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{{short description|American theoretical physicist and cosmologist}}
{{Use mdy dates|date=January 2021}}
{{Infobox scientist {{Infobox scientist
| name = Alan Harvey Guth | name = Alan Guth
| image = AlanGuthCambridge.jpg | image = AlanGuthCambridge.jpg
| caption = Alan Guth at ], 2007 | caption = Guth at ], 2007
| birth_name = Alan Harvey Guth
| birth_date = {{Birth date and age|1947|2|27}} | birth_date = {{Birth date and age|1947|2|27}}
| birth_place = ] | birth_place = ], U.S.
| death_date =
| death_place = | death_date =
| death_place =
| residence = ]
| nationality = ] | nationality = American
| field = ], ], ] | field = ], ], ]
| work_institution =]<br>]<br>]<br>]<br>] | work_institution = ]<br>]<br>]<br>]<br>]
| alma_mater = ] | alma_mater = ] (], ], ])
| doctoral_advisor = ] | doctoral_advisor = ]
| doctoral_students = | doctoral_students =
| known_for = ]<br>]<br>]
| influences = ]
| prizes = ] (1991)<br>
| influenced =
] for Physics of the ]<br>
| known_for = ]
] (2009)<br>
| societies = ]
] of the International Center for Theoretical Physics in Trieste<br>
]
] (2004)<br>
| prizes = MIT School of Science Prize for Undergraduate Teaching,
] (2012)<br>
Oscar Klein Medal (1991),
] (2014)
The Franklin Medal for Physics of the ],
| spouse = {{marriage|Susan Tisch|1971}}
] of ] (2009),
| children = 2, including ]
Dirac Prize of the International Center for Theoretical Physics in Trieste,
| website =
Cosmology Prize of the Peter Gruber Foundation (2004),
| footnotes =
] (2012).
] (2014).
| spouse =
| children =
| website =
| footnotes =
}} }}
{{Cosmology|scientists}}


'''Alan Harvey Guth''' ({{IPAc-en|g|uː|θ}}; born February 27, 1947) is an American ] and ] who is the ] Professor of Physics at the ]. Along with ] and ], he won the 2014 ] "for pioneering the theory of cosmic inflation."<ref name="KavliPrize">{{cite web |title=2014 Astrophysics Citation |url=http://www.kavlifoundation.org/2014-astrophysics-citation |url-status=dead |archive-url=https://web.archive.org/web/20140714114045/http://www.kavlifoundation.org/2014-astrophysics-citation |archive-date=July 14, 2014 |access-date=July 27, 2014 |website=The Kavli Foundation }}</ref> Guth's research focuses on ] theory and how particle theory is applicable to the early ].
'''Alan Harvey Guth''' (born February 27, 1947) is an ] ] and ]. Guth has researched ] theory (and how particle theory is applicable to the early ]). He is currently serving as ] Professor of Physics at the ]. According to some sources, Guth is the originator of the ];<ref></ref><ref></ref> however, according to other sources, the originator was ].<ref name=LindeSciAm/><ref name="JETP-19791205">{{cite journal |last=Starobinskii |first=A.A. |title=Spectrum of relict gravitational radiation and the early state of the universe |url=http://www.jetpletters.ac.ru/ps/1370/article_20738.shtml |date=5 December 1979 |journal=] |volume=30 |issue=11 |page=682 |format=http://www.jetpletters.ac.ru/ps/1370/article_20738.pdf |accessdate=14 June 2014 }}</ref> <!-- According to some sources, Guth is the originator of the ];<ref></ref><ref></ref> however, according to other sources, the originator was ].<ref name=LindeSciAm> by Andrei Linde, Scientific American, Volume 9, Issue 1 (1998) 98–104.</ref><ref name="JETP-19791205">{{cite journal |last=Starobinskii |first=A.A. |title=Spectrum of relict gravitational radiation and the early state of the universe |url=http://www.jetpletters.ac.ru/ps/1370/article_20738.shtml |date=December 5, 1979 |journal=] |volume=30 |issue=11 |page=682 |format=http://www.jetpletters.ac.ru/ps/1370/article_20738.pdf |access-date=June 14, 2014}}</ref> -->


He graduated from MIT in 1968 in physics and stayed to receive a master's and a doctorate, also in physics. He graduated from MIT in 1968 in physics and stayed to receive a master's and a doctorate, also in physics.


As a junior particle physicist, Guth developed the idea of ] in 1979 at ] and gave his first seminar on the subject in January 1980.<ref>{{citation|last1=Guth|first1=Alan H.|title=The Inflationary Universe|publisher=Perseus Books|location= Reading, Massachusetts|year=1997|isbn=0-201-14942-7}}</ref><ref name="SLAC">] seminar, "10-35 seconds after the Big Bang", 23 January 1980. see Guth (1997), pg 186</ref> Moving on to ] Guth formally proposed the idea of cosmic inflation in 1981, the idea that the nascent universe passed through a phase of exponential expansion that was driven by a positive ] density (negative vacuum pressure). The results of the ] mission in 2006 made the case for cosmic inflation very compelling. Measurements by the ] telescope give support to the idea of cosmic inflation, preliminary confirmation of which was given on March 17, 2014, with the findings of the B-mode polarization signature.<ref name=bicep2-nytimes>{{cite web|last=Overbye|first=Dennis|title=Space Ripples Reveal Big Bang’s Smoking Gun|url=http://nyti.ms/1ebT9LS|publisher=New York Times|accessdate=19 March 2014}}</ref><ref name="NYT-20140324">{{cite news |last=Overbye |first=Dennis |authorlink=Dennis Overbye |title=Ripples From the Big Bang |url=http://www.nytimes.com/2014/03/25/science/space/ripples-from-the-big-bang.html |date=24 March 2014 |work=] |accessdate=24 March 2014 }}</ref><ref name=bicep2-arxiv>{{cite web|last=BICEP2 Collaboration|title=BICEP2 I: Detection Of B-mode Polarization at Degree Angular Scales|url=http://arxiv.org/abs/1403.3985|publisher=arXiv.org|accessdate=19 March 2014}}</ref> However, on 19 June 2014, lowered confidence in confirming the ] findings was reported.<ref name="NYT-20140619">{{cite news |last=Overbye |first=Dennis |authorlink=Dennis Overbye |title=Astronomers Hedge on Big Bang Detection Claim |url=http://www.nytimes.com/2014/06/20/science/space/scientists-debate-gravity-wave-detection-claim.html |date=19 June 2014 |work=] |accessdate=20 June 2014 }}</ref><ref name="BBC-20140619">{{cite news |last=Amos |first=Jonathan |title=Cosmic inflation: Confidence lowered for Big Bang signal |url=http://www.bbc.com/news/science-environment-27935479 |date=19 June 2014 |work=] |accessdate=20 June 2014 }}</ref><ref name="PRL-20140619">{{cite journal |author=Ade, P.A.R. et al (BICEP2 Collaboration) |title=Detection of B-Mode Polarization at Degree Angular Scales by BICEP2 |url=http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.112.241101 |date=19 June 2014 |journal=] |volume=112 |page=241101 |doi=10.1103/PhysRevLett.112.241101 |format=|accessdate=20 June 2014 |arxiv = 1403.3985 |bibcode = 2014PhRvL.112x1101A }}</ref> As a junior particle physicist, Guth developed the idea of ] in 1979 at ] and gave his first seminar on the subject in January 1980.<ref>{{citation |last1=Guth |first1=Alan H. |title=] |publisher=Perseus Books |location=Reading, Massachusetts |date=1997 |isbn=0-201-14942-7}}</ref><ref name="SLAC">] seminar, "10-35 seconds after the Big Bang", January 23, 1980. see Guth (1997), pg 186.</ref> Moving on to the ] at ], Guth formally proposed the idea of cosmic inflation in 1981, the idea that the nascent universe passed through a phase of exponential expansion that was driven by a positive ] density (negative vacuum pressure). The results of the ] mission in 2006 made the case for cosmic inflation very compelling.


==Early life== ==Early life and education==
Guth was born to a ] family<ref>{{Cite web |url=https://news.nationalgeographic.com/news/innovators/2014/06/140630-alan-guth-profile-inflation-cosmology-science/ |archive-url=https://web.archive.org/web/20140702172441/http://news.nationalgeographic.com/news/innovators/2014/06/140630-alan-guth-profile-inflation-cosmology-science/ |url-status=dead |archive-date=July 2, 2014 |title=Alan Guth: Waiting for the Big Bang }}</ref> in ] in 1947 and grew up across the ] in ], where he attended the local public schools.<ref>, ]. Accessed January 23, 2018. "Professor Alan Guth was born in New Brunswick, New Jersey, in 1947. He grew up and attended the public schools in Highland Park, NJ, but skipped his senior year of high school to begin studies at the Massachusetts Institute of Technology."</ref> After his junior year at ],<ref name=":0">{{Cite news |date=1 Feb 1971 |title=Susan Tisch, Alan H Guth Plan to Wed |pages=7 |work=] |url=https://www.newspapers.com/image/316046041 |access-date=26 May 2023}}</ref> he left school and enrolled in a five-year program at the ] where he could get his ] and ] after two more years.<ref>, p. 219. ], 1988. Accessed January 23, 2018. "At the end of his junior year he left Highland Park (New Jersey) High School to enter the Massachusetts Institute of Technology, where his extracurricular activities included, as they had in high school, debating, track, and the mathematics club."</ref> Guth obtained a bachelor's and master's degree in 1969 and a doctorate in 1972. In 1971, he married Susan Tisch, his high school sweetheart.<ref name=":0" /> They have two children: ] (born 1977) and Jennifer (born 1983).<ref name="Cosmos2015">{{Cite web |url=https://cosmosmagazine.com/space/physicist-who-inflated-universe |title=The physicist who inflated the Universe |last=da Silva |first=Wilson |work=Cosmos |quote=When people said that gravitational waves would be the smoking gun for inflation, my response was that I thought the room was pretty filled with smoke already. |date=March 2, 2015 |access-date=February 20, 2020}}</ref>
Alan Guth was born on February 27, 1947 in ]. After his junior year at ], he enrolled in a five-year program where he could get his ]’s and ]’s after two more years. Guth obtained a bachelor’s and master’s degree in 1969 and a doctorate in 1972. In 1971, he married Susan Tisch, his high school sweetheart. They have two children: ] (born 1977) and Jennifer (born 1983).


Guth was at ] 1971 to 1974, ] 1974 to 1977, ] 1977 to 1979, and the ] (SLAC) 1979 to 1980. Like many other young physicists of the ] era, he had a hard time finding a permanent job, because there were far fewer assistant professorships than there were young scientists seeking such jobs, a phenomenon that has been referred to as the “generation of lost scholars.<ref>(1978) Carnegie Council on Policy Studies in Higher Education, “Preserving a Lost Generation: Policies to Assure a Steady Flow of Young Scholars Until the Year 2000”; http://pages.stern.nyu.edu/~rradner/publishedpapers/42PreservingLostGeneration.pdf Downloaded 2011-07-09</ref> Guth was at ] 1971 to 1974, ] 1974 to 1977, ] 1977 to 1979, and the ] (SLAC) 1979 to 1980. Like many other young physicists of the ] era, he had a hard time finding a permanent job, because there were far fewer assistant professorships than there were young scientists seeking such jobs, a phenomenon that has been referred to as the "generation of lost scholars."<ref>{{cite web |date=1978 |publisher=Carnegie Council on Policy Studies in Higher Education |title=Preserving a Lost Generation: Policies to Assure a Steady Flow of Young Scholars Until the Year 2000 |url=http://pages.stern.nyu.edu/~rradner/publishedpapers/42PreservingLostGeneration.pdf |access-date=July 9, 2011 }}</ref>


At the start of his career, Guth studied ], not ]. Guth's earliest work at Princeton was in the study of ]s, the elementary particles that make up protons and neutrons. At Columbia, Guth studied ] (GUTs), focusing on the ]s generated by ]. Most GUTs predict the generation of ] during spontaneous symmetry breaking, but none had ever been detected - the ]. At the start of his career, Guth studied ], not ]. Guth's earliest work at Princeton was in the study of ]s, the elementary particles that make up protons and neutrons. At Columbia, Guth studied ] (GUTs), focusing on the ] generated by ]. Most GUTs predict the generation of ] during spontaneous symmetry breaking, but none had ever been detected—the ].


==Inflationary theory== ==Career==
===Inflationary theory===
{{BLP sources section|date=July 2014}}
Guth's first step to developing his theory of inflation occurred at Cornell in 1978, when he attended a lecture by ] about the ] of the universe.<ref>]. </ref> Dicke explained how the flatness problem showed that something significant was missing from the Big Bang theory at the time. The fate of the universe depended on its density. If the density of the universe was large enough, it would collapse into a ], and if the actual density of the matter in the cosmos was lower than the critical density, the universe would increasingly get much bigger. Guth's first step to developing his theory of inflation occurred at Cornell in 1978, when he attended a lecture by ] about the ] of the universe.<ref>{{cite book |author-link=Timothy Ferris |author=Ferris, Timothy |url=https://books.google.com/books?id=k0vCHGD5Y00C&pg=PA356 |via=Google Books |title=Coming of Age in the Milky Way |date=July 6, 2010 |page=356|publisher=Harper Collins |isbn=9780062006547 }}</ref> Dicke explained how the flatness problem showed that something significant was missing from the ] theory at the time. The fate of the universe depended on its density. If the density of the universe was large enough, it would collapse into a ], and if the actual density of the matter in the cosmos was lower than the critical density, the universe would increasingly get much bigger.


The next part in Guth's path came when he heard a lecture by ] in early 1979. Weinberg talked in two lectures about the ] (GUT) that had been developed since 1974, and how it could explain the huge amount of matter in the universe compared to the amount of antimatter. The GUT explained all the fundamental forces known in science except for gravity. It established that in very hot conditions, such as those after the Big Bang, electromagnetism, the strong nuclear force, and the weak nuclear force were united to form one force. Weinberg also was the one who emphasized the idea that the universe goes through phase transitions, similar to the phases of matter, when going from high energy to low energy. Weinberg’s discussion of why matter is so dominant over anti-matter showed Guth how precise calculations about particles could be obtained by studying the first few seconds of the universe. The next part in Guth's path came when he heard a lecture by ] in early 1979.<ref name="Swidey-2014">{{cite web |last1=Swidey |first1=Neil |title=Alan Guth: What made the Big Bang bang? |url=https://www.bostonglobe.com/magazine/2014/05/02/alan-guth-what-made-big-bang-bang/RmI4s9yCI56jKF6ddMiF4L/story.html |publisher=The Boston Globe |access-date=July 14, 2015 |date=May 2, 2014 |archive-date=February 27, 2019 |archive-url=https://web.archive.org/web/20190227040746/https://www.bostonglobe.com/magazine/2014/05/02/alan-guth-what-made-big-bang-bang/RmI4s9yCI56jKF6ddMiF4L/story.html |url-status=dead }}</ref> Weinberg talked in two lectures about the ] (GUT) that had been developed since 1974, and how it could explain the huge amount of matter in the universe compared to the amount of antimatter. The GUT explained all the fundamental forces known in science except for gravity. It established that in very hot conditions, such as those after the Big Bang, electromagnetism, the strong nuclear force, and the weak nuclear force were united to form one force. Weinberg also was the one who emphasized the idea that the universe goes through ]s, similar to the phases of matter, when going from high energy to low energy. Weinberg's discussion of why matter is so dominant over anti-matter showed Guth how precise calculations about particles could be obtained by studying the first few seconds of the universe.


Guth decided to solve this problem by suggesting a ] during a delayed phase transition. This seemed very promising for solving the ] problem. By the time they came up with that, Guth had gone to the Stanford Linear Accelerator Center for a year, but Guth had been talking to ] back and forth. Tye suggested that they check that the expansion of the universe would not be affected by the supercooling. In the supercooled state, a ] is produced. The false vacuum is a vacuum in the sense that it is state of the lowest possible density of energy; it is false in the sense that it is not a permanent state of being. False vacuums decay, and Guth was to find that the decay of the false vacuum at the beginning of the universe would produce amazing results, namely the exponential expansion of space. This solved the ], since the expansion dilutes the monopole density. Guth decided to solve this problem by suggesting a ] during a delayed phase transition. This seemed very promising for solving the ] problem. By the time Guth and his collaborator ] came up with that, Guth had gone to the ] (SLAC) for a year. Tye suggested that they check that the expansion of the universe would not be affected by the supercooling. The supercooled state is a ]: It is a ''vacuum'' in the sense that it is the state of the lowest possible density of energy; it is "false" since its state is not permanent. False vacuums decay, and Guth found that the decay of the false vacuum at the beginning of the universe would produce an exponential expansion of space. This solved the ], since the expansion proportionately reduces the monopole density.


Guth realized from his theory that the reason the universe appears to be flat was that it was fantastically big, just the same way the spherical Earth appears flat to those on its surface. The observable universe was actually only a very small part of the actual universe. Traditional Big Bang theory found values of ] near one to be puzzling, because any deviations from one would quickly become much, much larger. In inflation theory, no matter where omega starts, it would be driven towards equal to one, because the universe becomes so huge. In fact, a major prediction of inflationary theory is that omega will be found to be one. Guth realized from his theory that the reason the universe appears to be flat was that it had enlarged to such an overwhelming size in comparison to its original size. The perspective is analogous to the apparent flatness of the Earth, on a human scale, when seen from its surface. The ''observable'' universe was actually only a very small part of the ''actual'' universe. Traditional Big Bang theory found values of ] near&nbsp;1 to be puzzling, because any deviations from 1 would quickly become much, much larger. In inflation theory, no matter where omega starts, it would approach&nbsp;1 because of the scale of the universe's expansion. In fact, a major prediction of inflationary theory is that omega will be found to be precisely&nbsp;1.


Two weeks later, Guth heard colleagues discussing something called the ]. The microwave background radiation discovered by ] and ] appeared extremely ], with almost no variance. This seemed very paradoxical because, when the radiation was released about 300,000 years after the Big Bang, the observable universe had a diameter of 90 million ]s. There was no time for one end of the cosmos to communicate with the other end, because energy can not move faster than the speed of light. The paradox was resolved, as Guth soon realized, by the inflation theory. Since inflation started with a far smaller amount of matter than the Big Bang had presupposed, an amount so small that all parts would have been in touch with each other. The universe then inflated at billion times the speed of light so the homogeneity remained unbroken. The universe after inflation would have been very uniform even though the parts were not still in touch with each other. Two weeks later, Guth heard colleagues discussing something called the ]. The microwave background radiation discovered by ] and ] appeared extremely uniform, with almost no variance. This seemed very paradoxical because when the radiation was released about 300,000&nbsp;years after the Big Bang, the observable universe had a diameter of 90&nbsp;million ]s. There was no time for one end of the cosmos to communicate with the other end, because energy cannot move faster than the speed of light. The paradox was resolved, as Guth soon realized, by the inflation theory. Since inflation started with a far smaller amount of matter than the Big Bang had presupposed, an amount so small that all parts would have been in touch{{vague|date=August 2019}} with each other. The universe then inflated, at a rate corresponding to a billion times the speed of light, and the homogeneity remained unbroken. The universe after inflation would have been very uniform, even though its parts were no longer able to influence each other.


Guth first made public his ideas on inflation in a seminar at SLAC on January 23, 1980. In August, he submitted his paper, entitled "The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems" to the journal '']''.<ref name="Inflationary Universe">{{cite journal|author=A. H. Guth| title=The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems|url= http://www.slac.stanford.edu/pubs/slacpubs/2000/slac-pub-2576.html |journal=]|oclc=4433735058 | volume=D23|page=347|date= 1981-01-15|year=1981}}</ref> He ignored magnetic monopoles because they were based on assumptions of GUT, which was outside the scope of the speech. Guth first made public his ideas on inflation in a seminar at SLAC in January&nbsp;1980. He ignored magnetic monopoles because they were based on assumptions of GUT, which was outside the scope of the speech. In August&nbsp;1980, he submitted his paper, entitled "Inflationary universe: A possible solution to the horizon and flatness problems" to the journal '']''.<ref name="Inflationary Universe">{{cite journal |last1=Guth |first1=Alan H. |title=Inflationary universe: A possible solution to the horizon and flatness problems |journal=Physical Review D |year=1981 |volume=23 |issue=2 |pages=347–356 |doi=10.1103/PhysRevD.23.347 |bibcode=1981PhRvD..23..347G|doi-access=free }}</ref> In this paper Guth postulated that the inflation of the universe could be explained if the universe were supercooled 28&nbsp;orders of magnitude below the critical temperatures required for a phase change.


In December 1981, Guth read a paper from Moscow physicist ] saying that the whole universe is within just one bubble, so nothing is destroyed by wall collisions. This conclusion was made using a ] with an energy graph that was originally proposed by ] and ]. Guth discussed this with Linde, who had independently been working on bubble inflation, but without considering the flatness problem. Linde and Guth eventually exchanged papers on the subject. In December&nbsp;1981, Guth read a paper from Moscow physicist ] saying that the whole universe is within just one bubble, so nothing is destroyed by wall collisions. This conclusion was made using a ] with an energy graph that was originally proposed by ] and ]. Guth discussed this with Linde, who had independently been working on bubble inflation, but without considering the flatness problem. Linde and Guth eventually exchanged papers on the subject.


By 1983, Guth had published a paper describing how his supercooled universe scenario was not ideal, as the "triggering mechanism" to exit such a state would require "extreme fine tuning of parameters" and felt a more natural solution was required.<ref name=KavliPrize/><ref name=LindeSciAm>{{cite magazine |url=http://www.mukto-mona.com/science/physics/Inflation_lself_prod_inde.pdf |title=The self-reproducing inflationary universe |first=Andrei |last=Linde |magazine=Scientific American |volume=9 |issue=1 |year=1998 |pages=98–104}}</ref><ref>{{cite journal |last1=Guth |first1=Alan H. |last2=Weinberg |first2=Erick J. |title=Could the universe have recovered from a slow first-order phase transition? |journal=Nuclear Physics B |year=1983 |volume=212 |issue=2 |pages=321–364 |doi=10.1016/0550-3213(83)90307-3 |bibcode=1983NuPhB.212..321G}}</ref> However, this did not deter him from the belief that the universe expanded exponentially in a vacuum in its early lifetime.<ref>{{cite journal |last1=GUTH |first1=ALAN H. |title=The New Inflationary Universe |journal=Annals of the New York Academy of Sciences |year=1984 |volume=422 |issue=1 Eleventh Texa |pages=1–14 |doi=10.1111/j.1749-6632.1984.tb23336.x |bibcode=1984NYASA.422....1G|s2cid=117856496 }}</ref>
===Guth's recanting of inflation theory===
{{See also|Talk:Alan Guth#Guth's recanting of inflation theory|l1=talk discussion}}
According to ] in his , Guth has recanted his inflation theory, in a paper more than 100 pages long.<ref>, interview with Clive Cookson. The Financial Times, 11 April 2014.</ref>


==Current interests==
Linde has been noted for stating this before as well, like in his ] article in which he explicitly stated: "''After investigating his model for a year, Guth finally renounced it in a paper he co-authored with Erick J. Weinberg of Columbia University''".<ref name=LindeSciAm> by Andrei Linde, Scientific American, Volume 9, Issue 1 (1998) 98-104.</ref>
In the past, Guth has studied ], magnetic monopoles and ]s, ], and a number of other topics in theoretical physics. Much of Guth's current work includes extrapolating density fluctuations arising from various versions of inflation, to test against observations, and investigating inflation in "]" models.


He is the ] Professor of Physics at the Massachusetts Institute of Technology (MIT). He has written more than 60 technical papers related to the effects of inflation and its interactions with particle physics.
The Guth's ''Astrophysics Kavli prize'' citation states basically that Guth’s model was flawed as he himself recognized.<ref>, Kavli Foundation Website.</ref>


==Current life== ==Honors and awards==
In the past Guth has studied lattice gauge theory, magnetic monopoles and instantons, ], and a number of other topics in theoretical physics. Much of Guth's current work includes extrapolating density fluctuations arising from various versions of inflation, to test against observations, and investigating inflation in "]" models.


Guth is the ''] Professor of Physics'' at the ] (MIT). So far, he has written about 60 technical papers related to the effects of inflation and its interactions with particle physics. He has won many awards and medals, including the Medal of the International Center for Theoretical Physics, ], with ] and ] and the ] in 1996, and the ], awarded by the British ]. Guth has won many awards and medals, including the Medal of the International Center for Theoretical Physics, ], with ] and ] and the ] in 1996, and the ], awarded by the British ].


In July 2012, he was an inaugural awardee of the ], the creation of physicist and internet entrepreneur, ].<ref> {{webarchive|url=https://web.archive.org/web/20120803211628/https://breakthroughprize.org/News/15 |date=August 3, 2012 }}, FPP, accessed August 1, 2012.</ref><ref name="NYT_Breakthrough">{{Cite web |url=https://www.nytimes.com/2012/07/31/science/9-scientists-win-yuri-milners-fundamental-physics-prize.html |title=xx |last=Chang |first=Kenneth |work=NY Times |quote=The nine are recipients of the Fundamental Physics Prize, established by Yuri Milner, a Russian physics student who dropped out of graduate school in 1989 and later earned billions investing in Internet companies like Facebook and Groupon. |date=July 31, 2012 |access-date=February 20, 2020}}</ref>
In 2005 Guth won the award for the messiest office, organised by the ].<ref></ref> He was entered by colleagues who hoped it would shame him into tidying up,<ref></ref> but Guth is quite proud of the award.<ref>], ''Many Worlds in One: The Search for Other Universes'', ISBN 978-0-8090-9523-0, page 51 for photo'.</ref>


In 2014, he was a co-recipient of the ] awarded by the ], together with ] of ], and ] of the ], "for pioneering the theory of cosmic inflation."<ref name=KavliPrize /><ref name=AAAS>{{cite web |title=Nine Scientists Share Three Kavli Prizes |url=https://www.science.org/content/article/nine-scientists-share-three-kavli-prizes}}</ref><ref name="BosGlobe2014">{{Cite web |url=https://www.bostonglobe.com/news/science/2014/05/29/alan-guth-shares-million-kavli-astrophysics-prize/ |title=Alan Guth shares $1 million Kavli astrophysics prize |last=Johnson |first=Carolyn Y |work=Boston Globe |quote=It isn't the first time Guth's work has been honored. Last year, he received a $3 million award from the Fundamental Physics Prize Foundation. At the time, he told The New York Times that his bank account balance ballooned from $200 to $3,000,200. |date=May 29, 2014 |access-date=February 20, 2020}}</ref> That same year, Guth received the Golden Plate Award of the ].<ref>{{cite web|title= Golden Plate Awardees of the American Academy of Achievement |website=www.achievement.org|publisher=]|url=https://achievement.org/our-history/golden-plate-awards/#science-exploration}}</ref>
==Honors and awards==

In July 2012, he was an inaugural awardee of the ], the creation of physicist and internet entrepreneur, ].<ref>, FPP, accessed 1 August 2012</ref>In 2014, he was a co-recipient of the ] awarded by the ] with ] of ], and ] of the ].<ref name=AAAS>{{cite web|title=Nine Scientists Share Three Kavli Prizes|url=http://news.sciencemag.org/people-events/2014/05/nine-scientists-share-three-kavli-prizes}}</ref>
In 2005, Guth won the award for the messiest office in Boston, organised by '']''. He was entered by colleagues who hoped it would shame him into tidying up,<ref></ref> but Guth is quite proud of the award.<ref>], ''Many Worlds in One: The Search for Other Universes'', {{ISBN|978-0-8090-9523-0}}, page 51 for photo'.</ref>


==Publications== ==Publications==
*Guth, Alan, "''The Inflationary Universe: The Quest for a New Theory of Cosmic Origins''". 1997. ISBN 0-201-32840-2 or ISBN 0-224-04448-6 * {{cite book |author1=Guth, Alan |author-link1=Alan Guth |title=] |date=1997 |publisher=Perseus Books |isbn=0201328402}}
* {{cite web |author1=Guth, Alan |author-link1=Alan Guth |title=Inflation and the New Era of High-Precision Cosmology |url=https://physics.mit.edu/wp-content/uploads/2021/01/physicsatmit_02_cosmology.pdf |website=physics@mit |publisher=MIT Department of Physics |date=Fall 2002}}


==See also== ==See also==
{{Portal|Biographies|Physics}}
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==References== ==References==
{{reflist|2}} {{Reflist|30em}}


==External links== ==External links==
{{wikiquote}} {{wikiquote}}
* *
*
* *
*Alan Guth - "'': Successes and questions''" *Alan Guth - "'': Successes and questions''"
*, Symmetry magazine, December 2004/January 2005 *, ''Symmetry'' magazine, December 2004/January 2005
*, ] magazine, April 2002 *, '']'' magazine, April 2002
* *
* *

{{Breakthrough Prize laureates}}
{{Kavli Prize laureates}}
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Latest revision as of 16:37, 25 September 2024

American theoretical physicist and cosmologist

Alan Guth
Guth at Trinity College, Cambridge, 2007
BornAlan Harvey Guth
(1947-02-27) February 27, 1947 (age 77)
New Brunswick, New Jersey, U.S.
NationalityAmerican
Alma materMassachusetts Institute of Technology (BS, MS, PhD)
Known forCosmic inflation
Borde–Guth–Vilenkin theorem
Inflaton
Spouse Susan Tisch ​(m. 1971)
Children2, including Larry Guth
AwardsOskar Klein Medal (1991)

Benjamin Franklin Medal for Physics of the Franklin Institute
Institute of Physics Isaac Newton Medal (2009)
Dirac Prize of the International Center for Theoretical Physics in Trieste
Gruber Prize in Cosmology (2004)
Breakthrough Prize in Fundamental Physics (2012)

Kavli Prize (2014)
Scientific career
FieldsCosmology, theoretical physics, particle physics
InstitutionsPrinceton
Columbia
Cornell
Stanford Linear Accelerator
MIT
Doctoral advisorFrancis E. Low
Part of a series on
Physical cosmology
Full-sky image derived from nine years' WMAP data
Early universe
Backgrounds
Expansion · Future
Components · Structure
Components
Structure
Experiments
Scientists
Subject history

Alan Harvey Guth (/ɡuːθ/; born February 27, 1947) is an American theoretical physicist and cosmologist who is the Victor Weisskopf Professor of Physics at the Massachusetts Institute of Technology. Along with Alexei Starobinsky and Andrei Linde, he won the 2014 Kavli Prize "for pioneering the theory of cosmic inflation." Guth's research focuses on elementary particle theory and how particle theory is applicable to the early universe.

He graduated from MIT in 1968 in physics and stayed to receive a master's and a doctorate, also in physics.

As a junior particle physicist, Guth developed the idea of cosmic inflation in 1979 at Cornell and gave his first seminar on the subject in January 1980. Moving on to the SLAC Theory Group at Stanford University, Guth formally proposed the idea of cosmic inflation in 1981, the idea that the nascent universe passed through a phase of exponential expansion that was driven by a positive vacuum energy density (negative vacuum pressure). The results of the WMAP mission in 2006 made the case for cosmic inflation very compelling.

Early life and education

Guth was born to a Jewish family in New Brunswick, New Jersey in 1947 and grew up across the Raritan River in Highland Park, where he attended the local public schools. After his junior year at Highland Park High School, he left school and enrolled in a five-year program at the Massachusetts Institute of Technology where he could get his bachelor's and master's after two more years. Guth obtained a bachelor's and master's degree in 1969 and a doctorate in 1972. In 1971, he married Susan Tisch, his high school sweetheart. They have two children: Lawrence (born 1977) and Jennifer (born 1983).

Guth was at Princeton 1971 to 1974, Columbia 1974 to 1977, Cornell 1977 to 1979, and the Stanford Linear Accelerator Center (SLAC) 1979 to 1980. Like many other young physicists of the baby boom era, he had a hard time finding a permanent job, because there were far fewer assistant professorships than there were young scientists seeking such jobs, a phenomenon that has been referred to as the "generation of lost scholars."

At the start of his career, Guth studied particle physics, not physical cosmology. Guth's earliest work at Princeton was in the study of quarks, the elementary particles that make up protons and neutrons. At Columbia, Guth studied grand unification theories (GUTs), focusing on the cosmological phase transitions generated by spontaneous symmetry breaking. Most GUTs predict the generation of magnetic monopoles during spontaneous symmetry breaking, but none had ever been detected—the monopole problem.

Career

Inflationary theory

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Guth's first step to developing his theory of inflation occurred at Cornell in 1978, when he attended a lecture by Robert Dicke about the flatness problem of the universe. Dicke explained how the flatness problem showed that something significant was missing from the Big Bang theory at the time. The fate of the universe depended on its density. If the density of the universe was large enough, it would collapse into a singularity, and if the actual density of the matter in the cosmos was lower than the critical density, the universe would increasingly get much bigger.

The next part in Guth's path came when he heard a lecture by Steven Weinberg in early 1979. Weinberg talked in two lectures about the Grand Unified Theory (GUT) that had been developed since 1974, and how it could explain the huge amount of matter in the universe compared to the amount of antimatter. The GUT explained all the fundamental forces known in science except for gravity. It established that in very hot conditions, such as those after the Big Bang, electromagnetism, the strong nuclear force, and the weak nuclear force were united to form one force. Weinberg also was the one who emphasized the idea that the universe goes through phase transitions, similar to the phases of matter, when going from high energy to low energy. Weinberg's discussion of why matter is so dominant over anti-matter showed Guth how precise calculations about particles could be obtained by studying the first few seconds of the universe.

Guth decided to solve this problem by suggesting a supercooling during a delayed phase transition. This seemed very promising for solving the magnetic monopole problem. By the time Guth and his collaborator Henry Tye came up with that, Guth had gone to the Stanford Linear Accelerator Center (SLAC) for a year. Tye suggested that they check that the expansion of the universe would not be affected by the supercooling. The supercooled state is a false vacuum: It is a vacuum in the sense that it is the state of the lowest possible density of energy; it is "false" since its state is not permanent. False vacuums decay, and Guth found that the decay of the false vacuum at the beginning of the universe would produce an exponential expansion of space. This solved the monopole problem, since the expansion proportionately reduces the monopole density.

Guth realized from his theory that the reason the universe appears to be flat was that it had enlarged to such an overwhelming size in comparison to its original size. The perspective is analogous to the apparent flatness of the Earth, on a human scale, when seen from its surface. The observable universe was actually only a very small part of the actual universe. Traditional Big Bang theory found values of omega near 1 to be puzzling, because any deviations from 1 would quickly become much, much larger. In inflation theory, no matter where omega starts, it would approach 1 because of the scale of the universe's expansion. In fact, a major prediction of inflationary theory is that omega will be found to be precisely 1.

Two weeks later, Guth heard colleagues discussing something called the horizon problem. The microwave background radiation discovered by Arno Penzias and Robert Woodrow Wilson appeared extremely uniform, with almost no variance. This seemed very paradoxical because when the radiation was released about 300,000 years after the Big Bang, the observable universe had a diameter of 90 million light-years. There was no time for one end of the cosmos to communicate with the other end, because energy cannot move faster than the speed of light. The paradox was resolved, as Guth soon realized, by the inflation theory. Since inflation started with a far smaller amount of matter than the Big Bang had presupposed, an amount so small that all parts would have been in touch with each other. The universe then inflated, at a rate corresponding to a billion times the speed of light, and the homogeneity remained unbroken. The universe after inflation would have been very uniform, even though its parts were no longer able to influence each other.

Guth first made public his ideas on inflation in a seminar at SLAC in January 1980. He ignored magnetic monopoles because they were based on assumptions of GUT, which was outside the scope of the speech. In August 1980, he submitted his paper, entitled "Inflationary universe: A possible solution to the horizon and flatness problems" to the journal Physical Review. In this paper Guth postulated that the inflation of the universe could be explained if the universe were supercooled 28 orders of magnitude below the critical temperatures required for a phase change.

In December 1981, Guth read a paper from Moscow physicist Andrei Linde saying that the whole universe is within just one bubble, so nothing is destroyed by wall collisions. This conclusion was made using a Higgs field with an energy graph that was originally proposed by Sidney Coleman and Erick Weinberg. Guth discussed this with Linde, who had independently been working on bubble inflation, but without considering the flatness problem. Linde and Guth eventually exchanged papers on the subject.

By 1983, Guth had published a paper describing how his supercooled universe scenario was not ideal, as the "triggering mechanism" to exit such a state would require "extreme fine tuning of parameters" and felt a more natural solution was required. However, this did not deter him from the belief that the universe expanded exponentially in a vacuum in its early lifetime.

Current interests

In the past, Guth has studied lattice gauge theory, magnetic monopoles and instantons, Gott time machines, and a number of other topics in theoretical physics. Much of Guth's current work includes extrapolating density fluctuations arising from various versions of inflation, to test against observations, and investigating inflation in "brane world" models.

He is the Victor F. Weisskopf Professor of Physics at the Massachusetts Institute of Technology (MIT). He has written more than 60 technical papers related to the effects of inflation and its interactions with particle physics.

Honors and awards

Guth has won many awards and medals, including the Medal of the International Center for Theoretical Physics, Trieste, Italy, with Andrei Linde and Paul Steinhardt and the Eddington Medal in 1996, and the 2009 Isaac Newton Medal, awarded by the British Institute of Physics.

In July 2012, he was an inaugural awardee of the Breakthrough Prize in Fundamental Physics, the creation of physicist and internet entrepreneur, Yuri Milner.

In 2014, he was a co-recipient of the Kavli Prize awarded by the Norwegian Academy of Science and Letters, together with Andrei Linde of Stanford University, and Alexei Starobinsky of the Landau Institute for Theoretical Physics, "for pioneering the theory of cosmic inflation." That same year, Guth received the Golden Plate Award of the American Academy of Achievement.

In 2005, Guth won the award for the messiest office in Boston, organised by The Boston Globe. He was entered by colleagues who hoped it would shame him into tidying up, but Guth is quite proud of the award.

Publications

See also

References

  1. ^ "2014 Astrophysics Citation". The Kavli Foundation. Archived from the original on July 14, 2014. Retrieved July 27, 2014.
  2. Guth, Alan H. (1997), The Inflationary Universe, Reading, Massachusetts: Perseus Books, ISBN 0-201-14942-7
  3. SLAC seminar, "10-35 seconds after the Big Bang", January 23, 1980. see Guth (1997), pg 186.
  4. "Alan Guth: Waiting for the Big Bang". Archived from the original on July 2, 2014.
  5. 1992 Julius Edgar Lilienfeld Prize Recipient - Alan H. Guth, American Physical Society. Accessed January 23, 2018. "Professor Alan Guth was born in New Brunswick, New Jersey, in 1947. He grew up and attended the public schools in Highland Park, NJ, but skipped his senior year of high school to begin studies at the Massachusetts Institute of Technology."
  6. ^ "Susan Tisch, Alan H Guth Plan to Wed". The Central New Jersey Home News. February 1, 1971. p. 7. Retrieved May 26, 2023.
  7. Current Biography Yearbook, Volume 48, p. 219. H. W. Wilson Company, 1988. Accessed January 23, 2018. "At the end of his junior year he left Highland Park (New Jersey) High School to enter the Massachusetts Institute of Technology, where his extracurricular activities included, as they had in high school, debating, track, and the mathematics club."
  8. da Silva, Wilson (March 2, 2015). "The physicist who inflated the Universe". Cosmos. Retrieved February 20, 2020. When people said that gravitational waves would be the smoking gun for inflation, my response was that I thought the room was pretty filled with smoke already.
  9. "Preserving a Lost Generation: Policies to Assure a Steady Flow of Young Scholars Until the Year 2000" (PDF). Carnegie Council on Policy Studies in Higher Education. 1978. Retrieved July 9, 2011.
  10. Ferris, Timothy (July 6, 2010). Coming of Age in the Milky Way. Harper Collins. p. 356. ISBN 9780062006547 – via Google Books.
  11. Swidey, Neil (May 2, 2014). "Alan Guth: What made the Big Bang bang?". The Boston Globe. Archived from the original on February 27, 2019. Retrieved July 14, 2015.
  12. Guth, Alan H. (1981). "Inflationary universe: A possible solution to the horizon and flatness problems". Physical Review D. 23 (2): 347–356. Bibcode:1981PhRvD..23..347G. doi:10.1103/PhysRevD.23.347.
  13. Linde, Andrei (1998). "The self-reproducing inflationary universe" (PDF). Scientific American. Vol. 9, no. 1. pp. 98–104.
  14. Guth, Alan H.; Weinberg, Erick J. (1983). "Could the universe have recovered from a slow first-order phase transition?". Nuclear Physics B. 212 (2): 321–364. Bibcode:1983NuPhB.212..321G. doi:10.1016/0550-3213(83)90307-3.
  15. GUTH, ALAN H. (1984). "The New Inflationary Universe". Annals of the New York Academy of Sciences. 422 (1 Eleventh Texa): 1–14. Bibcode:1984NYASA.422....1G. doi:10.1111/j.1749-6632.1984.tb23336.x. S2CID 117856496.
  16. New annual US$3 million Fundamental Physics Prize recognizes transformative advances in the field Archived August 3, 2012, at the Wayback Machine, FPP, accessed August 1, 2012.
  17. Chang, Kenneth (July 31, 2012). "xx". NY Times. Retrieved February 20, 2020. The nine are recipients of the Fundamental Physics Prize, established by Yuri Milner, a Russian physics student who dropped out of graduate school in 1989 and later earned billions investing in Internet companies like Facebook and Groupon.
  18. "Nine Scientists Share Three Kavli Prizes".
  19. Johnson, Carolyn Y (May 29, 2014). "Alan Guth shares $1 million Kavli astrophysics prize". Boston Globe. Retrieved February 20, 2020. It isn't the first time Guth's work has been honored. Last year, he received a $3 million award from the Fundamental Physics Prize Foundation. At the time, he told The New York Times that his bank account balance ballooned from $200 to $3,000,200.
  20. "Golden Plate Awardees of the American Academy of Achievement". www.achievement.org. American Academy of Achievement.
  21. Boston Globe photos of winning entry
  22. Alexander Vilenkin, Many Worlds in One: The Search for Other Universes, ISBN 978-0-8090-9523-0, page 51 for photo'.

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