Lecture 3 Basics.pdf

(135 KB) Pobierz
Microsoft Word - Lecture 3 Basics.2
Physics 596
BASICS OF SCIENTIFIC WRITING II
Dr. Herbst
E. REFERENCES
In scientific papers, the “footnotes” and the bibliography are normally combined into a
reference section, which appears at the end of the manuscript. Although each journal has its own
style, there are two major approaches:
(1) numerical system used in physics and chemistry . Here each reference is given a number
such that the first reference encountered in the text is 1, etc.
(2) alphabetical system used in astronomy . Here each reference is mentioned by the last
names of the authors and the year it was published; e.g., Herbst (1985) or Phelps
& Phelps (1975) or Herbst et al. (1999)
Physical System
IN TEXT: The data were originally collected by Phelps and Phelps. 1 (or [1])
These authors later showed their earlier results to be wrong. 2 (or [2])
IN REFERENCE SECTION AT END:
1 A. Phelps and E. Phelps, J. Chem. Phys. 42 , 316 (1975)
2 A Phelps and E. Phelps Theory of Everything (Academic Press, New York, 1985), p.
342
Astronomical System
IN TEXT: Phelps and Phelps (1975) collected the original data. These data were later
shown to be incorrect (Phelps & Phelps 1985).
Notice that the references are slightly different depending upon whether they are used in an active or passive
sense.
IN REFERENCE SECTION AT END (chronological):
Phelps, A. and Phelps, E. 1975, J. Chem. Phys., 42, 316
Phelps, A. and Phelps, E. 1985, Theory of Everything , Academic Press, New York, p.
342
Variations in the above examples include the title of the journal article, and the first and last
pages of the article.
URL REFERENCES
In the physical system, just use a number in the text, and mention the URL along with the
Example:
5 http:///www.uwp….. is the web site of the Department of Physics, Univ.
In the astronomical system, if there is no author, just put the reference into the text .
Example: The Ohio State code ( http://www.physics.ohio-state.edu/~eric/ ) was used to
solve the problem.
F. NUMBERS
1. 0-10 Rule. Write out any number with absolute value between zero
and ten. For larger numbers use the numerical digits. Contrast three
days with 32 cats. Some exceptions/qualifications:
(a) Start of a sentence must be a written word. Examples: The 32
cats….. Thirty-two cats…..
(b) Use digits for mathematical expressions such as “3 orders of
magnitude” or “raised to the 4 th power.”
(c) Use digits for dimensions or samples such as “3 dimensions” or
“sample 3.”
2. Exponential Notation
Try to use expressions like 3 x 10 6 or 3 x 10(6) rather than 3(6) 3E(6),
3. Decimals vs Fractions
In general, decimals are preferred.
4. Operators
Use a space. For example, 3 + 2 = 5, rather than 3+2=5.
5. Units
Omit period and plural in abbreviation. 12.6 hr 5.3 x 10 4 s
2
authors, if they are known, or the organization responsible, in the reference section .
of Washington.
3x10^6, 3*10**6
300 yr 10 cm -1
 
INTRODUCTORY MATERIAL
Initial sentence:
Try to make is splashy but avoid too wide or too narrow a field
EXAMPLES:
Ever since the dawn of humanity, people have been interested in
The source of turbulent mixing during star formation is thought to
Have you ever heard the siren of an ambulance change its pitch
These initial sentences illustrate one purpose of the introduction: to place the topic in
context. In addition to an opening sentence on the topic itself, you can discuss the work of
previous authors and mention the history of the subject.
EXAMPLE:
First proposed by Doppler in 1842, the hypothesis was tested
There are three other functions of an introduction. They are:
(1) an explanation of the topic. State it as clearly as possible and state
what special portion you may be considering.
EXAMPLE:
change in frequency and wavelength of a wave as perceived by an
observer moving relative to the source of the waves .
(2) the definition of any new terms and concepts
EXAMPLE:
for a system that is exponentially sensitive to initial conditions.
(3) to provide some sense of the rest of the paper (THESIS STATEMENT)
EXAMPLES:
In the rest of the paper, we will consider the relativistic treatment of
The Doppler Effect, as treated in elementary text books, does not
take into account the special theory of relativity, the importance
of which cannot be emphasized too strongly. (gives the sense that
this topic will be emphasized but not exclusively)
3
of vision.
the Doppler effect. (too broad)
Be instability of density wave fluctuations. 1 (too narrow)
as it drove by you?
for sound waves in 1845.
Named after Christian Doppler, the Doppler effect relates the
Turbulence occurs when a liquid flow becomes chaotic, a term
The Doppler Effect for the case of light waves. (rather pedantic)
OUTLINE EXAMPLE: SCHROEDINGER AND THE BIRTH OF QUANTUM
MECHANICS
I. INTRODUCTION
(A) Physics at the turn of the twentieth century ( the context)
(B) Successes of classical physics (explanation)
(C) Few failures, including black body spectrum (“ultraviolet catastrophe”) and atomic
spectra ( explanation, definition)
(D) Need for quantum mechanics (thesis statement)
II. THE OLD QUANTUM THEORY (1900-1925)
(A) Work of Planck and Einstein
(B) The Bohr atomic model
(C) de Broglie’s matter-wave hypothesis
(D) Heisenberg and matrix mechanics
III. THE SCHROEDINGER EQUATION
(A) Motivation
(B) Equation and definition of symbols
(C) An example of a solution – the harmonic oscillator
IV. CURRENT ROLE IN PHYSICS
V. THE FUTURE – DO WE KNOW EVERYTHING?
4
OUTLINE EXAMPLE: STAR FORMATION
I. INTRODUCTION
(A) What is a star, and where are they located? (explanation) .
(B) Stars are formed by collapse of portions of interstellar clouds (context)
(C) Interstellar Matter (explanation, context, definition)
(1) clouds of gas and dust
(2) nature of gas and how studied
(3) nature of dust and how studied
(4) heterogeneity of giant clouds
(D) Formation of stars by collapse of dense cold portions of clouds (thesis)
II. STAGES OF SINGLE STAR FORMATION
(A) Cold starless cores
(B) Pre-stellar cores (central isothermal collapse)
(C) Protostars (adiabatic collapse)
(D) Hot cores of organic molecules
(E) Protoplanetary disks (low-mass case)
(F) Photon-dominated regions (high-mass case)
(G) Formation of planets in disks
III. HOW DO MULTIPLE STAR SYSTEMSS FORM?
IV. THE FUTURE AND WHAT REMAINS TO BE EXPLORED?
(A) New telescopes and high spatial resolution
(B) Detection of terrestrial exo-planets
(C) Detection of non-terrestrial life
5
Zgłoś jeśli naruszono regulamin