KnowraGeorge GamowLinked fromLinked fromThe 19 pages that link to George Gamow, each with the reason it gives.All 19Related 17Narrower topic 1Compared with 1Cosmic microwave backgroundRelated: His work helped establish the expectation of a cooled cosmic radiation background.Edward TellerRelated: Gamow recruited Teller to the United States and became a close scientific collaborator.Stanisław UlamRelated: Gamow encouraged Ulam’s early interest in applying probability and mathematics to physical problems.Ralph AlpherRelated: Gamow recruited Alpher and helped shape the research program they pursued together.Freeman DysonRelated: Gamow’s group at George Washington University hosted Dyson during his formative American years.Harold JeffreysRelated: Gamow publicly disputed Jeffreys’s resistance to continental drift in a 1940s scientific exchange.Niels Bohr InstituteRelated: His time in Copenhagen connected the institute to early research on nuclear structure.Robert HermanRelated: Gamow supervised and promoted the work by Alpher and Herman on the early universe.Flatness problemRelated: The hot Big Bang framework sharpened the puzzle of the universe’s initial density.Alpher–Bethe–Gamow paperRelated: He proposed the cosmological setting and supervised Alpher’s research.Geiger–Nuttall lawRelated: His tunneling model explained why the empirical energy–lifetime relation holds.George SmootRelated: Gamow’s prediction made the cosmic microwave background a test of the universe’s hot early state.Semi-empirical mass formulaRelated: His early nuclear liquid-drop work helped prepare the conceptual ground for the formula.Arno Allan PenziasRelated: Gamow helped develop the theoretical tradition predicting a hot early universe and its residual radiation.Edwin E. SalpeterRelated: Gamow helped establish the nuclear astrophysics tradition in which Salpeter worked.Jim PeeblesRelated: Gamow’s early-universe program preceded and influenced the problems Peebles pursued.Quantum tunnellingRelated: His account connected tunnelling to radioactive decay and nuclear structure.
KnowraGeorge GamowLinked fromLinked fromThe 19 pages that link to George Gamow, each with the reason it gives.All 19Related 17Narrower topic 1Compared with 1Cosmic microwave backgroundRelated: His work helped establish the expectation of a cooled cosmic radiation background.Edward TellerRelated: Gamow recruited Teller to the United States and became a close scientific collaborator.Stanisław UlamRelated: Gamow encouraged Ulam’s early interest in applying probability and mathematics to physical problems.Ralph AlpherRelated: Gamow recruited Alpher and helped shape the research program they pursued together.Freeman DysonRelated: Gamow’s group at George Washington University hosted Dyson during his formative American years.Harold JeffreysRelated: Gamow publicly disputed Jeffreys’s resistance to continental drift in a 1940s scientific exchange.Niels Bohr InstituteRelated: His time in Copenhagen connected the institute to early research on nuclear structure.Robert HermanRelated: Gamow supervised and promoted the work by Alpher and Herman on the early universe.Flatness problemRelated: The hot Big Bang framework sharpened the puzzle of the universe’s initial density.Alpher–Bethe–Gamow paperRelated: He proposed the cosmological setting and supervised Alpher’s research.Geiger–Nuttall lawRelated: His tunneling model explained why the empirical energy–lifetime relation holds.George SmootRelated: Gamow’s prediction made the cosmic microwave background a test of the universe’s hot early state.Semi-empirical mass formulaRelated: His early nuclear liquid-drop work helped prepare the conceptual ground for the formula.Arno Allan PenziasRelated: Gamow helped develop the theoretical tradition predicting a hot early universe and its residual radiation.Edwin E. SalpeterRelated: Gamow helped establish the nuclear astrophysics tradition in which Salpeter worked.Jim PeeblesRelated: Gamow’s early-universe program preceded and influenced the problems Peebles pursued.Quantum tunnellingRelated: His account connected tunnelling to radioactive decay and nuclear structure.