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William Klemperer

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42: 440:, a field of fundamental importance for all of molecular- and nano-science. Before Klemperer introduced spectroscopy with supersonic beams, the spectra of weakly bound species were almost unknown, having been restricted to dimers of a few very light systems. Scattering measurements provided precise intermolecular potentials for atom–atom systems, but provided at best only limited information on the anisotropy of atom–molecule potentials. 321: 203: 463:. The observed microwave transitions all involved a simultaneous change in rotational and tunneling energy. The tunneling frequency is extremely sensitive to the height and shape of the inter-conversion barrier, and thus samples the potential in the classically forbidden regions. Resolved tunneling splittings proved to be common in the spectra of weakly bound molecular dimers. 429:
extremely stable molecule and thus its isoelectronic analog, HCO, whose structure and spectra could be well predicted by analogy, would also be stable, linear, and have a strong but sparse spectrum. Further, the chemical models he was developing predicted that HCO would be one of the most abundant molecular species. Laboratory spectra of HCO (taken later by Claude Woods
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the questions that could be asked. Nowadays it is routine for microwave and infrared spectroscopists to follow his "two step synthesis" to obtain the spectrum of a weakly bound complex: "Buy the components and expand." Klemperer quite literally changed the study of the intermolecular forces between molecules from a qualitative to a quantitative science.
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was the first hydrogen bonded complex to be studied by these new techniques, and it was a puzzle. Instead of the simple rigid-rotor spectrum, which would have produced a 1 to 0 transition at 12 GHz, the lowest frequency transition was observed at 19 GHz. Arguing by analogy to the well known
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He foresaw that he could synthesize dimers of almost any pair of molecules he could dilute in his beam and study their minimum energy structure in exquisite detail by rotational spectroscopy. This was later extended to other spectral regions by Klemperer and many others, and has qualitatively changed
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Klemperer's early work concentrated on the infrared spectroscopy of small molecules that are only stable in the gas phase at high temperatures. Among these are the alkali halides, for many of which he obtained the first vibrational spectra. The work provided basic structural data for many oxides and
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Klemperer helped to found the field of interstellar chemistry. In interstellar space, densities and temperatures are extremely low, and all chemical reactions must be exothermic, with no activation barriers. The chemistry is driven by ion-molecule reactions, and Klemperer's modeling of those that
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Klemperer arrived at this prediction by taking the data seriously. The radio telescope data showed an isolated transition with no hyperfine splitting; thus there were no nuclei in the carrier of the signal with spin of one or greater nor was it a free radical with a magnetic moment. HCN is an
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occur in molecular clouds has led to a remarkably detailed understanding of their rich highly non-equilibrium chemistry. Klemperer assigned HCO as the carrier of the mysterious but universal "X-ogen" radio-astronomical line at 89.6 GHz, which had been reported by D. Buhl and L.E. Snyder.
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fluorides, and gave insight into the details of the bonding. It also led Klemperer to recognize the potential of molecular beams in spectroscopy, and in particular the use of the electric resonance technique to address fundamental problems in structural chemistry.
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Bill Klemperer was born in New York City in 1927 as the child of two physicians. He and his younger brother were raised in New York and New Rochelle. He graduated from New Rochelle High School in 1944 and then enlisted in the
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Klemperer introduced the technique of supersonic cooling as a spectroscopic tool, which has increased the intensity of molecular beams and also simplified the spectra.
520: 853: 433:,) proved him right and thereby demonstrated that Herbst and Klemperer's models provided a predictive framework for our understanding of interstellar chemistry. 783: 793: 452:
tunneling-inversion spectrum of ammonia, Klemperer recognized that the key to understanding the spectrum was to recognize that HF–HF was undergoing
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After one semester as an instructor at Berkeley, Bill returned to Harvard in July 1954. Though his initial appointment was as an instructor of
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T.R. Dyke, B.J. Howard and W. Klemperer (1972). "Radio Frequency and Microwave Spectrum of the Hydrogen Fluoride Dimer: A Nonrigid Molecule",
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Each rotational level was split into two tunneling states, with an energy separation equal to the tunneling rate divided by the
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E. Herbst and W. Klemperer (1973). "The Formation and Depletion of Molecules in Dense Interstellar Clouds",
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The Bomem-Michelson Award for the advancement of the field of vibrational spectroscopy. awarded by the
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S.E. Novick, P.B. Davies, T.R. Dyke and W. Klemperer (1973). "Polarity of van der Waals Molecules",
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in 1950, majoring in Chemistry, and obtained a Ph.D. in Physical Chemistry under the direction of
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Inaugural George C. Pimentel Memorial Lecturer, Chemistry Department, UC Berkeley. 1991-2.
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The Distinguished Service Medal, awarded by the U.S. National Science Foundation, 1981
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and 1979-81 as Assistant Director for Mathematical and Physical Sciences at the U.S.
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Video of Klemperer's Faraday Medal Lecture on the Chemistry of Interstellar Space
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that predicted an abundance of the molecular HCO ion that was later confirmed by
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methods into chemical physics research, greatly increasing the understanding of
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D. Buhl and L.E. Snyder (1970). "Unidentified Interstellar Microwave Line",
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W. Klemperer (1970). "Carrier of the Interstellar 89.190 GHz Line",
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in Physical Chemistry, awarded by the American Chemical Society, 1994
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The greatest impact of Klemperer's work has been in the study of
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from the Maryland Section of the American Chemical Society, 1992
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to FH–FH, interchanging the roles of proton donor and acceptor.
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Bill Klemperer has had many awards and honors, which include:
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W. Klemperer (1995). "Some Spectroscopic Reminiscences" ,
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Members of the United States National Academy of Sciences
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between atoms and molecules through development of the
149:(October 6, 1927 – November 5, 2017) was an American 128: 118: 108: 86: 74: 55: 32: 161:. Klemperer is most widely known for introducing 521:Earle K. Plyler Prize for Molecular Spectroscopy 46:William Klemperer (captured by Stewart Novick, 794:Klemperer's C.V + publication list up to 2003. 8: 864:United States Navy personnel of World War II 177:formed in supersonic expansions, pioneering 554:The Faraday Medal and Lectureship from the 231:. Unsourced material may be challenged and 568:Honorary Citizen of Toulouse, France, 2000 40: 29: 824:University of California, Berkeley alumni 405:Learn how and when to remove this message 251:Learn how and when to remove this message 859:Fellows of the American Physical Society 661:Journal of the American Chemical Society 574:from the American Chemical Society, 2001 583: 477:Fellow of the American Physical Society 854:Scientists from New Rochelle, New York 572:E. Bright Wilson Award in Spectroscopy 561:Honorary Doctor of Science from the 484:American Academy of Arts and Sciences 7: 745:Annual Reviews in Physical Chemistry 629: 627: 625: 623: 597: 595: 593: 591: 589: 587: 343:adding citations to reliable sources 229:adding citations to reliable sources 303:. He also served as an advisor to 282:University of California, Berkeley 95:University of California, Berkeley 25: 299:. He was a visiting scientist at 319: 201: 874:New Rochelle High School alumni 603:"Remembering William Klemperer" 330:needs additional citations for 829:20th-century American chemists 1: 47: 491:National Academy of Sciences 272:. He obtained an A.B. from 761:Journal of Chemical Physics 297:National Science Foundation 890: 869:United States Navy sailors 844:Harvard University faculty 556:Royal Society of Chemistry 497:John Price Wetherill Medal 819:Harvard University alumni 677:The Astrophysical Journal 525:American Physical Society 511:American Chemical Society 159:molecular spectroscopists 140: 101: 39: 779:Faculty Homepage@Harvard 723:R.C. Woods, T.A. Dixon, 268:, where he trained as a 729:Physical Review Letters 635:"William Klemperer, 90" 175:van der Waals molecules 167:nonbonding interactions 171:microwave spectroscopy 607:chemistry.harvard.edu 563:University of Chicago 507:Irving Langmuir Award 438:intermolecular forces 339:improve this article 293:Cambridge University 289:analytical chemistry 225:improve this section 147:William A. Klemperer 18:William A. Klemperer 639:The Harvard Gazette 509:, awarded by the 354:"William Klemperer" 266:U.S. Navy Air Corps 155:chemical physicists 501:Franklin Institute 454:quantum tunnelling 284:, in early 1954. 278:George C. Pimentel 274:Harvard University 135:George C. Pimentel 123:Harvard University 91:Harvard University 549:Peter Debye Award 523:, awarded by the 499:, awarded by the 449:hydrogen fluoride 415: 414: 407: 389: 301:Bell Laboratories 261: 260: 253: 144: 143: 103:Scientific career 69:New York City, US 34:William Klemperer 16:(Redirected from 881: 767: 757: 751: 741: 735: 721: 715: 705: 699: 689: 683: 673: 667: 657: 651: 650: 648: 646: 631: 618: 617: 615: 613: 599: 532:Coblentz Society 410: 403: 399: 396: 390: 388: 347: 323: 315: 256: 249: 245: 242: 236: 205: 197: 183:molecular clouds 130:Doctoral advisor 81: 65: 63: 49: 44: 30: 27:American chemist 21: 889: 888: 884: 883: 882: 880: 879: 878: 834:Spectroscopists 799: 798: 775: 770: 758: 754: 742: 738: 722: 718: 706: 702: 690: 686: 674: 670: 658: 654: 644: 642: 633: 632: 621: 611: 609: 601: 600: 585: 581: 558:(England), 1995 489:Elected to the 482:Elected to the 469: 461:Planck constant 411: 400: 394: 391: 348: 346: 336: 324: 313: 257: 246: 240: 237: 222: 206: 195: 187:radio astronomy 87:Alma mater 79: 78:5 November 2017 70: 67: 61: 59: 51: 35: 28: 23: 22: 15: 12: 11: 5: 887: 885: 877: 876: 871: 866: 861: 856: 851: 846: 841: 836: 831: 826: 821: 816: 811: 801: 800: 797: 796: 791: 786: 781: 774: 773:External links 771: 769: 768: 752: 736: 716: 700: 684: 668: 652: 619: 582: 580: 577: 576: 575: 569: 566: 559: 552: 545: 538: 535: 528: 517: 514: 504: 494: 487: 480: 468: 465: 413: 412: 327: 325: 318: 312: 309: 259: 258: 209: 207: 200: 194: 191: 179:astrochemistry 163:molecular beam 142: 141: 138: 137: 132: 126: 125: 120: 116: 115: 110: 106: 105: 99: 98: 88: 84: 83: 82:(aged 90) 76: 72: 71: 68: 66:6 October 1927 57: 53: 52: 45: 37: 36: 33: 26: 24: 14: 13: 10: 9: 6: 4: 3: 2: 886: 875: 872: 870: 867: 865: 862: 860: 857: 855: 852: 850: 847: 845: 842: 840: 839:Astrochemists 837: 835: 832: 830: 827: 825: 822: 820: 817: 815: 812: 810: 807: 806: 804: 795: 792: 790: 787: 785: 782: 780: 777: 776: 772: 765: 762: 756: 753: 749: 746: 740: 737: 733: 730: 726: 725:R.J. 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Index

William A. Klemperer

Harvard University
University of California, Berkeley
Chemist
Harvard University
Doctoral advisor
George C. Pimentel
chemist
chemical physicists
molecular spectroscopists
molecular beam
nonbonding interactions
microwave spectroscopy
van der Waals molecules
astrochemistry
molecular clouds
radio astronomy

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U.S. Navy Air Corps
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Harvard University
George C. Pimentel
University of California, Berkeley

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