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Hiroshi Enatsu

Hiroshi Enatsu is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Hiroshi Enatsu rather than just read about it. In short: Hiroshi Enatsu (12 September 1922 – 4 August 2019) was a Japanese theoretical physicist who contributed to a relativistic Hamiltonian formalism in quantum field theory. Academic works Enatsu has found that the commutation relation [ ψ ( x , τ ) , ψ ∗ ( x ′ , τ ) ] = δ ( x − x ′ ) {\displaystyle [\psi (x,\tau ),\psi ^{*}(x',\tau )]=\delta (x-x')} in a relativistic Hamiltonian formalism is equivalent to that in the co…

Key takeaways

  • Hiroshi Enatsu belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Hiroshi Enatsu to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Hiroshi Enatsu from memory before moving on to harder problems.

Reference excerpt

Hiroshi Enatsu (12 September 1922 – 4 August 2019) was a Japanese theoretical physicist who contributed to a relativistic Hamiltonian formalism in quantum field theory.

Academic works Enatsu has found that the commutation relation

[ ψ ( x , τ ) , ψ ∗ ( x ′ , τ ) ] = δ ( x − x ′ ) {\displaystyle [\psi (x,\tau ),\psi ^{*}(x',\tau )]=\delta (x-x')}

in a relativistic Hamiltonian formalism is equivalent to that in the conventional non-relativistic Hamiltonian formalism of quantum field theory, where [ ψ , ϕ ] = ψ ϕ − ϕ ψ {\displaystyle [\psi ,\phi ]=\psi \phi -\phi \psi } is the commutator,

x {\displaystyle x} is space-time coordinates,

τ {\displaystyle \tau } is proper time,

ψ ∗ {\displaystyle \psi ^{*}} is Hermitian adjoint of ψ {\displaystyle \psi } , and δ ( x ) {\displaystyle \delta (x)} is the Dirac delta function, with the aid of the relation

ϵ ( x − x ′ ) ϵ ( τ − τ ′ ) = 1 {\displaystyle \epsilon (x-x')\epsilon (\tau -\tau ')=1} . Here, a step function ϵ ( x ) {\displaystyle \epsilon (x)} follows ϵ ( x ) = 1 {\displaystyle \epsilon (x)=1} for 0 < x {\displaystyle 0<x} , and ϵ ( x ) = − 1 {\displaystyle \epsilon (x)=-1} for x < 0 {\displaystyle x<0} .

Biography

Early stage Enatsu was born on 12 September 1922 in Miyakonojō as a son of Eizo and Fumi (Kuroiwa) Enatsu. Miyakonojō is a town within the territory of the former Satsuma Domain, and it was rather natural for Enatsu to receive an education in Kagoshima. So, he spent in Kagoshima for secondary education and junior college.

Encounter with Hideki Yukawa In the last year of junior college, Hideki Yukawa made a lecture on meson theory at Kagoshima. After listening to the lecture, Enatsu became interested in Yukawa and meson theory, so he decided to study under Yukawa. He studied on meson theory under Yukawa in undergraduate course. He received Bachelor of Science from Kyoto Imperial University in 1944. He received Doctor of Science. from Kyoto Imperial University in 1953 under Yukawa. Enatsu was an assistant under Yukawa at Kyoto University from 1946 to 1957. Enatsu was a research assistant at Columbia University in New York City from 1952 to 1953.

Encounter with Niels Bohr Enatsu was a visiting member of the Institute for Theoretical Physics in Copenhagen from 1955 to 1956. During his stay in Copenhagen, he could ask some questions to Bohr almost every week. It was a special treatment.

Professor at Ritsumeikan University In 1957, Enatsu was an assistant professor and inaugurated a professor at Ritsumeikan University in Kyoto. From 1971 to 1972, he was also the dean of faculty of science and engineering at Ritsumeikan University. In 1988, he retired from a professor at Ritsumeikan University in Kyoto, and has been a professor emeritus. In 1997. he received the 3rd class of the Order of the Sacred Treasure. Enatsu died on 4 August 2019 in Kyoto

Notes

Research articles On the Photodisintegration of the Deuteron (Pseudoscalar Meson Theory.), December 1949 On the Nuclear Forces, February 1950 On the Interaction of Mesons and Nucleons, September 1950 On the Mass of Cohesive Meson and the Mass Difference Of Nucleon, April 1951 On the Mass of Cohesive Meson and the Mass Difference of Nucleons, II, June 1951 On the Mass Difference of Nucleons and the Cohesive Mesons, October 1951 On the Self-energies of Mesons, October 1951 On the Self-Energies of Nucleons, October 1951 Self-Energies of Nucleons and the Mass Spectra of Heavy Particles, February 1952 Mass Spectrum of Elementary Particles I: Eigenvalue Problem in Space-time, February 1954 Mass Spectrum of Elementary Particles, II, September 1954 Theory of Unstable Heavy Particles, July 1954 Relativistic quantum mechanics and mass-quantization, 1956 Relativistic Hamiltonian Formalism in Quantum Field Theory and Micro-Noncausality, August 1963 Covariant Hamiltonian Formalism for Particles of any Spin and Nonzero Mass, 1968 Micro-noncausal theory of the hydrogen atom 1971 Covariant Hamiltonian formalism for quantized fields and the hydrogen mass levels, 1975 On the hyperfine structure splittings of hydrogen, 1975 Proton-proton scattering problem in a covariant Hamiltonian formalism, 1976 Four-dimensional tensor forces and electric quadrupole moments in the bound-states of the deuteron, 1976 Micrononcausal euclidean wave functions for hadrons, February 1978 Hyperfine structure splittings of the hydrogen atom in a covariant Hamiltonian formalism, 1983 Bethe-Salpeter type equations for a covariant Hamiltonian formalism in quantum field theory, 1984 Quantization of masses of elementary particles with micrononcausal structures, October 1986 Quantization of masses of elementary particles with micrononcausal structures 1987 Quantization of the mass of the W-boson in the Weinberg-Salam theory, 1988

… excerpt ends here. Continue reading the full article.

Worked examples

Example 1 — a first encounter with Hiroshi Enatsu

Start with the simplest possible case. Write down what Hiroshi Enatsu claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Hiroshi Enatsu before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Hiroshi Enatsu ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Hiroshi Enatsu

In research
Hiroshi Enatsu appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Hiroshi Enatsu in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Hiroshi Enatsu is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1922 births, 2019 deaths, Academic staff of Kyoto University, so understanding it makes those chapters shorter.
In everyday life
Look for Hiroshi Enatsu outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study Hiroshi Enatsu in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Hiroshi Enatsu means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Hiroshi Enatsu out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Hiroshi Enatsu in simple terms?

Hiroshi Enatsu (12 September 1922 – 4 August 2019) was a Japanese theoretical physicist who contributed to a relativistic Hamiltonian formalism in quantum field theory. Academic works Enatsu has found that the commutation relation [ ψ ( x , τ ) , ψ ∗ ( x ′ , τ ) ] = δ ( x − x ′ ) {\displaystyle [\p…

Why does Hiroshi Enatsu matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Hiroshi Enatsu?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Hiroshi Enatsu.

Tags

  • 1922 births
  • 2019 deaths
  • Academic staff of Kyoto University
  • Academic staff of Ritsumeikan University
  • Japanese expatriates in the United States
  • Japanese physicists
  • Kagoshima University alumni
  • Kyoto University alumni
  • People from Miyakonojō
  • Scientists from Miyazaki Prefecture

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