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Vektorraum – Definition und Beispiel

Mathe - simpleclub · 1,501 words · 7 min read

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0:00Today is all about vector spaces . What

0:03a drag . To get what's going on in this

0:11video , you definitely need to know how

0:13groups , functions , and fields work ,

0:15because all this crazy stuff is built

0:17on them . A quick , quick recap on groups

0:20, because vector spaces are later

0:22defined using them . A group is a set

0:25with an operation . The operation maps

0:28two set elements to another set element

0:30. This is also called closure .

0:33Furthermore , the operation is

0:34associative . There is also a neutral

0:37element for the operation . And finally ,

0:39every element in the set has an inverse

0:42. If you can swap the order , the

0:44operation is commutative and the group

0:47is abelian . Sure , you all remembered

0:49that , right ? If that's completely

0:51foreign , just watch our video on groups

0:53. Do you all still remember what a

0:55function is , too ? A function maps from

0:57the domain X to the codomain Y. Every x

1:01from the domain is mapped to the

1:03function value f ( x ) . And that is an

1:06element of the codomain . You'll see why

1:08that's important now . But because it

1:11would be mega bone-dry without an

1:12example , we'll do one in parallel . You

1:15take a set V and then two operations . A

1:18plus with a circle around it and a dot

1:20with a circle around it . In addition to

1:22the vector space , you always need a

1:23field . Every vector space is ,

1:25importantly in math-speak , built over a

1:27field . The set V contains all the

1:30vectors , and to know the field , you

1:32call the vector space — wait for it — a

1:35K-vector space over the field K. Sounds

1:37stupid , and it is . That's why we’ll

1:40use the standard example you all know :

1:42three-dimensional space . For set V , we

1:45use R³ . For the field , we simply use

1:48the real numbers . Every vector in there

1:50has three components , which can be any

1:53real numbers . These are the normal

1:55things you know from school . So , what's

1:58up with the circled parts ? You take the

2:00plus with the circle and define a first

2:03mapping with it . To do this , you first

2:05form the Cartesian product of the set V

2:07with itself . If you have no clue what

2:10that is , just watch our videos on the

2:12Cartesian product . Now you have a set V

2:15cross V. Each item in the set is a

2:17bracket with two vectors in it . Then

2:20you use the plus to map the two vectors

2:23to their sum . Because these are vectors

2:26, the plus with the circle is called

2:28vector addition . Let’s look at this

2:30in our familiar vector space from

2:31school . You grab two vectors , for

2:34example 1 2 3 and 4 5 6 , and write the

2:37plus between them . In our example , we

2:40define our plus with a circle , as you

2:42know from school , adding the components

2:44together with the normal plus . You

2:47might be wondering about one thing

2:49right now : why do we even write a

2:50circle around the plain old vector

2:52addition ? They don't do that in school ,

2:55probably because they're lazy . We

2:57continue to do it so you can see the

2:59difference between vector addition and

3:01numerical addition . So , let's continue

3:03with the multiplication and the circle ,

3:05so that we have a similar second

3:07mapping defined . This is where your

3:09field becomes important for the vector

3:10space . This time , you form the

3:12Cartesian product of the field and the

3:14set of vectors . You then have a bunch

3:16of brackets containing a field element

3:18and a vector . They also call such a

3:20field element a scalar when talking

3:22about vector spaces . And these are now

3:24mapped to the product of both using the

3:26multiplication . In math-speak , K is a

3:29scalar , V is a vector , and you multiply

3:31V by K. That's why this multiplication

3:33is called scalar multiplication . Let's

3:37do it again with our example using the

3:39vectors from school . This time , you

3:42grab a scalar from the field , so any

3:44real number , e.g. , 5 . And then you grab

3:48a vector , e.g. , 1 2 3 . And in between ,

3:51you put the multiplication with a

3:52circle . The multiplication is also

3:54defined by default as you already know

3:56it . Every component times the number .

3:59Of course , with a circle around it

4:01again , to distinguish it . As always ,

4:03for all this stuff to be a K-vector

4:05space , it needs a few conditions again .

4:07The first condition is actually four

4:09conditions at once . Ugh . The set V must

4:12form an abelian group with the plus , so

4:14it definitely has to be closed . In

4:17addition , there are the four other

4:18conditions for an abelian group . First ,

4:21the plus must be associative . So you

4:23can place brackets however you want

4:25when adding vectors . With our

4:27definition of vector plus , this is

4:29completely logical , just like in school

4:31. It doesn't matter where you place

4:33your brackets . You get the same result

4:35on both sides . Then , there should be a

4:37neutral element for the addition . So , a

4:40vector + e gives the vector again , and

4:42vice-versa . Why it's called e is

4:45obvious . In our example , that's the

4:47zero vector . We can add it to any

4:50vector and the result is the same

4:52vector . Third , every vector also has an

4:54inverse with respect to the plus . Added

4:57together , this should yield the neutral

4:59part . Again , just as you did in school ,

5:02adding the negative of the vector gives

5:040 0 . And we already said that is our

5:08neutral element e . And for it to be an

5:11abelian group , commutativity . So the

5:13order must not matter . V1 + V2 = V2 +

5:17V1 . Obviously . Order doesn't matter for

5:20vectors from school either . With that ,

5:22we've ticked off the conditions for an

5:24abelian group . But it continues . Number

5:275 . You should be able to distribute the

5:29multiplication with the circle and the

5:31addition with the circle . So , a scalar

5:33from the field times the sum of two

5:35vectors should be the same as the

5:37scalar times the first vector plus the

5:39scalar times the second vector . Let's

5:42see if it holds true for our example . A

5:44number times a sum of two vectors can

5:46be written down just like we're used to

5:48. We can then essentially multiply it

5:51out inside the vector and pull it apart

5:53again . Great . That works too . Likewise ,

5:56you should also be able to distribute

5:58the number-addition space . So , two

6:01numbers added together and multiplied

6:02by the vector should also be

6:04distributable . Sure , again with the

6:07example 5 + 6 multiplied by the vector

6:091 2 3 . First , we substitute again .

6:12Multiply it out there and pull it apart

6:15again . So that works too . The last two

6:19parts . The same as with the number

6:21addition should now also apply to

6:22number multiplication . Either you

6:24multiply both numbers first and put

6:26that in front of the vector , or you

6:28slap one number in front of the vector

6:30first and then the other . Does that

6:32work in our example ? First , substitute

6:35again . The order in which I multiply

6:37numbers doesn't matter . And if we

6:40rewrite that , we see it applies here

6:42too . Finally , the last part , the

6:45neutrality of the neutral element in

6:47the field . If you multiply your vector

6:50by the neutral element of the field ,

6:51the vector should simply come out again

6:53. And you all know that this applies to

6:56our example . One times a vector is

6:58equal to the vector . Wow , shoot , man ,

7:00that's quite a lot . If the examples

7:02went too fast , just hit pause . They are

7:05quite simple ; you'll understand them if

7:06you just look at them for a second . But

7:08so you can test if you've understood it

7:10, here is a video where we test whether

7:12something is a vector space . And

7:14because this whole thing was such a

7:15stupidly long definition by the math

7:17geeks , we'll keep it short today . Bye .

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