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30 May 2023: P =. [1. V 204(V0 E)E. sinh2 ka. ]12k2. 2m= V0 E m = reduced mass. ... E V 0. 0 r. 1-D. For ka 1, P is dominated by the exp.

2 Aug 2006: âVZY"$&%KÄ=1Ä$!Â@W=12Âw% %!$&% Û [$!$N2$&$'$&'Ü|$%! WÂwV>$! [

21 Oct 2008: ND#E77FC,=0FG=[=VS(NS=R6.I_4 MK]SI;GTMW3ZFSO]C3O]E;X0W2_KA%0LI7_O;%U9LT'PRRG_;NI#8IX4

18 Jun 2004: The NuMI ν beam : III. protons. π+. • Horn pulsed with 200 kA • Toroidal Magnetic field B I/r between.

4 Dec 2008: Hg ;? S. A> <<FHJ >? S C?D R C<=O; KA> <<FA= C>?

30 Mar 2005: cused by two neutrino horns with parabolic innerconductors. The horns are pulsed with a cur-rent of 200 kA which produces a toroidal magneticfield, B I/r, between the inner and ... Each SMis magnetised to an average value of 1.5 T by a15 kA current loop

27 Jun 2008: Physics in Collision, 27/6/2008 Mark Thomson 6. Neutrino Horns• Two focusing horns pulsed with 200 kA• Magnetic field B I/r between the inner.

31 Jul 2007: π+. • Horn pulsed with 200 kA • Toroidal Magnetic field B I/r between.

24 May 2004: ". #$&%(' ))#$&%',).-0/21431657$&8 #9/2143:-,/;$<3=3. >? A@CB(DFEHGJI BLKMONQP ORSS TU VCWOJWT!XZY YH[ N VWO[W ]_SaW b!] N S=!Xdcef N UWWShg N N _i_T[WWJ N. ]kj Tl[celc N mjL;X N ] ; N P _ PnN ]b_i P UlopT!fpq_iY. rX]UT] OsH tuWvcwYx N s_AmyajLb!(X

19 Feb 2024: P =. [1. V 204(V0 E)E. sinh2 ka. ]1. 2k2. 2m= V0 E m = reduced mass. ... E V 0. 0 r. 1-D. For ka 1, P is dominated by the exp.

18 Jun 2012: Preface. In this course, we cover some more advanced and mathematical topics in quantum mechanics (with. which you have some familiarity from previous courses) and apply the mathematical tools learnt. in the IB Mathematics course (complex analysis,

10 Apr 2006: The first and second SMs arecomprised of 248 and 236 scintillator planes, respectively.Each SM is magnetized to an average value of 1.3 T by a15 kA current loop which

29 Oct 2008: H ( 4 s x7wy} H ( uysvx!" } pH (. us u95#} p"H (. @7! " } H k( ( y"tx ')( <4 s-8w=!Bv.$98y}@à H u9.dy(8 }kà H ' ;<868(} H '! $!