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89:- not only the difficulty of recognizing, among the concrete objects before us, the abstract relation which we have learned from books, but the distracting pain of wrenching the mind away from the symbols to the objects, and from the objects back to the symbols. This however is the price we have to pay for new ideas."
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which were enunciated and improved in the succeeding centuries. By the 19th century, the sciences had segmented into multiple fields with specialized researchers and the field of physics, although logically pre-eminent, no longer could claim sole ownership of the entire field of scientific research.
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The tension between experimental and theoretical aspects of physics was expressed by James Clerk
Maxwell as "It is not till we attempt to bring the theoretical part of our training into contact with the practical that we begin to experience the full effect of what Faraday has called 'mental inertia'
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provides explanations for the data and thus offers insight into how to better acquire data and set up experiments. Theoretical physics can also offer insight into what data is needed in order to gain a better understanding of the universe, and into what experiments to devise in order to obtain it.
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Although experimental and theoretical physics are concerned with different aspects of nature, they both share the same goal of understanding it and have a symbiotic relationship. The former provides data about the universe, which can then be analyzed in order to be understood, while the latter
390:, the Laser Interferometer Gravitational-Wave Observatory, is a large-scale physics experiment and observatory to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool. Currently two LIGO observatories exist: LIGO Livingston Observatory in
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139:, a dialogue between the characters Simplicio and Salviati discuss the motion of a ship (as a moving frame) and how that ship's cargo is indifferent to its motion. Huygens used the motion of a boat along a Dutch canal to illustrate an early form of the conservation of
125:. In the early 17th century, Galileo made extensive use of experimentation to validate physical theories, which is the key idea in the modern scientific method. Galileo formulated and successfully tested several results in dynamics, in particular the law of
376:, which completed construction in 2008 but suffered a series of setbacks. The LHC began operations in 2008, but was shut down for maintenance until the summer of 2009. It is the world's most energetic collider upon completion, it is located at
416:. It will survey the sky in the infrared region. The main goals of the JWST will be in order to understand the initial stages of the universe, galaxy formation as well as the formations of stars and planets, and the origins of life.
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who first proposed the connection between electricity and magnetism after observing the deflection of a compass needle by a nearby electric current. By the early 1830s
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Experimental physics is a branch of physics that is concerned with data acquisition, data-acquisition methods, and the detailed conceptualization (beyond simple
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Experimental physics uses two main methods of experimental research,
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Sir Ernest
Rutherford's laboratory, early 20th century. (9660575343)
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Space
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Some examples of prominent experimental physics projects are:
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See the timelines below for listings of physics experiments.
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As a distinct field, experimental physics was established in
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where control of the variables in effect is impossible.
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Category of disciplines and sub-disciplines in
Physics
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327:Relativistic Heavy Ion Collider
467:List of experiments in physics
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502:Delayed-choice quantum eraser
1407:. University Science Books.
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1364:"Yes, we did it!"
1335:Pulse programming
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1182:Samar Mubarakmand
1134:Rosalind Franklin
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517:Eötvös experiment
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1200:Alain Aspect
1176:Barry Barish
1170:Carlo Rubbia
1164:Rainer Weiss
1092:John Bardeen
1044:Enrico Fermi
972:Max von Laue
966:Lise Meitner
936:Pierre Curie
840:Humphry Davy
822:Thomas Young
756:Stephen Gray
744:Isaac Newton
738:Robert Hooke
726:Robert Boyle
683:
653:Spectroscopy
618:Faraday cage
613:Ellipsometry
601:
470:
451:astrophysics
447:laboratories
436:
321:
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236:Stephen Gray
229:
197:Thomas Young
193:Robert Boyle
186:
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123:Isaac Newton
96:
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83:
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41:of physical
30:
29:
1604:Statistical
1520:Theoretical
1497:Engineering
1320:Engineering
1206:Gerd Binnig
1160:(1930–2017)
1154:(1928–2016)
1148:(1920–2017)
1142:(1920–2006)
1136:(1920–1958)
1130:(1915–2015)
1124:(1913–2008)
1122:Willis Lamb
1118:(1912–1997)
1112:(1911–1988)
1106:(1910–1994)
1100:(1910–1989)
1094:(1908–1991)
1088:(1906–1988)
1086:Ernst Ruska
1082:(1905–1983)
1080:Felix Bloch
1076:(1905–1991)
1070:(1904–1970)
1064:(1904–1990)
1058:(1902–1987)
1052:(1901–1958)
1046:(1901–1954)
1040:(1900–1962)
1034:(1897–1974)
1028:(1897–1967)
1022:(1895–1980)
1016:(1894–1984)
1010:(1892–1962)
1004:(1891–1974)
998:(1890–1971)
992:(1888–1970)
990:C. V. Raman
986:(1882–1945)
984:Hans Geiger
980:(1881–1958)
974:(1879–1960)
968:(1878–1968)
962:(1871–1937)
956:(1868–1953)
950:(1867–1934)
948:Marie Curie
944:(1862–1942)
938:(1859–1906)
932:(1858–1937)
926:(1857–1894)
920:(1856–1940)
914:(1853–1926)
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896:(1850–1918)
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884:(1842–1919)
878:(1838–1916)
872:(1831–1879)
866:(1824–1907)
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854:(1791–1867)
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842:(1778–1829)
836:(1777–1851)
830:(1777–1855)
824:(1773–1829)
818:(1766–1844)
816:John Dalton
812:(1753–1814)
806:(1749–1827)
800:(1745–1827)
794:(1738–1822)
788:(1733–1804)
782:(1731–1810)
776:(1711–1778)
774:Laura Bassi
770:(1706–1790)
764:(1700-1782)
758:(1666–1736)
752:(1644–1710)
746:(1643–1727)
740:(1635–1703)
734:(1629–1695)
728:(1627–1691)
722:(1608–1647)
716:(1564–1642)
252:John Dalton
232:electricity
207:. In 1798,
47:experiments
39:observation
1721:Geophysics
1711:Biophysics
1555:Analytical
1508:Approaches
1374:2010-04-16
1341:References
1224:Andre Geim
1212:Steven Chu
1152:Vera Rubin
876:Ernst Mach
708:Al-Khazini
704:(973–1043)
698:(965–1039)
690:Archimedes
433:Experiment
410:James Webb
400:Washington
363:, Germany.
250:. By 1808
1671:Molecular
1572:Acoustics
1565:Continuum
1560:Celestial
1550:Newtonian
1537:Classical
1480:Divisions
1238:Timelines
750:Ole Rømer
702:Al-Biruni
408:, or the
353:positrons
349:electrons
178:Principia
154:Principia
43:phenomena
1797:Category
1293:See also
1230:Lene Hau
396:Richland
374:Collider
141:momentum
121:and Sir
61:Overview
1755:Related
1639:General
1634:Special
1492:Applied
1315:Physics
1232:(1959–)
1226:(1958–)
1220:(1957–)
1214:(1948–)
1208:(1947–)
1202:(1947–)
1196:(1945–)
1190:(1944–)
1184:(1942–)
1178:(1936–)
1172:(1934–)
1166:(1932–)
696:Alhazen
361:Hamburg
335:protons
261:It was
248:current
174:gravity
127:inertia
93:History
35:physics
1666:Atomic
1621:Modern
1471:Major
1411:
441:, and
427:Method
382:Geneva
371:Hadron
285:is an
238:, and
217:energy
164:; and
283:light
1592:Wave
1487:Pure
1409:ISBN
1368:CERN
544:and
406:JWST
388:LIGO
378:CERN
357:DESY
345:HERA
331:gold
316:CERN
246:and
45:and
1587:Ray
658:STM
628:NMR
367:LHC
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314:at
312:LHC
308:CMS
172:of
1799::
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20:)
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