Chapter 1 Introduction Science what is it Science

Chapter 1 Introduction

Science: what is it? • Science is a system of acquiring knowledge (research) based on 1) empiricism (dependence on observable evidence) 2) experimentation 3) methodological naturalism (ruling out recourse to the supernatural) 4) organized body of knowledge gained by such research • Scientific investigation must adhere to the scientific method, a process for evaluating empirical knowledge that explains observable events as a result of natural causes

Scientific method: what is it? • Description: information must be reliable, replicable and relevant to the inquiry • Prediction: information must be valid for past, present, and future observations of given phenomena • Control: active and fair sampling of possible occurrences, whenever possible and proper (as opposed to the passive acceptance of opportunistic data) • Falsifiability: elimination of plausible alternatives – a gradual process requiring repeated experiments by multiple researchers who must be able to replicate results in order to corroborate them

Falsifiability • This requirement is one of the most frequently contended • All hypotheses and theories are in principle subject to disproof – peer review is a must • There is a point at which there might be a consensus about a particular hypothesis or theory, yet it must in principle remain tentative • As a body of knowledge grows and a particular hypothesis or theory repeatedly brings predictable results, confidence in the hypothesis or theory increases

Measurement • We measure things (such as weight, time, length, speed, etc. ) • We use tools (rulers, clocks, speedometers, etc. ) to measure things • Measurement tools are calibrated • Calibration is in units (inches, seconds, pounds, mph’s, etc. ) • Units require standards (conventional, habitual, customary)

Modern standards • Not all quantities in nature are independent (e. g. , speed is distance per time) • Standards are created for independent (base) quantities: length, time, mass, + some other • Modern day standards should be as invariable as possible • Should be uniformly defined • Should be accessible

SI (Systéme Internacional) – most accepted international system of units • Adopted in 1971 • Is commonly known as metric system • Standard units are (there are more): 1 m (meter) for length 1 s (second) for time 1 kg (kilogram) for mass • All other SI units are defined as derivatives of the base units (e. g. , energy: 1 J (Joule) = 1 kg x 1 m 2 / s 2)

Length • SI unit – m (meter) • Initially adopted as one ten-millionth of a distance between the North pole and the equator (standard – platinum-iridium bar) • Currently - a modern standard: 1 m = the length of the path traveled by light in vacuum during a time interval of 1/299 792 458 of a second

Time • SI unit – s (second) • Historically 1 s = 1 / 8640 day • Currently - a modern standard: 1 s = the duration of 9, 192, 631, 770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the Cs 133 atom

Time • SI unit – s (second) • Historically 1 s = 1 / 8640 day • Currently - a modern standard: 1 s = the duration of 9, 192, 631, 770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the Cs 133 atom

Mass • SI unit – kg (kilogram) • Historically 1 kg – mass of 1 liter of water • Initially adopted in prototype of the kilogram was made of platinum-iridium and declared: “This prototype shall henceforth be considered to be the unit of mass” • Currently - an alternative modern standard: 1 kg = mass of C 12 atom * 1026 / 1. 99264824 (Don’t confuse mass and weight: 1 kg is the same on the Earth and on the Moon)

Scientific notation 237 000 s = = 2. 37 x 108 s = = 2. 37 E 8 s 0. 0000664 m = = 6. 64 x 10 -5 m = = 6. 64 E-5 m

SI system prefixes Factor Name Symbol 1024 yotta Y 10 -1 deci d 1021 zetta Z 10 -2 centi c 1018 exa E 10 -3 milli m 1015 peta P 10 -6 micro µ 1012 tera T 10 -9 nano n 109 giga G 10 -12 pico p 106 mega M 10 -15 femto f 103 kilo k 10 -18 atto a 102 hecto h 10 -21 zepto z 101 deka da 10 -24 yocto y Examples: 1. 25 E 4 J = 12. 5 k. J 2. 34 x 10 -10 s = 0. 234 ns

Good SI web resource: National Institute of Standards and Technology (NIST) http: //physics. nist. gov/cuu/Units/

Dimensional analysis • Technique to check the correctness of an equation • Dimensions (length, mass, time, combinations) can be treated as algebraic quantities • Both sides of equation must have the same dimensions • Limitation: cannot give numerical factors

Chapter 1 Problem 5 Newton’s law of universal gravitation is represented by where F is the gravitational force, M and m are masses, and r is a length. Force has the SI units kg ∙ m/s 2. What are the SI units of the proportionality constant G?

Conversion of units • Need to know a conversion factor • Use chain-link conversion (Check inside front cover for SI conversion factors)

Order of magnitude • Order of magnitude is the power of 10 that applies • Divide the number by the power of 10 • Compare the remaining value to 3. 162 ( ) • If the remainder is less than 3. 162, the order of magnitude is the power of 10 in the scientific notation • If the remainder is greater than 3. 162, the order of magnitude is one more than the power of 10 in the scientific notation

Uncertainty in measurements • There is uncertainty in every measurement, it is carried over through the calculations • Rules for significant figures are used to approximate the uncertainty in results • A significant figure is one that is reliably known • All non-zero digits are significant • Zeros are significant when: a) between other nonzero digits; b) after the decimal point and another significant figure; c) can be clarified by using scientific notation

Uncertainty in measurements • Accuracy is a number of significant figures • When multiplying or dividing two or more quantities, the number of significant figures in the final result is the same as the number of significant figures in the least accurate of the factors being combined • When adding or subtracting, round the result to the smallest number of decimal places of any term in the sum • If the last digit to be dropped is less than 5, drop the digit, otherwise raise the last retained digit by 1

Coordinate systems • Coordinate systems are used to describe the position of a point in space • Coordinate system consists of: 1) a fixed reference point called the origin 2) specific axes with scales and labels 3) instructions on how to label a point relative to the origin and the axes • Types of coordinate systems: Cartesian, plane polar, etc.

Coordinate systems • Cartesian (rectangular) coordinate system: x- and y- axes; points are labeled (x, y) • Plane polar coordinate system: origin and reference line are noted; point is distance r from the origin in the direction of angle θ; ccw from reference line; points are labeled (r, θ)

Brief trigonometry review • Pythagorean theorem: • To find an angle, you need the inverse function • Be sure your calculator is set appropriately for degrees or radians

Problem-solving skills

Problem-solving skills • Equations are the tools of physics – understand what they mean and how to use them • Carry through the algebra as far as possible – substitute numbers at the end

Questions?

Answers to the even-numbered problems Chapter 1 Problem 2: (a) L/T 2 (b) L

Answers to the even-numbered problems Chapter 1 Problem 8: 209 cm 2 ± 4 cm 2

Answers to the even-numbered problems Chapter 1 Problem 38: 8. 1 cm

Answers to the even-numbered problems Chapter 1 Problem 44: 8. 60 m