Age, Biography and Wiki

Walter Heitler was born on 2 January, 1904 in Karlsruhe, German Empire, is a German physicist (1904-1981). Discover Walter Heitler's Biography, Age, Height, Physical Stats, Dating/Affairs, Family and career updates. Learn How rich is he in this year and how he spends money? Also learn how he earned most of networth at the age of 77 years old?

Popular As N/A
Occupation N/A
Age 77 years old
Zodiac Sign Capricorn
Born 2 January, 1904
Birthday 2 January
Birthplace Karlsruhe, German Empire
Date of death 15 November, 1981
Died Place Zollikon, Meilen, Switzerland
Nationality

We recommend you to check the complete list of Famous People born on 2 January. He is a member of famous with the age 77 years old group.

Walter Heitler Height, Weight & Measurements

At 77 years old, Walter Heitler height not available right now. We will update Walter Heitler's Height, weight, Body Measurements, Eye Color, Hair Color, Shoe & Dress size soon as possible.

Physical Status
Height Not Available
Weight Not Available
Body Measurements Not Available
Eye Color Not Available
Hair Color Not Available

Dating & Relationship status

He is currently single. He is not dating anyone. We don't have much information about He's past relationship and any previous engaged. According to our Database, He has no children.

Family
Parents Not Available
Wife Not Available
Sibling Not Available
Children Not Available

Walter Heitler Net Worth

His net worth has been growing significantly in 2023-2024. So, how much is Walter Heitler worth at the age of 77 years old? Walter Heitler’s income source is mostly from being a successful . He is from . We have estimated Walter Heitler's net worth, money, salary, income, and assets.

Net Worth in 2024 $1 Million - $5 Million
Salary in 2024 Under Review
Net Worth in 2023 Pending
Salary in 2023 Under Review
House Not Available
Cars Not Available
Source of Income

Walter Heitler Social Network

Instagram
Linkedin
Twitter
Facebook
Wikipedia
Imdb

Timeline

1904

Walter Heinrich Heitler (2 January 1904 – 15 November 1981) was a German physicist who made contributions to quantum electrodynamics and quantum field theory.

He brought chemistry under quantum mechanics through his theory of valence bonding.

1922

In 1922, Heitler began his study of physics at the Karlsruhe Technische Hochschule, in 1923 at the Humboldt University of Berlin, and in 1924 at the Ludwig Maximilian University of Munich (LMU), where he studied under both Arnold Sommerfeld and Karl Herzfeld.

1926

The latter was his thesis advisor when he obtained his doctorate in 1926; Herzfeld taught courses in theoretical physics and one in physical chemistry, and in Sommerfeld's absence often took over his classes.

From 1926 to 1927, he was a Rockefeller Foundation Fellow for postgraduate research with Niels Bohr at the Institute for Theoretical Physics at the University of Copenhagen and with Erwin Schrödinger at the University of Zurich.

He then became an assistant to Max Born at the Institute for Theoretical Physics at the University of Göttingen.

Also, in early 1926, Erwin Schrödinger, at the University of Zurich, began to publish his quintet of papers which launched the wave mechanics formulation of quantum mechanics and showed that the wave mechanics and matrix mechanics formulations were equivalent.

These papers immediately put the personnel at the leading theoretical physics institutes onto applying these new tools to understanding atomic and molecular structure.

It was in this environment that Heitler went on his Rockefeller Foundations Fellowship, leaving LMU and within a period of two years going to do research and study with the leading figures of the day in theoretical physics, Bohr's personnel in Copenhagen, Schrödinger in Zurich, and Born in Göttingen.

In Zurich, with Fritz London, Heitler applied the new quantum mechanics to deal with the saturable, nondynamic forces of attraction and repulsion, i.e., exchange forces, of the hydrogen molecule.

Their valence bond treatment of this problem, was a landmark in that it brought chemistry under quantum mechanics.

Furthermore, their work greatly influenced chemistry through Linus Pauling, who had just received his doctorate and on a Guggenheim Fellowship visited Heitler and London in Zurich.

Pauling spent much of his career studying the nature of the chemical bond.

The application of quantum mechanics to chemistry would be a prominent theme in Heitler's career.

1929

Heitler completed his Habilitation, under Born, in 1929, and then remained as a Privatdozent until 1933.

In that year, he was let go by the university because he was Jewish.

At the time Heitler received his doctorate, three Institutes for Theoretical Physics formed a consortium which worked on the key problems of the day, such as atomic and molecular structure, and exchanged both scientific information and personnel in their scientific quests.

These institutes were located at the LMU, under Arnold Sommerfeld, the University of Göttingen, under Max Born, and the University of Copenhagen, under Niels Bohr.

Furthermore, Werner Heisenberg and Born had just recently published their trilogy of papers which launched the matrix mechanics formulation of quantum mechanics.

1933

While Heitler was at Göttingen, Adolf Hitler came to power in 1933.

With the rising prominence of anti-Semitism under Hitler, Born took it upon himself to take the younger Jewish generation under his wing.

In doing so, Born arranged for Heitler to get a position that year as a Research Fellow at the University of Bristol, with Nevill Francis Mott.

At Bristol, Heitler was a Research Fellow of the Academic Assistance Council, in the H. H. Wills Physics Laboratory.

At Bristol, among other things, he worked on quantum field theory and quantum electrodynamics on his own, as well as in collaboration with other scientific refugees from Hitler, such as Hans Bethe and Herbert Fröhlich, who also left Germany in 1933.

With Bethe, he published a paper on pair production of gamma rays in the Coulomb field of an atomic nucleus, in which they developed the Bethe-Heitler formula for Bremsstrahlung.

1936

In 1936, Heitler published his major work on quantum electrodynamics, The Quantum Theory of Radiation, which marked the direction for future developments in quantum theory.

The book appeared in many editions and printings and has been translated into Russian.

Heitler also contributed to the understanding of cosmic rays,

as well as predicted the existence of the electrically neutral pi meson.

1937

While developing the theory of cosmic ray showers in 1937, he became aware of the latest experimental work in the field: the observation of cosmic ray interactions in Nuclear emulsion by Austrian physicists Marietta Blau and Hertha Wambacher.

He mentioned this to Bristol colleague Cecil Powell, saying that the method appeared so straightforward that 'even a theoretician might be able also to do it'.

This intrigued Powell, and he convinced theoretician Heitler to travel to Switzerland with a batch of llford emulsions and expose them on the Jungfraujoch at 3500m.

1939

In a letter to 'Nature' in August 1939, Heitler and Powell were able to confirm the observations of Blau and Wambacher.

1940

After the fall of France in 1940, Heitler was briefly interned on the Isle of Man for several months.

He has been described as the "unsung hero of DIAS in the 1940s".

At Dublin, Heitler's work with H. W. Peng on radiation damping theory and the meson scattering process resulted in the Heitler-Peng integral equation.

During his stay in Dublin he lived at 21 Seapark Road, Clontarf, down the road from Erwin Schrödinger.

1941

Heitler remained at Bristol eight years, until 1941, when he became a professor at the Dublin Institute for Advanced Studies, which was arranged there by Erwin Schrödinger, Director of the School for Theoretical Physics.

1942

During the 1942–1943 academic year, Heitler gave a course on elementary wave mechanics, during which W. S. E. Hickson took notes and prepared a finished copy.

1950

Thus Heitler had some influence in setting Cecil Powell on the first step of his path to the 1950 Nobel Prize in Physics, "for his development of the photographic method of studying nuclear processes and his discoveries regarding mesons made with this method".