum number of electrons allowed in each shell and subshell. But the order in which the shells and subshells are filled is complicated because of the large numbers of interactions between electrons.

Element | Number of electrons (Z) | Ground state configuration | |||||

H | 1 | $$1{s}^{1}$$ | |||||

He | 2 | $$1{s}^{2}$$ | |||||

Li | 3 | $$1{s}^{2}$$ | $$2{s}^{1}$$ | ||||

Be | 4 | " | $$2{s}^{2}$$ | ||||

B | 5 | " | $$2{s}^{2}$$ | $$2{p}^{1}$$ | |||

C | 6 | " | $$2{s}^{2}$$ | $$2{p}^{2}$$ | |||

N | 7 | " | $$2{s}^{2}$$ | $$2{p}^{3}$$ | |||

O | 8 | " | $$2{s}^{2}$$ | $$2{p}^{4}$$ | |||

F | 9 | " | $$2{s}^{2}$$ | $$2{p}^{5}$$ | |||

Ne | 10 | " | $$2{s}^{2}$$ | $$2{p}^{6}$$ | |||

Na | 11 | " | $$2{s}^{2}$$ | $$2{p}^{6}$$ | $$3{s}^{1}$$ | ||

Mg | 12 | " | " | " | $$3{s}^{2}$$ | ||

Al | 13 | " | " | " | $$3{s}^{2}$$ | $$3{p}^{1}$$ | |

Si | 14 | " | " | " | $$3{s}^{2}$$ | $$3{p}^{2}$$ | |

P | 15 | " | " | " | $$3{s}^{2}$$ | $$3{p}^{3}$$ | |

S | 16 | " | " | " | $$3{s}^{2}$$ | $$3{p}^{4}$$ | |

Cl | 17 | " | " | " | $$3{s}^{2}$$ | $$3{p}^{5}$$ | |

Ar | 18 | " | " | " | $$3{s}^{2}$$ | $$3{p}^{6}$$ | |

K | 19 | " | " | " | $$3{s}^{2}$$ | $$3{p}^{6}$$ | $$4{s}^{1}$$ |

Ca | 20 | " | " | " | " | " | $$4{s}^{2}$$ |

Examining the above table, you can see that as the number of electrons in an atom increases from 1 in hydrogen to 2 in helium and so on, the lowest-energy shell gets filled first—that is, the $n=1$ shell fills first, and then the $n=2$ shell begins to fill. Within a shell, the subshells fill starting with the lowest *$l$*, or with the *$s$* subshell, then the $p$, and so on, usually until all subshells are filled. The first exception to this occurs for potassium, where the $4s$ subshell begins to fill before any electrons go into the $3d$ subshell. The next exception is not shown in [link]; it occurs for rubidium, where the $5s$ subshell starts to fill before the $4d$ subshell. The reason for these exceptions is that $l=0$ electrons have probability clouds that penetrate closer to the nucleus and, thus, are more tightly bound (lower in energy).

[link] shows the periodic table of the elements, through element 118. Of special interest are elements in the main groups, namely, those in the columns numbered 1, 2, 13, 14, 15, 16, 17, and 18.

The number of electrons in the outermost subshell determines the atom’s chemical properties, since it is these electrons that are farthest from the nucleus and thus interact most with other atoms. If the outermost subshell can accept or give up an electron easily, then the atom will be highly reactive chemically. Each group in the periodic table is characterized by its outermost electron configuration. Perhaps the most familiar is Group 18 (Group VIII), the noble gases (helium, neon, argon, etc.). These gases are all characterized by a filled outer subshell that is particularly stable. This means that they have large ionization energies and do not readily give up an electron. Furthermore, if they were to accept an extra electron, it would be in a significantly higher level and thus loosely bound. Chemical reactions often involve sharing electrons. Noble gases can be forced into unstable chemical compounds only under high pressure and temperature.

Group 17 (Group VII) contains the halogens, such as fluorine, chlorine, iodine and bromine, each of which has one less electron than a neighboring noble gas. Each halogen has 5 $p$ electrons (a ${p}^{\text{5}}$ configuration), while the $p$ subshell can hold 6 electrons. This means the halogens have one vacancy in their outermost subshell. They thus readily accept an extra electron (it becomes tightly bound, closing the shell as in noble gases) and are highly reactive chemically. The halogens are also likely to form singly negative ions, such as ${\mathrm{C1}}^{-}$, fitting an extra electron into the vacancy in the outer subshell. In contrast, alkali metals, such as sodium and potassium, all have a single $s$ electron in their outermost subshell (an ${s}^{1}$ configuration) and are members of Group 1 (Group I). These elements easily give up their extra electron and are thus highly reactive chemically. As you might expect, they also tend to form singly positive ions, such as ${\text{Na}}^{+}$, by losing their loosely bound outermost electron. They are metals (conductors), because the loosely bound outer electron can move freely.

Of course, other groups are also of interest. Carbon, silicon, and germanium, for example, have similar chemistries and are in Group 4 (Group IV). Carbon, in particular, is extraordinary in its ability to form many types of bonds and to be part of long chains, such as inorganic molecules. The large group of what are called transitional elements is characterized by the filling of the $d$ subshells and crossing of energy levels. Heavier groups, such as the lanthanide series, are more complex—their shells do not fill in simple order. But the groups recognized by chemists such as Mendeleev have an explanation in the substructure of atoms.

# Section Summary

- The state of a system is completely described by a complete set of quantum numbers. This set is written as $\left(\mathrm{n,\; l,}\phantom{\rule{0.25em}{0ex}}{m}_{l},\phantom{\rule{0.25em}{0ex}}{m}_{s}\right)$.
- The Pauli exclusion principle says that no two electrons can have the same set of quantum numbers; that is, no two electrons can be in the same state.
- This exclusion limits the number of electrons in atomic shells and subshells. Each value of $n$ corresponds to a shell, and each value of $l$ corresponds to a subshell.
- The maximum number of electrons that can be in a subshell is $2\left(2l+1\right)$.
- The maximum number of electrons that can be in a shell is $2{n}^{2}$.

# Conceptual Questions

Identify the shell, subshell, and number of electrons for the following: (a) $2{p}^{3}$. (b) $4{d}^{9}$. (c) $3{s}^{1}$. (d) $5{g}^{\text{16}}$.

Which of the following are not allowed? State which rule is violated for any that are not allowed. (a) $1{p}^{3}$ (b) $2{p}^{8}$(c) $3{g}^{\text{11}}$ (d) $4{f}^{2}$

# Problem Exercises

(a) How many electrons can be in the $n=4$ shell?

(b) What are its subshells, and how many electrons can be in each?

(a) 32. (b) $2\phantom{\rule{0.25em}{0ex}}\text{in}\phantom{\rule{0.25em}{0ex}}s,\phantom{\rule{0.25em}{0ex}}\text{6 in}\phantom{\rule{0.25em}{0ex}}p,\phantom{\rule{0.25em}{0ex}}\text{10 in}\phantom{\rule{0.25em}{0ex}}d,$ and 14 in $f$, for a total of 32.

(a) What is the minimum value of 1 for a subshell that has 11 electrons in it?

(b) If this subshell is in the $n=\text{5}$ shell, what is the spectroscopic notation for this atom?

(a) If one subshell of an atom has 9 electrons in it, what is the minimum value of $l$? (b) What is the spectroscopic notation for this atom, if this subshell is part of the $n=3$ shell?

(a) 2

(b) $3{d}^{9}$

(a) List all possible sets of quantum numbers $\left(n,\phantom{\rule{0.25em}{0ex}}l,\phantom{\rule{0.25em}{0ex}}{m}_{l},\phantom{\rule{0.25em}{0ex}}{m}_{s}\right)$ for the $n=3$ shell, and determine the number of electrons that can be in the shell and each of its subshells.

(b) Show that the number of electrons in the shell equals $2{n}^{2}$ and that the number in each subshell is $2\left(2l+1\right)$.

Which of the following spectroscopic notations are not allowed? (a) $5{s}^{1}$ (b) $1{d}^{1}$ (c) $4{s}^{3}$ (d) $3{p}^{7}$ (e) $5{g}^{15}$. State which rule is violated for each that is not allowed.

(b) $n\ge l$ is violated,

(c) cannot have 3 electrons in $s$ subshell since $3>(2l+1)=2\phantom{\rule{0.25em}{0ex}}$

(d) cannot have 7 electrons in $p$ subshell since $7>(2l+1)=2(2+1)=6$

Which of the following spectroscopic notations are allowed (that is, which violate none of the rules regarding values of quantum numbers)? (a) $1{s}^{1}$(b) $1{d}^{3}$(c) $4{s}^{2}$ (d) $3{p}^{7}$(e) $6{h}^{\text{20}}$

(a) Using the Pauli exclusion principle and the rules relating the allowed values of the quantum numbers $\left(n,\phantom{\rule{0.25em}{0ex}}l,\phantom{\rule{0.25em}{0ex}}{m}_{l},\phantom{\rule{0.25em}{0ex}}{m}_{s}\right)$, prove that the maximum number of electrons in a subshell is $2{n}^{2}$.

(b) In a similar manner, prove that the maximum number of electrons in a shell is 2*n*^{2}.

(a) The number of different values of ${m}_{l}$ is $\pm l,\pm (l-1),\text{...,}0$ for each $l>0$ and one for $l=0\Rightarrow (2l+1)\text{.}$ Also an overall factor of 2 since each ${m}_{l}$ can have ${m}_{s}$ equal to either $+1/2$ or $-1/2\Rightarrow 2(2l+1)$.

(b) for each value of $l$, you get $2(2l+1)$

$=\text{0, 1, 2, ...,}(n\text{\u20131})\Rightarrow 2\left\{\left[(2)(0)+1\right]+\left[(2)(1)+1\right]+\text{.}\text{.}\text{.}\text{.}+\left[(2)(n-1)+1\right]\right\}=\underset{\underset{n\phantom{\rule{0.25em}{0ex}}\text{terms}}{\ufe38}}{2\left[1+3+\text{.}\text{.}\text{.}+(2n-3)+(2n-1)\right]}$ to see that the expression in the box is $={n}^{2},$ imagine taking $(n-1)$ from the last term and adding it to first term $=2\left[1+(n\text{\u20131})+3+\text{.}\text{.}\text{.}+(2n-3)+(2n-1)\u2013(n-1)\right]=2\left[n+3+\text{.}\text{.}\text{.}\text{.}+(2n-3)+n\right]\text{.}$ Now take $(n-3)$ from penultimate term and add to the second term $2\underset{\underset{n\phantom{\rule{0.25em}{0ex}}\text{terms}}{\ufe38}}{\left[n+n+\text{.}\text{.}\text{.}+n+n\right]}={2n}^{2}$.

**Integrated Concepts**

Estimate the density of a nucleus by calculating the density of a proton, taking it to be a sphere 1.2 fm in diameter. Compare your result with the value estimated in this chapter.

**Integrated Concepts**

The electric and magnetic forces on an electron in the CRT in [link] are supposed to be in opposite directions. Verify this by determining the direction of each force for the situation shown. Explain how you obtain the directions (that is, identify the rules used).

The electric force on the electron is up (toward the positively charged plate). The magnetic force is down (by the RHR).

(a) What is the distance between the slits of a diffraction grating that produces a first-order maximum for the first Balmer line at an angle of $\text{20.0\xba}$?

(b) At what angle will the fourth line of the Balmer series appear in first order?

(c) At what angle will the second-order maximum be for the first line?

**Integrated Concepts**

A galaxy moving away from the earth has a speed of $\text{0.0100}c$. What wavelength do we observe for an ${n}_{\text{i}}=7$ to ${n}_{\text{f}}=2$ transition for hydrogen in that galaxy?

401 nm

**Integrated Concepts**

Calculate the velocity of a star moving relative to the earth if you observe a wavelength of 91.0 nm for ionized hydrogen capturing an electron directly into the lowest orbital (that is, a ${n}_{\text{i}}=\infty $ to ${n}_{\text{f}}=1$, or a Lyman series transition).

**Integrated Concepts**

In a Millikan oil-drop experiment using a setup like that in [link], a 500-V potential difference is applied to plates separated by 2.50 cm. (a) What is the mass of an oil drop having two extra electrons that is suspended motionless by the field between the plates? (b) What is the diameter of the drop, assuming it is a sphere with the density of olive oil?

(a) $6\text{.}\text{54}\times {\text{10}}^{-\text{16}}\phantom{\rule{0.25em}{0ex}}\text{kg}$

(b) $5\text{.}\text{54}\times {\text{10}}^{-7}\phantom{\rule{0.25em}{0ex}}\text{m}$

**Integrated Concepts**

What double-slit separation would produce a first-order maximum at $3\text{.}\text{00\xba}$ for 25.0-keV x rays? The small answer indicates that the wave character of x rays is best determined by having them interact with very small objects such as atoms and molecules.

**Integrated Concepts **

In a laboratory experiment designed to duplicate Thomson’s determination of ${q}_{e}/{m}_{e}$, a beam of electrons having a velocity of $6\text{.}\text{00}\times {\text{10}}^{7}\phantom{\rule{0.25em}{0ex}}\text{m/s}$ enters a $\text{5.00}\times {\text{10}}^{-3}\phantom{\rule{0.25em}{0ex}}\text{T}$ magnetic field. The beam moves perpendicular to the field in a path having a 6.80-cm radius of curvature. Determine ${q}_{e}/{m}_{e}$ from these observations, and compare the result with the known value.

$1\text{.}\text{76}\times {\text{10}}^{\text{11}}\phantom{\rule{0.25em}{0ex}}\text{C/kg}$ , which agrees with the known value of $1\text{.}\text{759}\times {\text{10}}^{\text{11}}\phantom{\rule{0.25em}{0ex}}\text{C/kg}$ to within the precision of the measurement

**Integrated Concepts**

Find the value of $l$, the orbital angular momentum quantum number, for the moon around the earth. The extremely large value obtained implies that it is impossible to tell the difference between adjacent quantized orbits for macroscopic objects.

**Integrated Concepts**

Particles called muons exist in cosmic rays and can be created in particle accelerators. Muons are very similar to electrons, having the same charge and spin, but they have a mass 207 times greater. When muons are captured by an atom, they orbit just like an electron but with a smaller radius, since the mass in ${a}_{\text{B}}=\frac{{h}^{2}}{{\mathrm{4\pi}}^{2}{m}_{e}{\text{kq}}_{e}^{2}}=\text{0.529}\times {\text{10}}^{-\text{10}}\phantom{\rule{0.25em}{0ex}}\text{m}$ is 207 ${m}_{e}$.

(a) Calculate the radius of the $n=1$ orbit for a muon in a uranium ion ($Z=\text{92}$).

(b) Compare this with the 7.5-fm radius of a uranium nucleus. Note that since the muon orbits inside the electron, it falls into a hydrogen-like orbit. Since your answer is less than the radius of the nucleus, you can see that the photons emitted as the muon falls into its lowest orbit can give information about the nucleus.

(a) 2.78 fm

(b) 0.37 of the nuclear radius.

**Integrated Concepts**

Calculate the minimum amount of energy in joules needed to create a population inversion in a helium-neon laser containing $1\text{.}\text{00}\times {\text{10}}^{-4}$ moles of neon.

**Integrated Concepts**

A carbon dioxide laser used in surgery emits infrared radiation with a wavelength of $\text{10.6 \mu m}$. In 1.00 ms, this laser raised the temperature of ${\text{1.00 cm}}^{3}$ of flesh to $\text{100\xbaC}$ and evaporated it.

(a) How many photons were required? You may assume flesh has the same heat of vaporization as water. (b) What was the minimum power output during the flash?

(a) $1\text{.}\text{34}\times {\text{10}}^{\text{23}}$

(b) 2.52 MW

**Integrated Concepts**

Suppose an MRI scanner uses 100-MHz radio waves.

(a) Calculate the photon energy.

(b) How does this compare to typical molecular binding energies?

**Integrated Concepts**

(a) An excimer laser used for vision correction emits 193-nm UV. Calculate the photon energy in eV.

(b) These photons are used to evaporate corneal tissue, which is very similar to water in its properties. Calculate the amount of energy needed per molecule of water to make the phase change from liquid to gas. That is, divide the heat of vaporization in kJ/kg by the number of water molecules in a kilogram.

(c) Convert this to eV and compare to the photon energy. Discuss the implications.

(a) 6.42 eV

(b) $7.27\times {\text{10}}^{-\text{20}}\phantom{\rule{0.25em}{0ex}}\text{J/molecule}$

(c) 0.454 eV, 14.1 times less than a single UV photon. Therefore, each photon will evaporate approximately 14 molecules of tissue. This gives the surgeon a rather precise method of removing corneal tissue from the surface of the eye.

**Integrated Concepts**

A neighboring galaxy rotates on its axis so that stars on one side move toward us as fast as 200 km/s, while those on the other side move away as fast as 200 km/s. This causes the EM radiation we receive to be Doppler shifted by velocities over the entire range of ±200 km/s. What range of wavelengths will we observe for the 656.0-nm line in the Balmer series of hydrogen emitted by stars in this galaxy. (This is called line broadening.)

**Integrated Concepts**

A pulsar is a rapidly spinning remnant of a supernova. It rotates on its axis, sweeping hydrogen along with it so that hydrogen on one side moves toward us as fast as 50.0 km/s, while that on the other side moves away as fast as 50.0 km/s. This means that the EM radiation we receive will be Doppler shifted over a range of $\pm \text{50}\mathrm{.0\; km/s}$. What range of wavelengths will we observe for the 91.20-nm line in the Lyman series of hydrogen? (Such line broadening is observed and actually provides part of the evidence for rapid rotation.)

91.18 nm to 91.22 nm

**Integrated Concepts**

Prove that the velocity of charged particles moving along a straight path through perpendicular electric and magnetic fields is $v=E/B$. Thus crossed electric and magnetic fields can be used as a velocity selector independent of the charge and mass of the particle involved.

**Unreasonable Results**

(a) What voltage must be applied to an X-ray tube to obtain 0.0100-fm-wavelength X-rays for use in exploring the details of nuclei? (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent?

(a) $1\text{.}\text{24}\times {\text{10}}^{\text{11}}\phantom{\rule{0.25em}{0ex}}\text{V}$

(b) The voltage is extremely large compared with any practical value.

(c) The assumption of such a short wavelength by this method is unreasonable.

**Unreasonable Results**

A student in a physics laboratory observes a hydrogen spectrum with a diffraction grating for the purpose of measuring the wavelengths of the emitted radiation. In the spectrum, she observes a yellow line and finds its wavelength to be 589 nm. (a) Assuming this is part of the Balmer series, determine ${n}_{\text{i}}$, the principal quantum number of the initial state. (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent?

**Construct Your Own Problem**

The solar corona is so hot that most atoms in it are ionized. Consider a hydrogen-like atom in the corona that has only a single electron. Construct a problem in which you calculate selected spectral energies and wavelengths of the Lyman, Balmer, or other series of this atom that could be used to identify its presence in a very hot gas. You will need to choose the atomic number of the atom, identify the element, and choose which spectral lines to consider.

**Construct Your Own Problem**

Consider the Doppler-shifted hydrogen spectrum received from a rapidly receding galaxy. Construct a problem in which you calculate the energies of selected spectral lines in the Balmer series and examine whether they can be described with a formula like that in the equation $\frac{1}{\lambda}=R\left(\frac{1}{{n}_{\text{f}}^{2}}-\frac{1}{{n}_{\text{i}}^{2}}\right)$, but with a different constant $R$.

### Tập tin đính kèm

- build-an-atom_en.jar

- College Physics
- Preface
- Introduction: The Nature of Science and Physics
- Kinematics
- Introduction to One-Dimensional Kinematics
- Displacement
- Vectors, Scalars, and Coordinate Systems
- Time, Velocity, and Speed
- Acceleration
- Motion Equations for Constant Acceleration in One Dimension
- Problem-Solving Basics for One-Dimensional Kinematics
- Falling Objects
- Graphical Analysis of One-Dimensional Motion

- Two-Dimensional Kinematics
- Dynamics: Force and Newton's Laws of Motion
- Introduction to Dynamics: Newton’s Laws of Motion
- Development of Force Concept
- Newton’s First Law of Motion: Inertia
- Newton’s Second Law of Motion: Concept of a System
- Newton’s Third Law of Motion: Symmetry in Forces
- Normal, Tension, and Other Examples of Forces
- Problem-Solving Strategies
- Further Applications of Newton’s Laws of Motion
- Extended Topic: The Four Basic Forces—An Introduction

- Further Applications of Newton's Laws: Friction, Drag, and Elasticity
- Uniform Circular Motion and Gravitation
- Work, Energy, and Energy Resources
- Linear Momentum and Collisions
- Statics and Torque
- Rotational Motion and Angular Momentum
- Introduction to Rotational Motion and Angular Momentum
- Angular Acceleration
- Kinematics of Rotational Motion
- Dynamics of Rotational Motion: Rotational Inertia
- Rotational Kinetic Energy: Work and Energy Revisited
- Angular Momentum and Its Conservation
- Collisions of Extended Bodies in Two Dimensions
- Gyroscopic Effects: Vector Aspects of Angular Momentum

- Fluid Statics
- Fluid Dynamics and Its Biological and Medical Applications
- Introduction to Fluid Dynamics and Its Biological and Medical Applications
- Flow Rate and Its Relation to Velocity
- Bernoulli’s Equation
- The Most General Applications of Bernoulli’s Equation
- Viscosity and Laminar Flow; Poiseuille’s Law
- The Onset of Turbulence
- Motion of an Object in a Viscous Fluid
- Molecular Transport Phenomena: Diffusion, Osmosis, and Related Processes

- Temperature, Kinetic Theory, and the Gas Laws
- Heat and Heat Transfer Methods
- Thermodynamics
- Introduction to Thermodynamics
- The First Law of Thermodynamics
- The First Law of Thermodynamics and Some Simple Processes
- Introduction to the Second Law of Thermodynamics: Heat Engines and Their Efficiency
- Carnot’s Perfect Heat Engine: The Second Law of Thermodynamics Restated
- Applications of Thermodynamics: Heat Pumps and Refrigerators
- Entropy and the Second Law of Thermodynamics: Disorder and the Unavailability of Energy
- Statistical Interpretation of Entropy and the Second Law of Thermodynamics: The Underlying Explanation

- Oscillatory Motion and Waves
- Introduction to Oscillatory Motion and Waves
- Hooke’s Law: Stress and Strain Revisited
- Period and Frequency in Oscillations
- Simple Harmonic Motion: A Special Periodic Motion
- The Simple Pendulum
- Energy and the Simple Harmonic Oscillator
- Uniform Circular Motion and Simple Harmonic Motion
- Damped Harmonic Motion
- Forced Oscillations and Resonance
- Waves
- Superposition and Interference
- Energy in Waves: Intensity

- Physics of Hearing
- Electric Charge and Electric Field
- Introduction to Electric Charge and Electric Field
- Static Electricity and Charge: Conservation of Charge
- Conductors and Insulators
- Coulomb’s Law
- Electric Field: Concept of a Field Revisited
- Electric Field Lines: Multiple Charges
- Electric Forces in Biology
- Conductors and Electric Fields in Static Equilibrium
- Applications of Electrostatics

- Electric Potential and Electric Field
- Electric Current, Resistance, and Ohm's Law
- Circuits, Bioelectricity, and DC Instruments
- Magnetism
- Introduction to Magnetism
- Magnets
- Ferromagnets and Electromagnets
- Magnetic Fields and Magnetic Field Lines
- Magnetic Field Strength: Force on a Moving Charge in a Magnetic Field
- Force on a Moving Charge in a Magnetic Field: Examples and Applications
- The Hall Effect
- Magnetic Force on a Current-Carrying Conductor
- Torque on a Current Loop: Motors and Meters
- Magnetic Fields Produced by Currents: Ampere’s Law
- Magnetic Force between Two Parallel Conductors
- More Applications of Magnetism

- Electromagnetic Induction, AC Circuits, and Electrical Technologies
- Introduction to Electromagnetic Induction, AC Circuits and Electrical Technologies
- Induced Emf and Magnetic Flux
- Faraday’s Law of Induction: Lenz’s Law
- Motional Emf
- Eddy Currents and Magnetic Damping
- Electric Generators
- Back Emf
- Transformers
- Electrical Safety: Systems and Devices
- Inductance
- RL Circuits
- Reactance, Inductive and Capacitive
- RLC Series AC Circuits

- Electromagnetic Waves
- Geometric Optics
- Vision and Optical Instruments
- Wave Optics
- Introduction to Wave Optics
- The Wave Aspect of Light: Interference
- Huygens's Principle: Diffraction
- Young’s Double Slit Experiment
- Multiple Slit Diffraction
- Single Slit Diffraction
- Limits of Resolution: The Rayleigh Criterion
- Thin Film Interference
- Polarization
- *Extended Topic* Microscopy Enhanced by the Wave Characteristics of Light

- Special Relativity
- Introduction to Quantum Physics
- Atomic Physics
- Introduction to Atomic Physics
- Discovery of the Atom
- Discovery of the Parts of the Atom: Electrons and Nuclei
- Bohr’s Theory of the Hydrogen Atom
- X Rays: Atomic Origins and Applications
- Applications of Atomic Excitations and De-Excitations
- The Wave Nature of Matter Causes Quantization
- Patterns in Spectra Reveal More Quantization
- Quantum Numbers and Rules
- The Pauli Exclusion Principle

- Radioactivity and Nuclear Physics
- Medical Applications of Nuclear Physics
- Particle Physics
- Frontiers of Physics
- Atomic Masses
- Selected Radioactive Isotopes
- Useful Information
- Glossary of Key Symbols and Notation