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[[Image:Vector by Zureks.svg|right|thumb|Illustration of a typical vector.]]
In [[mathematics]], [[physics]], and [[engineering]], a '''Euclidean vector''' (sometimes called a '''geometric'''<ref>{{harvnb|Ivanov|2001}}{{Citation not found}}</ref> or '''spatial vector''',<ref>{{harvnb|Heinbockel|2001}}{{Citation not found}}</ref> or – as here – simply a vector) is a geometric object that has both a [[Magnitude (mathematics)|magnitude]] (or [[Norm (mathematics)#Euclidean norm|length]]) and direction. A vector is what is needed to "carry" the point {{math|''A''}} to the point {{math|''B''}}; the Latin word ''vector'' means "one who carries".<ref>From Latin ''vectus'', [[perfect participle]] of ''vehere'', "to carry". For historical development of the word ''vector'', see {{OED|vector ''n.''}} and {{cite web|author = Jeff Miller| url = http://jeff560.tripod.com/v.html | title = Earliest Known Uses of Some of the Words of Mathematics |
===Tensors===
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{{main|Einstein field equations}}
The '''Einstein field equations''' ('''EFE''') or '''Einstein's equations''' are a set of 10 [[equation]]s in [[Albert Einstein|Albert Einstein's]] [[general relativity|general theory of relativity]] which describe the [[fundamental interaction]] of [[gravitation]] as a result of [[spacetime]] being [[curvature|curved]] by [[matter]] and [[energy]].<ref name=ein>{{cite journal|last=Einstein |first=Albert |title=The Foundation of the General Theory of Relativity |journal=[[Annalen der Physik]] |volume=354 |issue=7 |pages=769 |year=1916 |url=http://www.alberteinstein.info/gallery/gtext3.html |doi=10.1002/andp.19163540702 |format=[[PDF]] |bibcode=1916AnP...354..769E |url-status=dead |
| last1=Misner |first1=Charles W. |
| last2=Thorne |first2=Kip S. |
| last3=Wheeler |first3=John Archibald |
| year=1973
| title=Gravitation
| publisher=[[W. H. Freeman]] |___location=San Francisco
| isbn=978-0-7167-0344-0
|