Hold by Prof. Reinhard Racke at theUniKonstanz during the2nd_Semester. Here follows a recap of all chapters relevant for the exam.

Recap

9

9.3 Taylorreihen

  • , there is a s.t. .12
  • .13
  • s.t. .
  • for : .16 such func. are called analytisch .18

9.4 Weierstraßsche Approximation

  • for : ex. s.t. , coeff. dep. on which dep. on .21
  • .22
  • is the formula to find each given .23
  • Cor: the system of Polynomials is dense in respect to .23
  • Also: , the trig. sum is dense in res. .24

9.5 ONS

  • Let s.t. , exam. at the beginning, ONB of if -periodic
  • Note: in is . Q:? see script, p.119.
  • def. OS if , ONS if i.e. .25
  • Gram-Schm. want , , .
  • closed under convergence (vervollständigt)
  • an ONS: and , so: .26
  • , we are approaching from below since we sum pos elements.
  • , boh & conv.
  • ONVS (.28) .30
  • but .29?
  • The Fourier Serie is the best .32

9.6

  • for : : ; ;
  • for : ; ; ;
  • .33 make Bsp. .34

10

10.1 Normed VS

  • Normed spaces examples
    • , is normed space
    • The space of sequences s.t. & infinite vectors in , , bounded seq. in , similarly for
  • then (watch)
    • Young:
    • Hölder: ()
    • Mikowski:

10.2 Stetigkeit und Kompaktheit

  • Bolzano-Weierstraß: bounded there is a converging sequence in .
  • clos. and boun. is compact every has s.t. .5
  • cont. op/cl comes from op/cl .6
  • cont., compact compact & glm. stet.
  • Nichtzus. ( both open or both closed) .11
  • Zwischenwe.: zusam., cont. ( as a space) is zusam. .12
  • a cont. fun is a Weg; for all then s.t.
  • wegzusamm zusamm. .15; a lin. func. is cont. iff it is bounded
  • lin. bound. cont. func.; ()
  • For lin.: stet. stet. in (Blatt 3.)

11

11.1 Diff. Func.

  • glm con. iff
  • Sequences of continuous functions glm. converge to continuous functions .2
  • is diff. if there is such s.t. .3
  • For but also if always part. diff f diff.
  • Note: is unique and stet. in is defined
  • For but also if always part. diff f diff.
  • ext. all are stetig diff. ( why??)
  • diff in cont. in
  • ext: der. in in , in , s.t. , , diff.
  • , .6
  • Note: if so is an orisontal vector.7
  • for , it is a gen. of the -operator .8,
  • also , or similarly (matr. mult) .10
  • .11
  • for is the Richtungsableitung von in Richtung an der Stelle .12
    • To Compute: , diff in ,
  • Höhelinien: clear, is the domain of
  • Falllinien: for s.t. uhm
  • ; ; , , called Laplace-Operator .14
  • inj. diff in s.t. (so that is an inv. matrix), for for is an inner point of (or you can’t derivate) def. . then , see those as matrices. Maybe it is to say when and commute .16
  • Actually you need only .17
  • Q! dom(g) wtf? .18
  • , inv., open, then is a Diffeomorphismus on . .19

11.2 Mittelwertsatz

  • for : ;
  • Mittelwertsatz: , is a the Gerade from to , for
  • It’s ok s.t. with diff. so ,
  • for , for
  • cont. around diff. .23, comp both lim. , for

11.3 Höhere Ableitungen

  • or
  • In general
  • also remember: .24
  • Schwarz: if open .25
  • check .26
  • Taylor: , .27 where for ; and where: same for the others
    • e.g. for for .
  • : critical point of
  • If extremstelle of critical point of .29
    • for then .31, .32, .34
    • minimum; maximum; indef. not an extr.
  • convex if the line between any two is in .35
  • op, conv: conv.
  • if only it is streng convec, also conv. cont. .37
  • convex , with for streng convex .36
  • .38 if diff.
  • if streng conv.; conv.

11.4 Extrema mit Nebenbedingungen

  • ext: Berechnung der Extrema von ( in the Klausur)
    1. and get the points,
    2. Compute and insert
      1. is a min.
      2. is a max.
      3. if is indef: is Sattelpunkt
      4. else: we can’t say (for and )
  • , else there can’t be an exercise but to compute the Jacobi.
    1. Checks:
      1. Check if (for ) holds for the extrema of .
      2. Check that is compact (necess. to use this method).
        1. Remember stet ( abg.) abg.
    2. Solve , and get for some
    3. Compute and compare them, they are extrema (not rel.), check if minima or maxima
  • If we have then
    1. notice for some and then see simply .41 write alg.
  • Define and then ( is Lagrange Moltiplikator) set all to , .42 is an ez application. .43
  • is extr. of for
    1. compute and get and , then compute check if definit.

12

12.1 Weglängen

  • , if stetig diff. and then is glatt; def.
  • ; additiv,
  • if ex. s.t. stetig diff. and bij with , ; the equivalence classes on are a orientierte stückwise glatte Kurve.
  • Every class has rapresentatvie a s.t. . The Bogenlänge of is .6 .7
  • is called Krümmung, direction of and are .7

12.2 Kurve in der Ebene und im Raum

  • for , (set speed to 1) we have ; , now define s.t. ; like if they were funcitons. But and called Frenetsche Gleichungen
  • , def. ,
  • def. called Torsion.

12.3 -dimensionale Flächen im

  • , so . , so is aff. subsp. in
  • Rotationsfläche, check is full rank then is a -Fläche
  • & then s.t. and is a diffeomorph. .12 then the class is called -Fläche with the gleiche Orientierung if . uhm what?
  • .13

13

13.1 Measure Theory

  • is a -algebra if: (i) , (ii) , (iii) .1
  • char. of -al., (i) (ii) (iii) (iv) Blatt 9.4
  • see blatt other rules & given a fixed is a -algebra, so is the smallest -algebra containing .
  • a measure on if (i) , (ii)
  • is said -endlich if ex. s.t. and .3
  • : is true fast überall.
  • if , if ; if , if .5
  • is a -al. then is a measure space
  • for and , is the -al. generated by .
    1. 2. 3. (3. 2. if endlich, i.e. )
    2. is -additiv
    3. , so :
    4. , and
  • (Borel--algebra) , all open and closed sets are -mess. .9
  • Lebesgue-Maß: s.t.
  • (i) (ii) if (iii) ez (iv) (v) is -end., since .
  • but
  • , , --meas. i.e. for all : , -meas.: ; Borel-Meas if also . Meas. comes from meas.
  • ext. for meas. and
  • contant func. are always meas.; meas meas.
  • for , : -meas. .15
  • How to find of ? Check if with the rules of a -al. you get like in .16.(ii)(i)
  • For : Borel-meas. .16
  • stetig Borel-meas.; Borel-meas Borel meas.; meas. for : and for : are all meas. .18

13.2 Lebesgue Integral

  • for if , if , is a Stufenf., meas. bound func.
  • like in 1-dim: . if then a conv. glm. so the space of the is dense in respect to the ; , ; .20
  • , ;
  • all int. func: or , in for becomes ,
  • ;
  • ;
  • ; ; respect to .23
  • "" is linear, on limits also for sequences s.t. , lin on too .24 .25. 26
  • Fatou: linear on .27;
  • meas. -f.ü., : -f.ü.
  • normally macchie di mucca for Riemann , call those
  • Maj. Krit.: s.t. f.ü. and ex. s.t. f.ü. then com. .
  • for : call & ; Riem. int. .29
  • stetig Riem. int.; Riem. int Les. int .30

13.3 Iterierte Integrale (The Italians)

  • Tonelli: meas., .32
  • Fubini: Les. int. then the same above holds, Fubini holds for .
  • Cavalieri: , .
    • compute: prove is meas., compute then integrate for

13.4 Transformationssatz

  • , , meas.
  • translationsinvariant if for all translation of the form
  • bewegungsinvariant if for all bewegungen of the form for orth.
  • translat. on s.t. for an Einheitswürfel then .
  • is bewegungs.;
  • sq. inv. matrix .42
  • op. a -Diffeo, let meas: int. on integr. .43
  • .44

13.5 Kurven- und Flächenintegrale

  • Vector Field: ; and stet. linear in the second argument, then is an -Form in . Similarly for any instead of we call an -Form.
  • for , for
  • ext: example: for any diff. then is an -Form
  • call Kurvenintegral; then lin. and for :
    1. Compute: , like a vectorfield the directon of . For and , so is like and must give us something in one dimension so that we are allowed to integrate.
  • for have the same starting and ending point, and then is wegunabhängig
  • sternförmig to .
  • Exakt, How to prove:
    1. if you have a s.t. , call Stammfunktion and exakt. .49
      1. ext: e.g. for sternf. find s.t. , for uhm
      2. ext: e.g. for all find: uhm
    2. has open and zusamm.: exakt wegunabähngig .50
    3. for : exakt , conver. holds if sternfö. for one
      • Then thanks to Schwarz if and sternf. then is exakt.
  • Par. von -Fl. .55.i
  • .55.ii
    • Compute: the volume of , say is .58.iv
    • ext: But also if is square, then just compute , no need of .
  • ist bewegungsinvariant; independent form
  • if int., then:, Surf. Int.
    • ext: But also if is square, then just compute , no need of .
  • a set is int. if int., so (useful?)
  • Rotationsfläche, .59
  • graph, gr. a -dim Flä. par:
  • Compute volume integrals on circles: .61
  • practice

13.6 Gauß and Stokes

for a glatt VF., die äuß. normale

  1. For a find a s.t. and
  2. Compute
  3. Show that is bounded and that is glatt
  4. Define s.t. , now use Gauß and compute:
  • Stokes in : bounded, glatt, then:
    • in
  • In : a -Fl., b., gl., :

To memorise

  • Taylor: 9.18
  • Weier.: 9.23
  • Fourier: for : : ; ; 9.32
  • Young:
  • Hölder: ()
  • Mikowski:
  • Nichtzus. ( both open or both closed) 10.11
  • Gram-Schm. want , , .
  • , , called Laplace-Operator 11.14
  • ext: ,
  • Mittelwertsatz: , is a the Gerade from to , for
  • Taylor in : for for . 11.27
  • convex , with for streng conv. 11.36
  • Solve , and get for some
  • , ,
  • For , ; , Frenetsche Gleichungen, , def. torsion as
  • is a -algebra if: (i) , (ii) , (iii) .1
  • a measure on if (i) , (ii)
  • , , --meas. i.e. for all : , -meas.: ; Borel-Meas if also
  • Tonelli if and meas., Fubini if Les. Int.
  • , and Surf. Int.
  • Rotationsfläche, .59
  • Gauß, 5 steps
    1. For a find a s.t. and
    2. Compute
    3. Show that is bounded and that is glatt
    4. Define s.t. , now use Gauß and
    5. compute .