Class-XI Physics

JEE PYQs MCQs

  • To convert a physical quantity from one system of units to other system of units:
    \(
    n_2=n_1 \frac{u_1}{u_2}=n_1\left[\frac{\mathrm{M}_1}{\mathrm{M}_2}\right]^a\left[\frac{\mathrm{~L}_1}{\mathrm{~L}_2}\right]^b\left[\frac{\mathrm{~T}_1}{\mathrm{~T}_2}\right]^c
    \)
  • Some of the commonly used systems of units are as follows
    (i) CGS system: In this system, the units of length, mass and time are centimetre (cm), gram (g) and second (s), respectively. The unit of force in this system is dyne and that of work or energy is erg.
    (ii) FPS system: In this system, the units of length, mass and time are foot (ft), pound (lb) and second (s), respectively. The unit of force in this system is poundal.
    (iii) MKS system: In this system, the units of length, mass and time are metre (m), kilogram (kg) and second (s), respectively. The unit of force in this system is newton (N) and that of work or energy is joule (J).
    (iv) International system (SI): This system of units helps in revolutionary changes over the MKS system and is known as rationalised MKS system. It is helpful to obtain all the physical quantities in physics.
  • Those physical quantities which are independent of each other and not defined in terms of other physical quantities, are called fundamental quantities or base quantities. The units of these quantities are called fundamental or base units.
  • The quantities which can be expressed in terms of the fundamental quantities are called derived quantities. The units of these quantities are called derived units.
  • Rules to determine significant figures
    For determining number of significant figures, we use the following rules
    Rule 1: All non-zero digits are significant, e.g. \(x=2567\) has four significant figures.
    Rule 2: The zeros appearing between two non-zero digits are significant, no matter where the decimal point is, if at all, e.g. 6.028 has 4 significant figures.
    Rule 3: If the number is less than 1 , the zero(s) on the right of decimal point but to the left of first non-zero digit are not significant.
    e.g. 0.0042 has two significant digits.
    Rule 4: The terminal or trailing zero(s) in a number without a decimal point are not significant. Thus, \(426 \mathrm{~m}=42600 \mathrm{~cm} =426000 \mathrm{~mm}\) has three significant figures.
    Rule 5 In a number with decimal, zeros to the right of last non-zero digit are significant.
    e.g. 4.600 or 0.002300 have four significant figures each.
  • Addition or subtraction:
    Suppose in the measured values to be added or subtracted, the least number of significant digits after the decimal is \(n\). Then, in the sum or difference also, the number of significant digits after the decimal should be \(n\).
  • Multiplication or division:
    Suppose in the measured values to be multiplied or divided, the least number of significant digits be \(n\), then in the product or quotient, the number of significant digits should also be \(n\).
    Rules for rounding off a measurement:
  • Following are the rules for rounding off a measurement:
    Rule 1: If the number lying to the right of cut-off digit is less than 5 , then the cut-off digit is retained as such. However, if it is more than 5 , then the cut-off digit is increased by 1. e.g. \(x=6.24\) is rounded off to 6.2 to two significant digits and \(x=5.328\) is rounded off to 5.33 to three significant digits.
    Rule 2: If the insignificant digit to be dropped is 5 , then the rule is
    (i) if the preceding digit is even, the insignificant digit is simply dropped.
    (ii) if the preceding digit is odd, the preceding digit is raised by 1 .
    e.g. \(x=6.265\) is rounded off to \(x=6.26\) to three significant digits and \(x=6.275\) is rounded off to \(x=6.28\) to three significant digits.
    Rule 3: The exact numbers like \(\pi, 2,3\) and 4, etc., that appear in formulae and are known to have infinite significant figures, can be rounded off to a limited number of significant figures as per the requirement.
  • Error \(=\) True value – Measured value
  • Absolute error: The difference between the true value and the measured value of a quantity is called an absolute error. Usually the mean value \(a_m\) is taken as the true value. So, if
    \(
    a_m=\frac{a_1+a_2+\ldots+a_n}{n}=\frac{1}{n} \sum_{i=1}^n a_i
    \)
    Then by definition, absolute errors in the measured values of the quantity are
    \(
    \begin{gathered}
    \Delta a_1=a_1-a_m \\
    \Delta a_2=a_2-a_m \\
    \vdots \\
    \vdots \\
    \Delta a_n=a_n-a_m
    \end{gathered}
    \)
    Absolute error may be positive or negative.
    Mean absolute error It is the arithmetic mean of the magnitudes of absolute errors. Thus,
    \(
    \Delta a_{\text {mean }}=\frac{\left|\Delta a_1\right|+\left|\Delta a_2\right|+\ldots+\left|\Delta a_n\right|}{n}=\frac{1}{n} \sum_{i=1}^n\left|\Delta a_i\right|
    \)
    Thus final result of measurement can be written as
    \(
    a=a_m \pm \Delta a_{\text {mean }}
    \)
    This implies that value of \(a\) is likely to lie between \(a_m+\Delta a_{\text {mean }}\) and \(a_m-\Delta a_{\text {mean }}\).
  • Relative or fractional error: The ratio of mean absolute error to the mean value of the quantity measured is called relative or fractional error.
    Thus, \(\quad\) Relative error \(=\frac{\Delta a_{\text {mean }}}{a_m}\)
    Percentage error When the relative error is expressed in percent, it is called percentage error. It is denoted by \(\delta a\).
    Thus, \(\quad \delta a=\frac{\Delta a_{\text {mean }}}{a_m} \times 100 \%\)
  • Error in sum or difference: Let \(x=a \pm b\):
    \(
    \Delta x= \pm(\Delta a+\Delta b)
    \)
  • Error in product: Let \(x=a b\):
    \(
    \frac{\Delta x}{x}= \pm\left(\frac{\Delta a}{a}+\frac{\Delta b}{b}\right)
    \)
  • Error in division: Let \(x=\frac{a}{b}\):
    \(
    \frac{\Delta x}{x}= \pm\left(\frac{\Delta a}{a}+\frac{\Delta b}{b}\right)
    \)
  • Error in quantity raised to some power:
    Let \(x=\frac{a^n}{b^m}\)
    \(
    \frac{\Delta x}{x}= \pm\left(n \frac{\Delta a}{a}+m \frac{\Delta b}{b}\right)
    \)

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