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James Hartle

James Hartle is a physics 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 James Hartle rather than just read about it. In short: James Burkett Hartle (August 17, 1939 – May 17, 2023) was an American theoretical physicist known for his work in general relativity, astrophysics, and interpreting quantum mechanics. He was one of the pioneers of quantum cosmology.

James Hartle — main illustration
James Hartle — illustration

Key takeaways

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

Reference excerpt

James Burkett Hartle (August 17, 1939 – May 17, 2023) was an American theoretical physicist known for his work in general relativity, astrophysics, and interpreting quantum mechanics. He was one of the pioneers of quantum cosmology. He joined the faculty of the University of California, Santa Barbara in 1966, and was a member of the external faculty of the Santa Fe Institute.

Early life and education Hartle was born on August 17, 1939, in Baltimore, Maryland, to Anna Elizabeth Burkett and Charles James Hartle, who worked for IBM. His father's job required the family to relocated multiple times while Hartle was growing up. He attended public schools in Ohio and Connecticut, as well as the Gilman School in Baltimore. There, Hartle became interested in physics thanks to his teacher, Bill Potter. He began as an engineering major upon matriculation at Princeton University, but switched to physics due to the influence of John Archibald Wheeler. Hartle earned his AB at Princeton in 1960 and his Ph.D. in particle physics under Murray Gell-Mann in 1964 at the California Institute of Technology (Caltech). Afterwards, he briefly taught at Princeton before accepting a position at the University of California, Santa Barbara.

Work With Dieter Brill in 1964, he discovered the Brill–Hartle geon, an approximate solution realizing Wheeler's suggestion of a hypothetical phenomenon in which a gravitational wave packet is confined to a compact region of spacetime by the gravitational attraction of its own field energy. Hartle then turned his attention towards astrophysics. Starting in 1967, Hartle worked with Kip Thorne on the physics of rotating compact objects, such as neutron stars, including the influence of the coupling of their multipole moments to the spacetime curvature of nearby objects, as described by general relativity. They discovered the Hartle–Thorne metric, an approximate solution which describes the exterior of a slowly and rigidly rotating, stationary and axially symmetric body. Funded by an award from the Sloan Foundation, Hartle spent a year at the Institute for Theoretical Astronomy at the University of Cambridge, where he met Stephen Hawking, with whom he became a long-time collaborator. In 1976, Hartle and Hawking utilized path integrals to show that black holes must emit radiation (later dubbed Hawking radiation), the same conclusion Hawking himself had reached two years earlier. Their work on the thermodynamics of black holes led to the development of the Euclidean approach to quantum gravity. In 1983, Hartle and Hawking proposed the no-boundary wave function for the Universe. Their aim was to explain the initial conditions of the Big Bang model of cosmology. Hartle considered this to be his greatest contribution to the subject. In later decades, Hartle collaborated with Gell-Mann and others to develop an alternative to the standard Copenhagen interpretation of quantum mechanics, more general and appropriate to quantum cosmology, based on the notion of consistent histories. Hartle published his textbook on general relativity, Gravity: An Introduction to Einstein's General Relativity, in 2003. Reviewers have praised the book for its lucid explanations and focus on physical insight rather than mathematical details. Only requires familiarity with calculus and differential equations, making the book suitable for junior or senior undergraduates in physics. He explained his vision for teaching general relativity to undergraduates in a 2006 article. Hartle was a founder of the Kavli Institute for Theoretical Physics at UC Santa Barbara and served as its director from 1995 to 1997. He was elected to the American Philosophical Society in 2016. He was also a Fellow of the American Physical Society (APS), a Guggenheim Fellow, and was elected to the National Academy of Sciences. He received the 2009 Einstein Prize from the APS for his "broad range of fundamental contributions to relativistic stars, quantum fields in curved spacetime, and especially quantum cosmology."

Personal life Hartle married Mary Jo Wheeler, a niece of John Archibald Wheeler, in 1984. Hartle was diagnosed with Alzheimer's disease in 2022. He died in Zurich, Switzerland on May 17, 2023, at the age of 83.

References

External links James Hartle homepage Archived July 25, 2011, at the Wayback Machine Faculty profile "The Future of Gravity" – April 2000 online lecture (RealAudio plus slides) "Spacetime Quantum Mechanics" online RealAudio lecture "The Classical Behavior of Quantum Universes" online RealAudio lecture James Hartle at the Mathematics Genealogy Project "The Quantum Universe: Essays on Quantum Mechanics, Quantum Cosmology, and Physics in General" book (World Scientific, 2021)

Illustrations

James Hartle illustration

Worked examples

Example 1 — a first encounter with James Hartle

Start with the simplest possible case. Write down what James Hartle claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In physics, 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 James Hartle 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 James Hartle 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 James Hartle

In research
James Hartle appears in physics 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 James Hartle 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
James Hartle is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1939 births, 2023 deaths, 20th-century American physicists, so understanding it makes those chapters shorter.
In everyday life
Look for James Hartle 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 James Hartle in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what James Hartle 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 James Hartle out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is James Hartle in simple terms?

James Burkett Hartle (August 17, 1939 – May 17, 2023) was an American theoretical physicist known for his work in general relativity, astrophysics, and interpreting quantum mechanics. He was one of the pioneers of quantum cosmology.

Why does James Hartle matter?

Because it connects several physics 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 James Hartle?

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 James Hartle.

Tags

  • 1939 births
  • 2023 deaths
  • 20th-century American physicists
  • 21st-century American physicists
  • American male non-fiction writers
  • American relativity theorists
  • American textbook writers
  • California Institute of Technology alumni
  • Fellows of the American Academy of Arts and Sciences
  • Fellows of the American Physical Society
  • Members of the American Philosophical Society
  • Members of the United States National Academy of Sciences

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