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Backgrounds, and Font, Size, Color, & Style. Bulleted/enumerated lists ... Molecular Beam Epitaxy (MBE): Self Assembly. Picture of MBE/STM. in situ STM of Dots ... – PowerPoint PPT presentation

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Title: YOUR TITLE GOES HERE


1
YOUR TITLE GOES HERE
Capstone Talk PHYS 4300
  • Date
  • Author
  • Advisor
  • Acknowledgements

2
Outline
  • Motivation
  • Background
  • e.g. Maxwells Equations
  • e.g. Relativistic Corrections
  • Viewgraph Formatting
  • Power Point Tricks
  • Backgrounds, and Font, Size, Color, Style
  • Bulleted/enumerated lists and hierarchy
  • Images, Graphs, Schematics, and Cartoons
  • The Perfect Viewgraph
  • Conclusions
  • Appendix Prof. John Wilkins Rules for Physics
    Talks

3
Motivation
  • Make it simple and interesting -lose them here
    and they are gone for good.
  • General Motivation
  • save the known world
  • Specific
  • Graphics are important here

4
Background
Know your audience! use this to get them up to
speed.
  • Maxwells Equations
  • Use equation editor for simple equation or import
    as objects from pdf etc. or cut and paste using
    ltPrint Screengt
  • Relativistic Corrections

5
Viewgraph Formatting
  • Font
  • Size - depends on room
  • Color - depends on background
  • Style - font, italics, bold, shadow, underline
    etc.
  • Backgrounds keep them simple
  • Bulleted/enumerated lists and hierarchy
  • Images, Graphs, Schematics, and Cartoons
  • The Perfect Viewgraph

6
Background 1 Good
7
Background 2 Bad
8
Background 2 Ugly
9
Viewgraph Formatting Font Size
  • Depends on room and on font
  • Can you read me now? (36)
  • Can you read me now? (32)
  • Can you read me now? (28)
  • Can you read me now? (24)
  • Can you read me now? (20)
  • Can you read me now? (18)
  • Can you read me now? (16)
  • Can you read me now? (14)
  • Can you read me now? (12)
  • Can you read me now? (10)

10
Colors
Can you read me Now? Can you read me Now? Can you
read me Now? Can you read me Now? Can you read me
Now? Can you read me Now? Can you read me Now?
Can you read me Now?
Can you read me Now? Can you read me Now? Can you
read me Now? Can you read me Now? Can you read me
Now? Can you read me Now? Can you read me Now?
Can you read me Now?
Can you read me Now? Can you read me Now? Can you
read me Now? Can you read me Now? Can you read me
Now? Can you read me Now? Can you read me Now?
Can you read me Now?
Readability depends heavily on the actual output
device used.
11
ON VIEWGRAPH FONTS TNR 40
Tools for Clarity TNR 28
  • Hierarchy is crucial. TNR 24
  • Group ideas logically, but be consistent. TNR
    20
  • This adds needed order to a viewgraph. TNR 16
  • But too much hierarchy is confusing. TNR 14
  • For example, can you read this? TNR 14, 12, 10
  • Colour too is useful. TNR 24
  • Be consistent within and between viewgraphs. TNR
    20
  • But to not be frivolous. TNR 16
  • Over use of colour is distracting. TNR 14
  • And some colours really do not work well. TNR 14
  • Other tricks include distinctive fonts and
    highlighting. TNR 24
  • Italics, bold, underlined, shadow and
    combinations? Be consistent TNR 20
  • And do not over use. TNR 16
  • For this can be very distracting Arial16, To
    say the least Alg..D 16
  • Too much of this is bad.

12
ON VIEWGRAPH FONTS TNR 40
Tools for Clarity TNR 28
  • Hierarchy is crucial. TNR 24
  • Group ideas logically, but be consistent. TNR
    20
  • This adds needed order to a viewgraph. TNR 16
  • But too much hierarchy is confusing. TNR 14
  • For example, can you read this? TNR 14, 12, 10
  • Colour too is useful. TNR 24
  • Be consistent within and between viewgraphs. TNR
    20
  • But to not be frivolous. TNR 16
  • Over use of colour is distracting. TNR 14
  • And some colours really do not work well. TNR 14
  • Other tricks include distinctive fonts and
    highlighting. TNR 24
  • Italics, bold, underlined, shadow and
    combinations? Be consistent TNR 20
  • And do not over use. TNR 16
  • For this can be very distracting Arial16, To
    say the least Alg..D 16
  • Too much of this is bad.

13
Demonstration PowerPoint
  • Use the predefined blank.pot
  • Bulleted items are formatted correctly
  • you must use the Title and Text layout to get
    this bullet layout
  • Addition bulleted text boxes should be a copy of
    this
  • Go no deeper than this (and this is too deep)
  • Keep text above 16 points (18 preferred) if you
    want the audience to be able to read the text
  • Group graphical objects together as it makes it
    easier to modify the layout
  • Use multiple groupings
  • text and arrow
  • text and scale bar
  • Etc.
  • Then group the groups to have a composite drawing
  • Name your PowerPoint Well DescriptiveTitle-YearMo
    nthDate.ppt
  • i.e. DemonstrationPowerPoint-20050610.ppt

14
Power Point Tricks
  • Use Master Page it does save time!
  • I like Font size to be defined by me, and the
    text box to fit around it.
  • ltRight Clickgt ltFormat Place Holder..gt ltText Boxgt
    ltResize Autoshape ..gt
  • Tricks to minimize white space.
  • Use ltViewgt ltRulergt to minimize bullet-text
    separation
  • Use ltFormatgt ltLine Spacinggt - minimum settings
    of 0.85 line and 0.15 before/after works.
  • Maximize figure size. ltCopygt ltPaste Special, as
    Picture pnggt Very useful.
  • If bulleted item is gt 2 lines you are probably
    being too verbose.
  • For graphs, when you create the plots using
    whatever software package, use sensible colors
    (e.g. Bl R G B, and stay consistent!), thick
    enough lines, and large enough fonts.
  • Fonts be sensible Arial is clean and Times New
    Roman dense.
  • Graphics need a title and caption!
  • Stealing graphics on the web ltPrint Screengt,
    ltPastegt and crop! But you must cite best cite
    below the figure.

15
Death of a Star
  • Nuclear fusion in stars core
  • Occurs in phases
  • Massive stars ( gt 8 Msun) burn to Fe peak
    elements
  • Fe core collapses
  • Energetic explosion
  • Supernova
  • Remnant is neutron star or black hole

16
Death of a Star
  • Nuclear fusion in stars core
  • Occurs in phases
  • Massive stars ( M gt 8 Msun) burn to Fe peak
    elements
  • Fe core collapses
  • Energetic explosion
  • Supernova
  • Remnant is neutron star or black hole

17
Aug. 21 -10 days (before max light)
  • Again, higher metallicity makes better 6200Ã…
    feature
  • Quality of fit roughly the same for both models

18
Aug. 21 -10 days (before max light)
  • Again, higher metallicity makes better 6200Ã…
    feature
  • Quality of fit roughly the same for both models

19
Mass Spectrometry
  • We use Isotopic Mass Spectrometry to detect
    isotopologues (or isotopomers) in a given gas
    sample
  • In Mass Spectrometry, a sample is prepared,
    injected, and borne via an inert carrier gas
    (He) through a catalytic oven into an ionization
    source, where the gas particles are ionized via
    electron impact
  • These ions are then accelerated through a high
    voltage static potential, into a magnetic field,
    which bends the ions into a circular path by
    mass
  • A series of sequential Faraday cup detectors then
    detect the ionized particles, thus detecting the
    isotopologues
  • For our experiment, we used a Thermo Scientific
    Delta V Isotope Mass Spectrometer, outputting
    all ion currents into the Isodat Acquisition
    program

20
What is Mass Spectrometry?
  • Mass spectrometry takes an ionized sample and
    differentially separates it by mass-to-charge
    ratio (m/z)
  • Developed by JJ Thompson in 1897
  • 1906 Nobel Prize
  • Three common elements to all modern mass
    spectrometers
  • Ionization Source (converts sample particles)
  • Mass analyzer Deflects charged particles
    according to Lorentz Force Law and Newtons
    Second Law (m/z)aE(v x B)
  • Ion currents detected
  • Limitation Some compounds have same mass

21
What is Mass Spectrometry?
  • Mass spectrometry (MS) takes an ionized sample
    and separates it by mass-to-charge ratio (m/z)
  • e.g. z1 for singly ionized species, m is mass of
    ion in atomic mass units AMU.
  • Brief history
  • Pioneered by J.J. Thomson in the early 1900s
  • First full MS demonstrated by William Aston
    (1922 Nobel Prize)
  • First modern MS demonstrated by A.J. Dempster
    (circa 1920)
  • Three elements in modern Mass Specs
  • Ionization Source ionize gas molecules and
    accelerates ions
  • Mass analyzer Deflects charged particles
    according to Lorentz Force Law
  • Detector
  • Limitation Some ions have same mass
  • e.g. CO (m121628) AMU and N2 (M21428).

Detector Single slit or array
Mass Analyzer Sector Magnet (uniform B)
B
Ions deflected in arc radius R Solving for v in
(1), inserting into (2) and rearranging,

Ion Source Accelerate through V
22
What is Mass Spectrometry?
Detector Single slit or array
  • Mass spectrometry (MS) takes an ionized sample
    and separates it by mass-to-charge ratio (m/z)
  • e.g. z1 for singly ionized species, m is mass of
    ion in atomic mass units AMU.
  • Brief history
  • Pioneered by J.J. Thomson in the early 1900s
  • First full MS demonstrated by William Aston
    (1922 Nobel Prize)
  • First modern added sector magnet MS
    demonstrated by A.J. Dempster (circa 1920)
  • Three elements in modern Mass Specs
  • Ionization Source ionize gas molecules and
    accelerates ions
  • Mass analyzer Deflects charged particles
    according to Lorentz Force Law
  • Detector Detects ion currents
  • Limitation Some ions have same mass
  • e.g. CO (m121628) AMU and N2 (M21428).

Mass Analyzer Sector Magnet (uniform B)
B
v
Ion Source Accelerate through V
  • Schematic of Mass Spec.
  • R of ion trajectories only dependent on (m/z) for
    given V and B
  • Typically set V and scan B to scan through (m/z)

23
SWNT Thin Films
  • Combine electrical and optical properties
  • Potential Applications
  • Transparent Electrodes
  • LCDs
  • Touch Screens

24
Single-Wall Nanotube Thin Films
  • Combine electrical and optical properties
  • Potential Applications
  • Transparent Electrodes
  • LCDs and Touch Screens

Transmission vs. l for SWNTs Deposited from
Various Solutions
Scanning Electron Microscope (SEM) image of SWNTs
deposited on to glass
25
Core Collapse SN Types Ib, Ic, and II
  • (a) A massive star has evolved an iron core by
    fusing silicon.
  • (b) once the iron core reaches the Chandrasekhar
    limit, it begins to collapse. The outer core is
    represented by black arrows and the inner core by
    white. Black arrows are moving supersonically
    and white are moving subsonically.
  • (c) the inner core is compressed into neutrons
    while the gravitational potential energy is
    converted and released in a neutrino burst.

26
Core Collapse SN Types Ib, Ic, and II
  • (d) material that is still falling inwards (black
    arrows, outer core) bounces off the dense core
    and creates a shock wave which propagates
    outwards, represented by the red arrows.
  • (e) the shock slows down as energy is used up by
    nuclear processes, but neutrino interaction keeps
    it going.
  • (f) outside of the inner core, the material is
    ejected and only a degenerate core remnant is
    left behind.

27
Core Collapse SN Types Ib, Ic, and II
  • a. A massive star has evolved an iron core by
    fusing silicon.

b. Once iron core reaches the Chandrasekhar
limit, it begins to collapse. (outer core is
shown as ? inner core ? by white. Black
arrows are ? move supersonically and ? move
subsonically.
c. Inner core is compressed into neutrons while
the gravitational potential energy is converted
and released in a neutrino burst.
d. Material that is still falling inwards ( ?,
outer core) bounces off the dense core and
creates a shock wave which propagates outwards (
?, red arrows).
e. Shock slows down as energy is used up by
nuclear processes, but neutrino interaction keeps
it going.
f. Outside of the inner core, the material is
ejected and only a degenerate core remnant is
left behind.
28
Molecular Beam Epitaxy(MBE) Self Assembly
  • Picture of MBE/STM

in situ STM of Dots
29
Anodized Aluminum Oxide Masks
  • Tunable diameters 20 to 500 nm
  • Ordered micron-sized domains

30
Conclusions
  • Often a summary and conclusions
  • Future
  • What will be done on the project after you
    leave/graduate

31
Prof. John Wilkins Rules for Physics Talks
  • Rules for preparing talk/viewgraphs
  • Decide on take-home message.What do you want
    listeners to carry away? Design talk to that aim.
  • Pick figures and illustrations that deliver
    take-home message.
  • On each viewgraph, put
  • Title that summarize subject of viewgraph.
  • Carefully formulated argument.
  • Conclusion of argument at bottom of viewgraph.
  • Practice for
  • Length. Shorter is better.
  • Connectivity. Cleanly segue from one viewgraph to
    the next.
  • Clarity . Formulate your ideas accurately and
    concisely.
  • Segue
  • To move smoothly and unhesitatingly from one
    state, condition, situation, or element to
    another.
  • "Daylight segued into dusk" - Susan Dworski.
  • How do the world's most celebrated adolescents
    sc. the Rolling Stones segue into middle age?
  • http//www.physics.ohio-state.edu/wilkins/writing
    /
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