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Weber, M. J. “Frontmatter”
Handbook of Laser Wavelengths.
Ed. Marvin J. Weber
Boca Raton: CRC Press LLC, 1999
PERIODIC TABLE OF THE ELEMENTS
1
Group
IA
2
IIA
New Notation
Previous IUPAC Form
CAS Version
13
IIIB
IIIA
14
IVB
IVA
15
VB
VA
16
VIB
VIA
17
VIIB
VIIA
18
VIIIA
Shell
1
1.00794
1
+1
-1
2
He
4.002602
2
0
K
3
Li
+1
4
Be
+2
5
B
+3
6
C
+2
+4
-4
7
N
+ +2
+ +4
+ -1
- -3
8
O
-2
9
F
-1
10
Ne
0
Key to Chart
Atomic Number
Symbol
1995 Atomic Weight
50
Sn
118.710
-18-18-4
+2
+4
Oxidation States
6.941
2-1
9.012182
2-2
10.811
2-3
12.0107
2-4
14.00674
2-5
15.9994
2-6
18.9984032
2-7
20.1797
2-8
Electron
Configuration
K-L
11
Na
+1
12
Mg
+2
13
Al
+3
14
Si
+2
+4
-4
15
P
+3
+5
-3
16
S
+4
+6
-2
17
Cl
+1
+5
+7
-1
18
Ar
0
3
IIIA
IIIB
4
IVA
IVB
5
VA
VB
6
VIA
VIB
7
VIIA
VIIB
8
9
VIIIA
VIII
10
11
IB
IB
12
IIB
IIB
22.989770
2-8-1
24.3050
2-8-2
26.981538
2-8-3
28.0855
2-8-4
30.973761
2-8-5
32.066
2-8-6
35.4527
2-8-7
39.948
2-8-8
K-L-M
19
K
+1
20
Ca
+2
21
Sc
+3
22
Ti
+2
+3
+4
23
V
+2
+3
+4
+5
24
Cr
+2
+3
+6
25
Mn
+2
+3
+4
+7
26
Fe
+2
+3
27
Co
+2
+3
28
Ni
+2
+3
29
Cu
+1
+2
30
Zn
+2
31
Ga
+3
32
Ge
+2
+4
33
As
+3
+5
-3
34
Se
+4
+6
-2
35
Br
+1
+5
-1
36
Kr
0
39.0983
-8-8-1
40.078
-8-8-2
44.955910
-8-9-2
47.867
-8-10-2
50.9415
-8-11-2
51.9961
-8-13-1
55.845
-8-13-2
58.933200
-8-15-2
58.6934
-8-16-2
63.546
-8-18-1
65.39
-8-18-2
69.723
-8-18-3
72.61
-8-18-4
74.92160
-8-18-5
78.96
-8-18-6
79.904
-8-18-7
83.80
-8-18-8
-L-M-N
-8-13-2
37
Rb
+1
38
Sr
+2
39
Y
+3
40
Zr
+4
41
Nb
+3
+5
42
Mo
+6
43
Tc
+4
+6
+7
44
Ru
+3
45
Rh
+3
46
Pd
+2
+3
47
Ag
+1
48
Cd
+2
49
In
+3
50
Sn
+2
+4
51
Sb
+3
+5
-3
52
Te
+4
+6
-2
53
I
+1
+5
+7
-1
54
Xe
0
54.938049
85.4678
-18-8-1
87.62
-18-8-2
88.90585
-18-9-2
91.224
-18-10-2
92.90638
-18-12-1
95.94
-18-13-1
(98)
-18-13-2
101.07
-18-15-1
102.90550
-18-16-1
106.42
-18-18-0
107.8682
-18-18-1
112.411
-18-18-2
114.818
-18-18-3
118.710
-18-18 -4
121.760
-18-18-5
127.60
-18-18-6
126.90447
-18-18-7
131.29
-18-18-8
-M-N-O
55
Cs
+1
56
Ba
+2
57*
La
+3
72
Hf
+4
73
Ta
+5
74
W
+6
75
Re
+4
+6
+7
76
Os
+3
+4
77
Ir
+3
+4
78
Pt
+2
+4
79
Au
+1
+3
80
Hg
+1
+2
81
Tl
+1
+3
82
Pb
+2
+4
83
Bi
+3
+5
84
Po
+2
+4
85
At
86
Rn
0
132.90545
-18-8-1
137.327
-18-8-2
138.9055
-18-9-2
178.49
-32-10-2
180.9479
-32-11-2
183.84
-32-12-2
186.207
-32-13-2
190.23
-32-14-2
192.217
-32-15-2
195.078
-32-17-1
196.96655
-32-18-1
200.59
-32-18-2
204.3833
-32-18-3
207.2
-32-18-4
208.98038
-32-18-5
(209)
-32-18-6
(210)
-32-18-7
(222)
-32-18-8
-N-O-P
87
Fr
(223)
-18-8-1
+1
88
Ra
(226)
-18-8-2
+2
89**
Ac
(227)
-18-9-2
+3
104
Rf
(261)
-32-10-2
+4
105
Db
(262)
-32-11-2
106
Sg
(266)
-32-12-2
107
Bh
(264)
-32-13-2
108
Hs
(269)
-32-14-2
109
Mt
(268)
-32-15-2
110
Uun
(271)
-32-16-2
111
Uuu
112
Uub
(272)
-O-P-Q
58
Ce
+3
+4
59
Pr
+3
60
Nd
+3
61
Pm
+3
62
Sm
+2
+3
63
Eu
+2
+3
64
Gd
+3
65
Tb
+3
66
Dy
+3
67
Ho
+3
68
Er
+3
69
Tm
+3
70
Yb
+2
+3
71
Lu
+3
* Lanthanides
140.116
-19-9-2
140.90765
-21-8-2
144.24
-22-8-2
(145)
-23-8-2
150.36
-24-8-2
151.964
-25-8-2
157 .25
-25-9-2
158.92534
-27-8-2
162.50
-28-8-2
164.93032
-29-8-2
167.26
-30-8-2
168.93421
-31-8-2
173.04
-32-8-2
174.967
-32-9-2
-N-O-P
90
Th
232.0381
-18-10-2
+4
91
Pa
231.03588
-20-9-2
+5
+4
92
U
238.0289
-21-9-2
+ + + +6
93
Np
(237)
-22-9-2
+ + + +6
94
Pu
(244)
-24-8-2
+ + + +6
95
Am
(243)
-25-8-2
+ + + +6
96
Cm
(247)
-25-9-2
+3
97
Bk
(247)
-27-8-2
+3
+4
98
Cf
(251)
-28-8-2
+3
99
Es
(252)
-29-8-2
+3
100
Fm
(257)
-30-8-2
+3
101
Md
(258)
-31-8-2
+2
+3
102
No
(259)
-32-8-2
+2
+3
103
Lr
(262)
-32-9-2
+3
** Actinides
-O-P-Q
The new IUPAC format numbers the groups from 1 to 18. The previous IUPAC numbering system and the system used by Chemical Abstracts Service (CAS) are also shown. For radioactive
elements that do not occur in nature, the mass number of the most stable isotope is given in parentheses.
References
1. G. J. Leigh, Editor, Nomenclature of Inorganic Chemistry , Blackwell Scientific Publications, Oxford, 1990.
2. Chemical and Engineering News , 63(5), 27, 1985.
3. Atomic Weights of the Elements, 1995, Pure & Appl. Chem. , 68, 2339, 1996.
© CRC Press
1999
LLC
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Handbook of
Laser
Wavelengths
Marvin J. Weber Ph.D.
Lawence Berkeley National Laboratory
University of California
Berkeley, California
1999 by CRC PRESS LLC
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© CRC Press
1999
LLC
809217776.032.png
Foreword
It is really amazing how many laser transitions and how many laser wavelengths have
been discovered. They cover nearly every class of material, from free electrons through
gases, liquids, and solids. It is perhaps even more amazing that the comprehensive
listing in this book could be compiled through the collaboration of leading experts in
each of the fields.
Forty years ago, when Charles Townes and I were first trying to discover how lasers
might be made, it seemed very difficult. We had always been taught that the world was
pretty close to being in equilibrium, even though masers had shown that you could
sometimes get away from it. As Ali Javan pointed out then, when discussing possible
gas lasers, there are many processes tending to restore equilibrium. Moreover, since
nobody had ever made a laser, we thought it might be very difficult. There might be
some hidden problem that we had over-looked. But that turned out to be wrong and
some kinds of lasers are quite easy to make once you know how.
When thinking of possible laser materials, I for one had plenty of blind spots and poorly
based prejudices. For instance, I knew that the optical gain, for a given excess of
excited atoms, would be inversely proportional to the spectral linewidth. Thus I felt that
narrow lines were essential, overlooking the fact that some broad bands in things like
organic dyes have large oscillator strengths and so make up for their large width. Also,
for a time I couldn't see why anyone would want to use a laser to pump another, thereby
compounding their inefficiencies.
Fortunately, lasers attracted the interest and stimulated the imagination of large
numbers of very clever people. Some of them had specialized knowledge of things like
crystal growing, very hot plasmas, or semiconductor luminescence. From their work
have come the very many types of lasers listed in this book. Some of the discoveries
resulted from careful study and planning, while others were serendipitous.
Many lasers have been discovered but never put to any practical use. In some cases,
gases are too corrosive or too easily adsorbed on the walls. In others, crystalline
materials are too difficult to grow in useful sizes, or are too hygroscopic. Sometimes,
there just isn’t any obvious need for that kind of laser. Perhaps someone browsing in this
book will find something for a new use, or will think of ways to overcome the apparent
difficulties.
Perhaps also in the future, or even now, someone will recognize other blind spots and
will see new approaches to yield still more types of useful lasers.
Arthur L. Schawlow
Stanford University
1999 by CRC PRESS LLC
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