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Nobel Prize winner in physics

Walter Bothe 1954, Rudolf Mössbauer 1961, Hans Jensen 1963

Nobel Prize winner in physics

The Nobel Prize has been awarded since 1901 and is considered the world's highest award for significant achievements in physics, chemistry, physiology and medicine, as well as for literature and peace. The prize was founded by the Swede Alfred Nobel. Having achieved great wealth with the invention of dynamite, Nobel stipulated in his will in 1895 that almost his entire fortune should go into a fund "the interest on which is to be distributed annually as a prize to those who have been of the greatest benefit to mankind in the past year." Nobel went on to explain that it was his express wish that the most worthy should receive the prize, regardless of nationality. The award ceremony is held in Stockholm every year on December 10, the anniversary of Nobel's death. The Nobel Peace Prize is awarded in Oslo.

We can be proud of the fact that our region has also produced numerous Nobel Prize winners. In the physics category, these are Walther Bothe, Hans Jensen and Rudolf Mößbauer.

Walther Wilhelm Georg Bothe

was born on January 8, 1891 in Oranienburg near Berlin, the son of master watchmaker Friedrich Bothe and seamstress Charlotte Bothe. All that is known about Walther's childhood is that he was interested in science, painting and music and enjoyed playing pieces by Bach on the piano.

After graduating from the Oberrealschule in Berlin, he studied physics, mathematics, chemistry and musicology at the Humboldt University in Berlin from 1908. He financed his studies with scholarships and odd jobs. In 1913, he passed his teaching exam and initially worked at the Agricultural College in Berlin.

At the same time, he worked on his doctoral thesis. When Bothe asked his physics professor Max Planck if he could do his doctorate with him, Planck asked him, "What topic did you have in mind?" Bothe replies that he would like to devote himself to explaining the refraction and reflection of light from the scattering of individual atoms. Planck replies "Yes, you could try that" and accepts Bothe as one of his only seven doctoral students. Even before the outbreak of the First World War, Bothe received his doctorate in 1914 and went to work as an assistant to Hans Geiger (3), the head of the new Lauboratorium for Radioactivity at the Physikalisch-Technische Reichsanstalt. With Geiger, the most important nuclear physicist in Germany, he learned how to conduct experiments. Geiger's experiments on the scattering of alpha rays are among the beginnings of experimental atomic physics.

However, Bothe was soon drafted and was taken prisoner of war in Siberia in 1915, where he learned Russian and devoted himself to mathematical studies. When he was released in 1920, he married Varvara Belova in Moscow, whom he had already met in Berlin before the war, and returned to Berlin with her. There he continued his collaboration with Hans Geiger at the Laboratory for Radioactivity and worked both theoretically and experimentally on the scattering of electrons.

In 1924, Bothe and Geiger began experiments to investigate the Compton effect, discovered by Arthur Holly Compton in 1923 and named after him. When a photon, i.e. a "particle of light", hits an electron, a negatively charged elementary particle, it is scattered. When it hits the electron, the photons give off some of their energy, which increases their wavelength. The electron now has the energy of the photon and is pushed away, i.e. scattered. This is why this effect is also known as Compton scattering.

With their experiment, Bothe and Geiger want to find out whether a scattered photon and a recoil electron are always observed simultaneously, i.e. "coincident", in Compton scattering. To do this, they used the needle counter developed by Geiger, which reacts to ionizing radiation. This counting tube was further improved by Geiger and Müller in 1928 and became known as the "Geiger counter".

Bothe and Geiger developed the "coincidence method", which became a widely used technique in nuclear physics. It provides insight into the details of a reaction or decay. For their work, Geiger and Bothe also had to develop completely new electronic circuits and devices to electronically record the reaction of the counting tubes and automatically count the number of coincidence events in which both counting tubes react simultaneously, or almost simultaneously.

Their experimental set-up consists of two needle counters embedded in a hydrogen atmosphere, between whose common, non-contacting end wall an X-ray beam is directed. Hydrogen absorbs the X-rays only weakly, but scatters them strongly.

One of the counting tubes is open and therefore filled with hydrogen. The other counting tube, covered with a platinum foil, is filled with air. This counting tube does not react to electrons, as the platinum foil absorbs the recoil electrons. However, the photons penetrate the foil and release photoelectrons from the air and the foil, which the counting tube registers. The open counter tube, on the other hand, registers almost no photons, as these are hardly absorbed by the hydrogen. The recoil electrons, on the other hand, are measured.

Using the Koinizidendz method, Bothe and Geiger were able to prove beyond doubt the quantum nature of the photon and thus disprove the - at that time still widely accepted - view held by Niels Bohr and several other renowned physicists that two important physical principles, namely the conservation of energy and momentum, were only fulfilled statistically, i.e. on average, in Compton scattering, but were violated in the individual process.

Bothe summarized his work in several handbook articles, thus laying the methodological foundations for the analysis of scattering processes. When Geiger accepted an appointment at the University of Kiel in 1925, Bothe became his successor as head of the Lauboratorium for Radioactivity. At Geiger's generous suggestion, Bothe was assigned the coincidence method when the areas previously worked on together were divided up. The years of collaboration with Geiger, of whom he always spoke with great admiration and affection, marked a decisive turning point in Bothe's scientific career.

In 1925, Bothe habilitated under Max Planck at the University of Berlin with his thesis "On the elementary process of photoelectric electron triggering". In the following years, Bothe developed coincidence measurement into an important method for researching cosmic rays. He placed several of the latest Geiger-Müller counters on top of each other and arranged absorbing layers of different thicknesses between and above the counters in order to be able to determine the absorption of cosmic rays in different materials by reducing the number of coincidences accordingly. He hoped to gain profound insights from the investigation of cosmic radiation discovered by Victor Hess during balloon flights in 1912.

Together with the astronomer Werner Kolhörster, he carried out coincidence measurements in which rays were guided through Geiger counters and the response of the counting tubes was only indicated if the measurements were taken within a predetermined short time interval of each other. As this only happens when one and the same particle passes through all the counting tubes, only radiation from a specific direction is registered. With this new method of random counting, the path of a charged particle can be tracked through the counting tubes. This shows that the particles prefer to fall perpendicular to the earth's surface. If the apparatus is tilted towards the horizon, the intensity of incidence decreases. As the vertically incident particles have the shortest path through the Earth's atmosphere, they are absorbed the least, which clearly indicates the origin of the radiation under investigation outside the Earth.

With their experiments, Bothe and Kolhörster prove that cosmic radiation does not primarily consist of gamma rays, as previously assumed due to their high penetrating power, but of material particles with an energy of at least 1,000 million electron volts.

In 1930, Bothe was appointed Professor of Physics and Director of the Institute of Physics at the University of Giessen. He was the first to address quantum mechanics in his lectures and turned his institute into an important research center. When he shoots beryllium with alpha rays, he obtains an unusually penetrating radiation. However, he did not realize that it was a new particle. Two years later, Sir James Chadwick discovered the neutron and was awarded the Nobel Prize in 1935.

After the discovery of neutrons, experimental nuclear physics began to develop rapidly, thanks in part to the completion of the first accelerators and the enormous improvements in measuring and counting techniques.

In 1932, Bothe was appointed to the University of Heidelberg, but resigned from his professorship and the management of the institute after the Nazi regime came to power. In 1934, he became head of the physics department at the Kaiser Wilhelm Institute for Medical Research, which was founded in 1930 and consisted of four independent sub-institutes. This later became the Max Planck Institute for Nuclear Physics. Bothe was able to return to his basic research and work on the controlled nuclear fission chain reaction. He and his colleagues are among the first scientists to investigate nuclear reactions and the properties and structures of the atom, carry out nuclear spectroscopic studies and produce artificial isotopes.

During the Second World War, the Army Ordnance Office undertakes efforts to build nuclear weapons and has the best German nuclear physicists working on the so-called uranium project. Bothes Institute is also involved. When measuring the absorption of slow neutrons in graphite, he came to the conclusion that graphite was unsuitable as a nuclear moderator. This assessment prevented the National Socialists from producing nuclear weapons until the end of the war. It was not until 1945 that it was realized that Bothe had determined an incorrect value because the graphite he had used was contaminated. But could a scientist like Bothe, who worked so conscientiously and meticulously with such high concentration, really have made such a serious mistake? The first graphite-moderated reactor was built by Enrico Fermi in Chicago in 1945. The fission of uranium produces fast neutrons. Graphite slows them down and reflects them back into the reactor core, where they are then available for further fissions and thus maintain the nuclear chain reaction.

For his research, Bothe needs a cyclotron, a particle accelerator in which elementary particles, atomic nuclei, ionized atoms or molecules are accelerated to high speeds by electric fields. He succeeds in procuring the necessary funds and, together with his assistant Wolfgang Gentner in Heidelberg, constructs the first German cyclotron, which is used for the first time in the fall of 1943. After the Second World War, the Americans used the institute as an Aero-Medical Center and also the cyclotron. The physics department, however, was closed.

Although he was initially not allowed to work in his original field of nuclear physics, Bothe returned to the Institute of Physics at the University of Heidelberg as Director in 1945. He ensured that Hans Jensen was appointed to Heidelberg in 1949, put the cyclotron back into operation and carried out nuclear physics experiments with his students. (10) .

The Max Planck Society is founded as the successor to the Kaiser Wilhelm Society and Bothe is able to continue his work at the Institute of Physics in 1952, devoting himself to research in the fields of nuclear physics and cosmic radiation and working on the further development of nuclear spectroscopy.

However, progressive vasoconstriction, which even necessitated the amputation of a leg, eventually forced him to retire from research. From 1953, he was only able to take care of the management of the Institute of Physics.

Ten years after the death of Hans Geiger, Walther Bothe was awarded the Nobel Prize in Physics in 1954 for the development of the coincidence method and the discoveries he had made with it, together with Max Born, who was honored for his fundamental research in quantum mechanics. Unfortunately, Bothe is unable to travel to Stockholm for health reasons. At his request, his daughter Dr. Elena Riedel accepted the award.(11) The coincidence method is still one of the most important means of investigating cosmic rays and all types of nuclear and elementary particle processes.

Alongside other Nobel Prize winners, on July 15, 1955, Bothe signs an appeal to the world's politicians to renounce violence as a means of politics. On February 10, 1957, Prof. Dr. Walter Bothe (12) dies in Heidelberg after a long illness at the age of 66 and is laid to rest in the cemetery in Handschuhsheim.

Rudolf Ludwig Mößbauer

is born in Munich on January 31, 1929 as one of two children of the photo technician Ludwig Mößbauer and his wife Erna. He attended the Oberrealschule in Munich-Pasing. It sounds surprising, but physics is his weakest subject at school. However, he believes this is due to the bad teachers. He often visits the Deutsches Museum in Munich and is convinced that there is much more to what is taught at school. After passing his Abitur exams in 1948, he first completed an internship at the well-known Optische Werke Rodenstock and then decided to study physics at the Technische Hochschule München, now the Technical University of Munich.

In 1952, when Mößbauer was still in the middle of his studies, Heinz Meier-Leibnitz (14) was appointed to the Chair of Technical Physics at the Technical University of Munich. This chair includes the Laboratory for Technical Physics, which becomes an important nucleus for nuclear physics. Under his leadership, the first German nuclear research reactor was built, which went into operation in Garching near Munich in 1957 and became known as the "Atomic Egg" (15).

After graduating in 1955, Mößbauer joined Prof. Walther Bothe at the Institute of Physics at the Max Planck Institute for Medical Research in Heidelberg. Here he found the best conditions to research the passage of gamma rays through matter at the suggestion of his doctoral supervisor Heinz Maier-Leibnitz, a former colleague of Bothe.

Gamma rays differ from light rays in that they have a much shorter wavelength. The energy contained in a photon, i.e. a "particle of light", is inversely proportional to its wavelength. The photons of gamma rays have a much shorter wavelength than the light visible to our eyes and therefore a much higher energy.

The photons of visible light are produced in the electron shells of atoms when the energy state of the electrons changes. The amount of change in the energy state is an exact measure of the wavelength of the emitted photon. Conversely, photons of suitable energy, i.e. with a corresponding wavelength, can be absorbed by an atom of the same type, thereby increasing its energy state.

Gamma rays are not produced by energy changes in the electrons in the electron shell, but by energy changes in the atomic nuclei. Here too, as with visible light, there are absorption and emission processes. However, the relationships here are much more complicated.

The exact wavelength of the emitted or absorbed radiation depends on the state of motion of the emitter or absorber. We see something very similar in the so-called Doppler effect, which was first described by the Austrian physicist Christian Doppler in 1842. We are familiar with this phenomenon from everyday life as a sudden change in pitch from high to low as a sound source approaches and then moves away. A typical example is the changing pitch of the siren of a passing fire engine.

An example from astronomy is the red shift of light as a galaxy moves away. In this way, if the frequency of the source is known, its speed relative to the observer can be determined.

In the case of gamma radiation from atomic nuclei, however, it was observed that the emitted radiation was not readily absorbed by similar nuclei. Apparently, the energy contained in the emitted gamma quantum did not match the required excitation energy of the absorber.

Mössbauer uses the Doppler effect for his experimental setup. This means that he allows the source of the gamma rays to move towards and away from the sample at different speeds. In this way, he can determine exactly at what speed absorption occurs again and convert this speed into energy.

In 1957, during his experiments with gamma radiation in iridium-191, an isotope (the Greek word "isotope" refers to different types of atoms of the same chemical element) of the element iridium, he observed minimal deviations from the actually expected measurement result. When he investigated the reason for this unclear and initially seemingly negligible effect, he discovered the phenomenon that the γ-radiation emitted by an atomic nucleus can be absorbed by nuclei of the same isotope in another sample without any loss of energy.

Mössbauer finds the solution to the puzzle. If free atomic nuclei emit gamma rays, the physical law of conservation of momentum requires that the emitted particle - i.e. the gamma quantum - is not given all of its energy, but that part of this energy is consumed in the recoil of the emitting nucleus. The wavelength of the gamma radiation changes with the strength of the recoil, and a shift occurs between the absorption and emission lines.

However, if the emitting nucleus is not free, but bound in a solid, such as a molecule or crystal, this crystal absorbs the recoil momentum. Due to the unequal mass of the crystal, the energy shift is negligible. The emission or absorption is therefore "recoilless". This process is referred to as "recoilless nuclear resonance absorption". The emitting nucleus has a different spectral line than in the free state. The extraordinary energy sharpness of the gamma spectral line allows even the smallest changes in gamma energy to be determined with precision.

The Mössbauer effect can be explained more simply with a figurative comparison: If a child wants to jump from a small boat onto land, it lands in the water because the boat moves backwards due to the recoil during the jump. If the boat is in a frozen lake, it cannot move and the child receives all the energy from the jump and lands safely on the shore.

In Mössbauer's experiment, the gamma ray emitting iridium-191 atoms take on the role of the boat. And the rushing gamma particle, like the child, transmits a powerful shock to the atom, losing some of its energy in the process. However, if the atom is built into a crystal, the light particle can take all its energy with it, just like the child on the frozen lake.

The discovery of recoilless nuclear resonance absorption, i.e. the Mößbauer effect later named after him, became the basis for a completely new type of gamma spectroscopy (16). It represents the most precise method for determining energy changes in electromagnetic radiation in spectroscopy.

The Mössbauer effect enables a wide range of spectroscopic applications in nuclear and solid-state physics as well as in chemistry, biosciences, geology and archaeology, making even tiny splittings or line shifts visible and extremely accurate to measure. Even when the movements of the gamma ray sources are only a thousandth of a millimeter per second.

In 1960, with the help of high-precision Mößbauer spectroscopy, experimental proof of the red shift of gamma rays in the Earth's gravitational field predicted by Albert Einstein in his theory of general relativity was achieved.

And the Mößbauer effect is even used in space research. During the Mars mission, the "Spirit" and "Opportunity" robots use Mößbauer spectrometers to analyze the chemical composition of Martian rock. They measure the characteristic gamma radiation emitted by the atomic nuclei of certain elements when they are excited by radioactive radiation. The data they found shows that there are minerals on Mars that only form in the presence of water. This not only proves the earlier existence of water, but also that there must have been a much more oxygen-rich atmosphere than today.

Mößbauer completed his doctoral thesis entitled "Nuclear resonance fluorescence of gamma rays in iridium-191" at the end of October 1957 and was awarded his doctorate by Professor Maier-Leibnitz at the Technical University of Munich after the oral examination in January 1958.

Mößbauer then continued as a research assistant to Professor Heinz Maier-Leibniz in Munich until 1960, when he was invited by none other than Richard Feynman to conduct research at the renowned California Institute of Technology in Pasadena, the "Caltec". One year later, he was appointed full professor. In October 1961, he received an early morning phone call from Stockholm. Together with the American Robert Hofstadter, he was awarded the 1961 Nobel Prize in Physics for his research into the resonance absorption of gamma radiation and the associated discovery of the effect named after him.

He received the highest scientific award for the results and discoveries he had already made as a doctoral student at the Institute of Physics at the Max Planck Institute for Medical Research in Heidelberg between 1956 and 1958. At just 32 years old (17), he is one of the youngest Nobel Prize winners ever. According to Mößbauer, "it is young people who make a significant contribution to progress in physics, as they try things out and take unconventional paths that more experienced researchers would not take because they know too much." This was followed by countless honors from the most prestigious scientific institutions around the world.

Mößbauer remained in California for another two years before the Technical University succeeded in bringing him back to Munich as Professor of Experimental Physics in 1965. His condition for his return was fulfilled with the construction of a physics building in Munich-Garching with excellent facilities and staff. He was also granted permission to restructure the previously independent Institutes of Theory, Experimental Physics and Technical Physics into a physics department based on the American model.

Thanks to the interdisciplinary approach, Mößbauer achieves better conditions for research and teaching, which he sees as a unit. After all, Rudolf Mößbauer is not only interested in research, but also in teaching. He wants to get students excited about physics, which he succeeds in doing with his didactically brilliant lectures. He is committed to excellence and believes that "justice does not consist of pushing everyone down to the same level."

For Mößbauer, science is a language that connects all people in the world. He promotes international cooperation and scientific exchange, including with Soviet scientists during the Cold War. And he regularly invites guest scientists to Garching to conduct research in his working group. He wants to attract the best scientists to his university, also from abroad. He was not afraid to take a clear stance on problems such as the increasing hostility towards technology in society or the constantly growing bureaucracy.

In 1972, he took a leave of absence to head the Institut Laue-Langevin in Grenoble, named after the German physicist Max von Laue and the French physicist Paul Langevin, with one of the most powerful neutron sources in Europe at the time. He was excited by the task of breaking new scientific ground with research into neutrino physics. Initial experiments contradict the previous assumption that neutrinos, like light, have no mass.

He therefore began working on neutrino physics in Grenoble and established neutrino research in Munich after his return to the Technical University in 1977.

Rudolf Mößbauer remained full professor of experimental physics at the Technical University of Munich until his retirement in 1997 and continued his research into neutrinos, neutrons and nuclear fusion, i.e. the conversion of hydrogen into helium.

And he remained a passionate pianist throughout his life. There is even a grand piano in his laboratory, which he occasionally plays while working. He also enjoys photography and hiking.

Rudolf Mößbauer (18) died at the age of 82 on September 14, 2011 in Grünwald near Munich. (19) Not only his wife Christel and his children Susi, Peter and Regine, but also his university and colleagues mourn the loss of a great scientist.

Hans Jensen

Johannes Daniel Jensen,(20) known as "Hans" for short, was born in Hamburg on June 25, 1907 as the third child of gardener Karl Friedrich Jensen and his wife Helene Auguste. He initially attended elementary school here, but was later able to transfer to secondary school due to his extraordinary talent. He was particularly interested in the natural sciences. When he lost his parents in quick succession at the age of 15, his older sister Lisbeth took care of him and ensured that he was able to finish school and take his Abitur in 1926.

Supported by the German National Academic Foundation, he was able to study physics, mathematics, chemistry and philosophy at the universities of Hamburg and Freiburg im Breisgau. In 1931, he passed his state examination for the higher teaching profession, but decided to pursue an academic career. In 1932, he completed his doctorate with a dissertation on "Charge distribution in ions" (21) under Wilhelm Lenz and was employed as an assistant at the Institute for Theoretical Physics at the University of Hamburg. After his habilitation in theoretical physics in 1936, he also became a lecturer there.

Supported by the German National Academic Foundation, he was able to study physics, mathematics, chemistry and philosophy at the universities of Hamburg and Freiburg im Breisgau. In 1931, he passed his state examination for the higher teaching profession, but decided to pursue an academic career. In 1932, he completed his doctorate with a dissertation on "Charge distribution in ions" (21) under Wilhelm Lenz and was employed as an assistant at the Institute for Theoretical Physics at the University of Hamburg. After his habilitation in theoretical physics in 1936, he also became a lecturer there.

During the National Socialist era, when even outstanding achievements were no guarantee of a university career, all but a few of the Hamburg lecturers joined the NSDAP, which put Jensen under pressure to join. On the advice of two of his highly esteemed colleagues, Jensen decided to take this step in 1937 despite his reservations. The decisive factor was ultimately the fact that his wife Elisabeth would otherwise not have been allowed to continue her medical studies because she publicly supported a left-wing ASTA list.

In 1939, Jensen was ordered to join the Wehrmacht's weather service, but a year later he was released to work on the uranium project of German nuclear physicists. He was to develop a centrifuge system in Hamburg for the enrichment of fissile uranium. Under the direction of Werner Heisenberg, this was to be used to build nuclear weapons. But this did not happen. Due to an incorrect measurement carried out by Walther Bothe, graphite is ruled out as a material for the German reactor.

And Jensen informs his friend, the Danish nuclear physicist Niels Bohr (22), about the uranium project, even though he knows about his connections to the Allies. He later wrote about this in a letter: "On two trips to Norway (at the end of 1942 and 43), I myself had the opportunity to discuss the issue in detail with Bohr in Copenhagen, to ask for his approval for our activities, to report on the attitude of a not insignificant number of uranium physicists and to assure him that there was no danger that the Nazis could misuse the uranium." Whether the German scientists were sabotaging the project will never be clarified.

After Jensen had dealt with the statistical Thomas-Fermi model of the atomic shell in both his dissertation and his habilitation, he turned his attention to the structure of atomic nuclei at the end of the 1930s and published a paper on the state of the systematics of atomic nuclei at the time in 1939. In it, he deals for the first time with models of nuclear structure.

In 1941, the year his daughter Anne was born, Jensen was appointed Professor of Theoretical Physics at the Technical University of Hanover (23). However, the war years greatly impaired his research work.

In 1949, Prof. Jensen accepted an appointment at the University of Heidelberg and began to establish the Institute for Theoretical Physics. On his initiative, the university acquired the beautiful Merton House at Philosophenweg 16 in 1952 to set up the Institute of Theoretical Physics and the Central Library of Physics. Jensen lived in two rooms there and transformed the property into a flourishing garden with his own hands.

It was not until the end of the 1940s that Jensen was able to devote himself to his research again. Although much was already known about the atomic nucleus after the Second World War, its structure was still largely unknown. What is known is that protons and neutrons form particularly stable atomic nuclei when their number corresponds to one of the so-called magic numbers 2, 8, 20, 28, 50, 82 and 126. Jensen has found extensive experimental material for the existence of such magic numbers, but there is no theoretical explanation.

Atoms consist of a nucleus of nucleons, i.e. positively charged protons and electrically neutral neutrons, and an extended cloud of electrically negatively charged electrons. Almost the entire mass of the atom is combined in the tiny nucleus. In contrast, the diameter of the electron shell is between 20,000 and 150,000 times the size of the atomic nucleus.

By assuming that a nucleon should have different energies depending on whether it "rotates" in the same or opposite direction when orbiting the nucleus, Jensen made the breakthrough in 1948 to explain the magic numbers. The additional assumption of a particularly strong interaction between its intrinsic rotation, the "spin", and its orbital motion proves to be decisive.

In the early post-war years, it was difficult for German scientists to access international journals. Jensen was therefore delighted when he was able to travel to Copenhagen again in 1948 and read in an article by Maria Goeppert-Mayer (1906-1972), Professor of Physics at the University of Chicago, in an issue of "Physical Review" that she had also found experimental evidence for the "magic numbers" and was working on an explanation, as was he.

Jensen contacted her and an intensive scientific exchange developed between them, which ultimately led to them jointly developing the models they had previously developed independently of each other into the so-called "shell model" of the atomic nucleus.

The Danish nuclear physicist Niels Bohr had a major influence on their attempts to understand nuclei. However, while the droplet model developed by Niels Bohr in 1936 compares the atomic nucleus with a drop of water behaving according to the rules of mechanics, the shell model developed from this looks at the individual nucleons and their movement according to the laws of quantum mechanics (the "Pauli principle" named after the physicist Wolfgang Pauli).

For the development of the shell model, Jensen was awarded one half of the Nobel Prize in Physics in 1963 in equal shares with Maria Goeppert-Mayer, (24) while the other half went to Eugene Wigner for the discovery of the nuclear shell structure of the atomic nucleus, (25) who showed that most of the essential properties of nuclei follow from generally valid symmetries of the laws of motion.

Despite many honorable calls from Germany and abroad, Prof. Hans Jensen (26) remained loyal to Heidelberg University and helped Heidelberg to play a leading role in nuclear physics. He retired in 1969 and died unexpectedly on February 11, 1973 at the age of 65 in his Institute for Theoretical Physics in Heidelberg, which can still be found today at Philosophenweg 16. In 2007, it was given the name "Jensen House" and a memorial plaque commemorates the important researcher. (27)

Picture credits

  • 1 Alfred Nobel, public domain
  • 2 Walther Bothe, © Archive of the Order Pour le mérite for Sciences and Arts
  • 3 Hans Geiger 1928, public domain
  • 4 Geiger counter 1932, © Science Museum London.cc BY-SA 2.0
  • 5. experimental setup
  • 6 Kaiser Wilhelm Institute Heidelberg,
  • 7 Report of Heidelberg
  • 8. from left to right: Johannes Prast, Dr. Ingeborg Schmidt, Dr. Heinz Haber, Prof. Hubertus Strughold, Dr. Siegfried Gerathewohl and Dr. Heinrich Rose.
  • 9th cyclotron
  • 6th - 9th © The story of the US Army Medical Center in Heidelberg. National library of medicine, Bethesda Maryland. 1947
  • 10. cyclotron, 1952 © Archive of the MPG
  • 11 © NobelPrize.org.
  • 12 Walther Bothe 1954 public domain
  • 13 Rudolf Mössbauer
  • 14 Heinz Maier-Leibnitz, Bundesarchiv, B 145 Bild-F041738-0006 / Wienke, Ulrich / CC-BY-SA 3.0
  • 15. atomic egg in Garching of the then Technical University of Munich. © TUM
  • 15 Rudolf Mößbauer, 1961
  • 16. 1961 © Nobel Foundation archive
  • 17. 1961 © Nobel Foundation archive
  • 18 © picture-alliance dpa
  • 19. obituary
  • 20 Hans Jensen 1917, Jörn Scheer archive
  • 21. doctoral certificate
  • 22 Niels Bohr 1922 public domain
  • 23. certificate of appointment
  • 24 Hans Jensen picture-alliance/dpa
  • 25 Eugene Wigner, Maria Goeppert-Mayer, Hans Jensen 1963 © Nobel Foundation archive
  • 26 Hans Jensen 1963 © Nobel Foundation archive
  • 27 Jensen memorial plaque

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