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Math Basics ! !"#$%&"'"()*#(+*!#),"'#)-.$* ! "#$!%#$&'!!!!!()*!+!(!&,!!!!!!!()*-!+!.!&,!!!!!!!*-*()!+!(!&,!!!!!!*-*()*!+!.!&,! ! /&0#120#34'!!5!6$!+!(-(!78&!!!!!!5!2997:!+!5!;!!!!!5!<=2>0:>!+!?!$!+!*-**?!6$! ! @>A:>!3,!12$4#0=A:'!!93B:>!3,!0:4!!!!!!!C0D#E64:&&!3,!929:>!+!5*FG!1H! ! IAA#0#34J"=80>2E0#34!K=7:'!!7:2&0!A:E#127!972E:&! ! L=70#97#E20#34JM#N#"!K=7:'!!7:2&0!&#$4#,#E240!,#$=>:&! •Algebra •Trigonometry ! ! ! ! "#$#%&'!(&)*!+,-''./! !! (#&.0%-$1/!!20'#%3!4%5)%&6)5%! 7%&8!9#6)5%.!)5!.6&'#! ! :$-).!;!<=><?+@! ! !"#$%&'#(%)*"#+(,* "#$%&'(')*+!! &'(')*+!! ,'-(#&'(')*+! &#$$#&'(')*! !! "#$%.)/&*+!! .)/&*! Algebra 1st Show Units Calculator in degrees! Right Triangles ! !"#$#%&!"#$%&'()*+!,&-./! 5'6($&1+! 78++*! ! ! 9&.(:'&%!+-6+4! Tools protractor metric ruler '(")*%&!"#$%&'()*+!$&*!*'0+1(',&/!2!,&-.!34! 5'68-$1+#+&(! ;+-,1'(.! 911+-+0$(',&! <,01+!"=+'%:(>!&,0#$-!?,01+>!+(1@/! A,#+&()#! B#8)-6+! <'+-*6!"%0$C'($(',&$->!+-+1(0'1>!#$%&+('1/! ! ! "#$%&'$&! (!)!*! +,-.*&! (!)!/0! !!12#3.!)!4(540! 6,$.'-! (!)!/0!7!8! 6,$.'-! 9:$;,-.*&<! (!)!/0!7!8! :$=.-%.! %>?'-.! ! +,-.*&! %>?'-.! ! ! ! Constant Velocity Kinematics - Motion! "#$!"%&'(!$)!*$+,$-! Uniform Acceleration Constant v=d t Forces are unbalanced Fnet ! 0, a ! 0 not in equilibrium Newton’s second law •acceleration a = ∆v t d = vit + 1/2at2 slo pe slo Distance v. time vf2 = vi2 + 2ad pe = = v a Forces are balanced Fnet = 0, a = 0 In equilibrium Newton’s first law •constant velocity Speed v. time Acceleration v. time Distance v. time Speed v. time Acceleration v. time area under line = displacement ! "#$%&'()*&+! ! ! ! ! ! Horizontal ! velocity ,-.*&!/01-'2! vx =! constant – constant speed ! Vertical – constantmotion acceleration Angle vy = accelerated Launch ! 3&#()'0*!/01-'2!!!!!!!!!!!!!!!!!!!!!!!4$#)5$-(0*!/01-'2 Horizontal Launch ! ! Components ! v -g vy +g θ v0 = vy a = g = 9.81 m/s2 vx v0 = vx v0 = vx + vy Dynamics - Forces! • 3 Laws of motion Free Body Diagrams Forces at angles FN = Fg 1. Inertia 2. a = Fnet m F newtons FA = 0. 10 Fy =? θ = 30˚ Ff = μFN 3. Action and Reaction Fx =? ax = Fx m ! N Fy = (sin θ)(F) Fx = (cos θ)(F) Fg = mg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aximum 2 ! = 00 Minimum 2 ! = 1800 FN Resultant Concurrent <2+@-!,/!7,33%'&-!(-3$&.2+.3*!!!!!!! Block on an Incline (at rest) FA Equilibrant 5 7 5 Ff θ θ 3 Fgy Fg ! Fgx ! "#$$"%!&'()!! !!!!!!!*+!,--%"%.,$#/0!12%!$/!'.,3#$45!20#$6)!78695!!!!!!!!!:/.72",)!'!;!<'87!! ! Circular Motion ! "#$%&$'(! ! )&*&$%!+#$%&$'(!,*&!#-.&/!0!*112$-3!+'#%-!4(&$2!5'&$'(!.&*#&.! ! 6$(-&$%!+#$%&$'(!,$(!5'&$'(/!$.!%'(.&*(&! ! 7*8$545!.&*&$%!+#$%&$'(!$.!9#-*&-#!&:*(!;$(-&$%!+#$%&$'(! ! v Ff = μFN Fc ac centripetal = “center seeking” • • centripetal acceleration ac = centripetal force Fc = v2 r mv2 r Momentum Gravitational Force F F p = mv Fg = G m1 m2 r2 m2 m1 (kg ⋅ m/s) J = Δp Impulse = change in momentum r Ft = Δmv mutual attraction Conservation of Momentum m1v1 = m2v2 Fg Fg Before m v = 10 m/s r direct After 5 kg 2 kg v = 0 m/s v = 0 m/s 2 kg inverse square •work elastic collision KE and p conserved Bouncy! W = Fd Joule (J) inelastic collision p conserved KE not conserved Sticky! work done change in total energy of the system F 5 =6 N Fy 55˚ W = Fxdx Fx d = 15 m •power watt (W) P = W = Fd = Fv t t 5 kg energy Waves joules Gravitational Potential Energy PE = mgΔh Spring Potential Energy PEs = 1/2kx2 F = kx k = spring constant (units: N/m) Kinetic Energy KE = 1/2mv2 PEg increases if height increases. KE increases if speed increases. PEs increases if spring is stretched or compressed. types mechanical (medium required) - sound electromagnetic (no medium required) - light energy + medium shapes longitudinal - sound ! ! ! ! transverse - water ! 2m frequency (Hz) Period (s) T = 1/f Amplitude (m) Wavelength (m) λ Conservation of Energy ET = PE + KE + Q 2m period T = 1/f ET wave speed (J) depends upon the medium! v=fλ h (J) inverse relationship between f and λ energy transformations f λ speed of sound 331 m/s speed of light 3.00 x 108 m/s Reflection Refraction law of reflection measure + draw normal θ2 Diffraction In phase (+ amplitudes) λ, 360˚ index of refraction n1 sinθ1 = n2 sinθ2 θ1 Interference ! Out of phase (- amplitudes λ/ , 180˚ 2 n1 n2 n2 = v1 = λ1 n1 v2 λ2 beats = f1 - f2 ! "#$%&'$#()*!$%'&+,#)-!(./!(0! 1#-2/!#)/(!3(4%()&)/$!,.&!/(! '&0'+3/#()!5!&+32!3(1('!2+$! $1#-2/16!,#00&'&)/!#),&7!+),!$%&&,! ! !1.&!!&),$!!&$/!8!$1(9&$/! "&,!"&$#$/$!"&0'+3/#()!8!0+$/&$/! ! Doppler Effect: change in the observed frequency due to motion Polarization Only transverse waves can be polarized – light = yes, sound = no. lower frequency higher frequency Electricity and Magnetism •electrostatics electric fields Fe = K q1q2 r2 test charges ! ! coulomb ! F F q r Law of Charges A neutral object will be attracted (never repelled) by any charged object. If two objects attract, they could have opposite charges or one could be neutral. If two objects repel, they must have the same type of charge. Elementary Charge electroscope electron = proton = 1.6 x 10-19C { Conservation of Charge If two or more identical charged spheres touch, the final charge on each is the average charge (total charge ⁄ # of spheres). The total charge is conserved. e+ ! "#$%&!'(!)*(+!,!-(!./! "#$%&!$%0%*!1*(&&/! "#$%&!&2(3!4#*%1-#($!()!)(*1%!($!&+566!7(&#-#0%!-%&-! 125*'%/! 8#%64!#&!+(&-!#$-%$&%!32%*%!)#%64!6#$%&!5*%!+(&-! 4%$&%/! Field Strength uniform electric field + E = Fe q Potential Difference - V= W q electron volts •current electricity circuit types series parallel power current I = Δq t amps watts P = VI = I2R = V2 R 12 V = 2.0Ω = 4.0Ω Ohm’s Law R = V I Rt = R1 + R2 + R3 +... ohms 1 1 1 1 Rt = R1 + R2 + R3 It = I1 = I2 = I3 . . . Vt = V1 = V2 = V3 ... resistance R= ρl A •magnetism Kirchoff’s Conservation Rules law of magnets Vt = V1 + V2 + V3 ... “short, fat, cold” = least resistance N S N-S poles It = I1 + I2 + I3 ... magnetic fields N to S compass slope = resistance ! V voltmeters/ammeters ! I A in series V in parallel "#$%&'()!*(&+,-! From N to S, density = strength (intensity) Direction of lines = direction of compass needle Modern + Nuclear Physics wave - particle duality "#$%$&'&(%)*(!+,,&(%! ! ! -.($/*.0!1#$%$.!2*,!#*0#!&.$30#! &.&)04!5!,)&63&.(4!78$9&!%#)&:#$';! ,)&63&.(4<!&=&(%:!&'&(%)$.!>!:$/&! &.&)04!.&&;&;!%$!)&'&7:&!&'&(%)$.! 2?$)@!,3.(%*$.<!>!)&/7*.*.0!&.&)04!*:! @*.&%*(!&.&)04! "#$%&#'!()*&&+,-'.! /01#&#'!"#22-3-#'34! +'+,.5!6!$#$+'&7$! *,+!)#'3+,8+9! ! energy level diagram Rutherford Model emit photon Bohr Model n=3 Ephoton = hf -.()&7:*.0!,)&63&.(4!$,!'*0#%!5! *.()&7:*.0!A+!$,!&'&(%)$.:! ! -.()&7:*.0!*.%&.:*%4!$,!'*0#%!5! *.()&7:*.0!.3/8&)!$,!&'&(%)$.:! ! "#$%$&'&(%)*(!&,,&(%!0)71#:B! C'$1&!5!"'7.(@D:!($.:%7.%! EF!*.%&)(&1%!5!F?$)@!,3.(%*$.! GF*.%&)(&1%!5!%#)&:#$';!,)&63&.(4! ! Ionization energy 1.51 eV Cloud Model n=2 3.40 eV Standard Model n=1 13.6 eV Excited state: higher energy Ephoton = Ei - Ef Ground state: lowest energy absorb photon "#$$%&!'#(%)!*+%! ,&-./0%!1#(%/%2.$345!2-$! 2-$06%+!)026%!$--!)7#//!8-&! %(%&9+#9!-:;%6$)! ! ! ! "#$%$&! '$()&%*(+! photon = “particle” of light Fundamental forces Fundamental particles electromagnetic quarks gravitational Baryons Mesons Leptons weak proton = uud [+1] strong antiproton = uud [-1] ! Mass Defect: mass of nucleus less than expected E = mc2 (kg) ____ x 931 MeV (u) fission fusion