Mcat Physics Formula Sheet

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mcat physics formula sheet is an essential resource for students preparing for the Medical College Admission Test (MCAT). Mastering physics concepts and formulas is crucial for achieving a high score in this section. A well-organized MCAT physics formula sheet helps streamline your study process, reinforce key principles, and improve your problem-solving efficiency. This comprehensive guide provides a detailed and structured overview of the most important physics formulas you need to know, categorized by topic, to help you excel on the exam.

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Importance of a Physics Formula Sheet for MCAT Preparation

Before diving into the formulas, it's important to understand why having a dedicated formula sheet is beneficial:

- Quick Reference: Allows rapid access to formulas during practice and review sessions.
- Memory Reinforcement: Repetition helps memorize key formulas.
- Conceptual Clarity: Organizing formulas by topics clarifies connections between concepts.
- Exam Strategy: Familiarity with formulas can speed up problem-solving during the test.

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Core Topics Covered in the MCAT Physics Formula Sheet

The MCAT physics section encompasses various fundamental topics. The following categories summarize the key formulas:

- Kinematics
- Dynamics (Newton’s Laws)
- Work and Energy
- Momentum
- Circular Motion and Gravitation
- Fluids
- Thermodynamics
- Electrostatics
- Magnetism
- Waves and Sound
- Light and Optics

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Kinematics Formulas

Kinematics deals with motion without considering forces.

Basic Kinematic Equations

1. Velocity-Time Relation
\[ v = v_0 + a t \]
Where:
- \( v \): final velocity
- \( v_0 \): initial velocity
- \( a \): acceleration
- \( t \): time

2. Displacement
\[ x = v_0 t + \frac{1}{2} a t^2 \]

3. Velocity-Displacement Relation
\[ v^2 = v_0^2 + 2 a x \]

4. Average Velocity
\[ v_{avg} = \frac{v_0 + v}{2} \]

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Dynamics and Newton’s Laws

Foundation of mechanics describing how forces affect motion.

Newton’s Second Law

\[ F_{net} = m a \]
Where:
- \( F_{net} \): net force
- \( m \): mass
- \( a \): acceleration

Weight

\[ W = m g \]
Where:
- \( g \): acceleration due to gravity (~9.8 m/s²)

Frictional Forces

- Static Friction:
\[ F_{s} \leq \mu_{s} F_{N} \]
- Kinetic Friction:
\[ F_{k} = \mu_{k} F_{N} \]

Where:
- \( \mu_{s} \), \( \mu_{k} \): coefficient of static and kinetic friction
- \( F_{N} \): normal force

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Work, Power, and Energy

Understanding energy transfer and conservation principles.

Work

\[ W = F d \cos \theta \]

Kinetic Energy

\[ KE = \frac{1}{2} m v^2 \]

Potential Energy

- Gravitational Potential Energy
\[ PE_{grav} = m g h \]
- Elastic Potential Energy (spring)
\[ PE_{spring} = \frac{1}{2} k x^2 \]

Where:
- \( k \): spring constant
- \( x \): displacement from equilibrium

Work-Energy Theorem

\[ W_{net} = \Delta KE \]

Power

\[ P = \frac{W}{t} = F v \]
Average power during work done at constant velocity.

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Momentum and Collisions

Principles governing the motion of objects during interactions.

Linear Momentum

\[ p = m v \]

Impulse

\[ J = F \Delta t = \Delta p \]

Conservation of Momentum

\[ m_1 v_{1i} + m_2 v_{2i} = m_1 v_{1f} + m_2 v_{2f} \]

Collisions

- Elastic Collisions (both momentum and kinetic energy conserved)
- Inelastic Collisions (momentum conserved, kinetic energy not conserved)

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Circular Motion and Gravitation

Focus on objects moving in circles and gravitational forces.

Centripetal Force

\[ F_{c} = \frac{m v^2}{r} \]

Period and Frequency

\[ T = \frac{2 \pi r}{v} \]

\[ f = \frac{1}{T} \]

Universal Law of Gravitation

\[ F_{grav} = G \frac{m_1 m_2}{r^2} \]

Where:
- \( G \): gravitational constant (~6.674×10⁻¹¹ N·m²/kg²)

Orbital Velocity

\[ v_{orb} = \sqrt{\frac{G M}{r}} \]

Where:
- \( M \): mass of central object

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Fluids

Principles of fluids at rest and in motion.

Density and Specific Weight

\[ \rho = \frac{m}{V} \]
\[ \gamma = \rho g \]

Pressure

\[ P = P_0 + \rho g h \]
Or for liquids at depth \( h \):

\[ P = P_{atm} + \rho g h \]

Buoyant Force (Archimedes’ Principle)

\[ F_b = \rho_{fluid} g V_{displaced} \]

Continuity Equation

\[ A_1 v_1 = A_2 v_2 \]

Bernoulli’s Equation

\[ P_1 + \frac{1}{2} \rho v_1^2 + \rho g h_1 = P_2 + \frac{1}{2} \rho v_2^2 + \rho g h_2 \]

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Thermodynamics

Energy transfer involving heat and work.

Specific Heat

\[ Q = mc \Delta T \]

Heat Transfer

- Conduction:
\[ Q = \frac{k A \Delta T}{d} t \]
- Convection and Radiation involve more complex formulas but are essential in understanding heat transfer.

First Law of Thermodynamics

\[ \Delta U = Q - W \]

Where:
- \( \Delta U \): change in internal energy
- \( Q \): heat added
- \( W \): work done by system

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Electrostatics

For the physics of stationary charges.

Coulomb’s Law

\[ F = k_e \frac{|q_1 q_2|}{r^2} \]

Where:
- \( k_e \): Coulomb’s constant (~8.988×10⁹ N·m²/C²)

Electric Field

\[ E = \frac{F}{q} = k_e \frac{|q|}{r^2} \]

Electric Potential Energy

\[ U = k_e \frac{q_1 q_2}{r} \]

Electric Potential (Voltage)

\[ V = \frac{U}{q} \]

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Magnetism

Magnetic forces and fields.

Magnetic Force on a Moving Charge

\[ F = q v B \sin \theta \]

Magnetic Force on a Current-Carrying Wire

\[ F = I L B \sin \theta \]

Magnetic Field of a Long, Straight Wire

\[ B = \frac{\mu_0 I}{2 \pi r} \]

Where:
- \( \mu_0 \): permeability of free space (~4π×10⁻⁷ T·m/A)

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Waves and Sound

Properties of wave motion and sound.

Wave Speed

\[ v = f \lambda \]

Frequency

\[ f = \frac{v}{\lambda} \]

Sound Intensity Level

\[ \beta = 10 \log_{10} \left( \frac{I}{I_0} \right) \]

Where:
- \( I_0 \): reference intensity (10⁻¹² W/m²)

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Light and Optics

Behavior of light, reflection, refraction, and lenses.

Snell’s Law

\[ n_1 \sin \theta_1 = n_2 \sin \theta_2 \]

Lens Formula

\[ \frac{1}{f} = \frac{1}{d_o} + \frac{1}{d_i} \]

Where:
- \( f \): focal length
- \( d_o \): object distance
- \( d_i \): image distance

Magnification

\[ M = \frac{h_i}{h_o} = -\frac{d_i}{d_o} \]

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Additional Tips for Using Your MCAT Physics Formula Sheet

- Customize your sheet by adding any formulas you find challenging.
- Practice solving problems using only your formula sheet to simulate test conditions.
- Regularly review and update your sheet as you learn new concepts.
- Use visual aids like diagrams or mnemonics for complex formulas.

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Conclusion

A well-structured MCAT physics formula sheet is an indispensable tool for mastering the exam content. By organizing formulas logically and understanding their applications, students can improve their problem-solving speed and

Frequently Asked Questions


What are the most essential physics formulas to include on an MCAT physics formula sheet?

Key formulas include kinematic equations, Newton's laws, conservation of energy, momentum equations, electrostatics formulas (Coulomb's law), and basic wave and optics equations such as the speed of a wave and lens/mirror formulas.

How can I effectively organize my MCAT physics formula sheet?

Group formulas by topic—motion, forces, energy, momentum, fluids, electricity, and waves—using clear headings and color coding to facilitate quick reference during study and practice exams.

Are there any common mistakes to avoid when creating a physics formula sheet for the MCAT?

Yes, ensure all formulas are accurate, include units, and avoid cluttering the sheet with unnecessary information. Focus on formulas you frequently forget or find challenging, and double-check for common errors or variations.

Is it better to memorize all formulas or understand their derivations for the MCAT physics section?

While understanding derivations aids deeper comprehension, for the MCAT, focus on memorizing key formulas and their applications, as the exam emphasizes problem-solving over derivation.

Can I include cheat sheets or notes on my MCAT physics formula sheet?

Official MCAT guidelines prohibit bringing external notes or cheat sheets into the exam. However, creating a concise, personal formula sheet for study purposes is highly effective for retention and quick reference during practice.

How often should I review my MCAT physics formula sheet during my preparation?

Regular review—weekly or biweekly—helps reinforce memory. Incorporate quick revision sessions into your study routine to ensure formulas become second nature before test day.