Physics GRE

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Flashcards to study for the 2026 Physics GRE

Last updated 1:37 AM on 9/13/26
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59 Terms

1
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period for a simple pendulum

T=2πLgT = 2\pi\sqrt{\frac{L}{g}}

2
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relativistic gamma

γ=11(v/c)2\gamma = \frac{1}{\sqrt{1 - (v/c)²}}

3
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Relativistic energy

E2=(pc)2+(mc2)2=γmc2E² = (pc)² + (mc²)² = \gamma mc²

4
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Equivalent resistance for two resistors in series

Req=R1+R2R_{eq} = R_1 + R_2

5
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Equivalent resistance for two resistors in parallel

1Req=1R1+1R2\frac{1}{R_{eq}}=\frac{1}{R_1}+\frac{1}{R_2}

6
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Ohm’s law

V=IRV = IR

7
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Photoelectric effect relation

Kmax=hνϕK_{max} = h\nu - \phi

8
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ground state energy of a particle confined in an infinite square well of length aa

h28ma2\frac{h²}{8ma²}

9
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velocity of light within a nonmagnetic dielectric material

v=cϵv = \frac{c}{\sqrt{\epsilon}}

10
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orbital period of a planet around a star

T=4π2r3GMT = \sqrt{ \frac{4\pi²r³}{GM}} , rr is the radius of the orbiting body to the star, MM is the mass of the central body

11
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velocity of an orbiting body

vorbit=GMrv_{orbit} = \sqrt{ \frac{GM}{r}}

12
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angular momentum

L=IωL = I\omega or L=r×pL = \vec{r} \times \vec{p}

13
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relationship between angular velocity and linear velocity

v=ωRv = \omega R

14
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cyclotron frequency

ω=qBm\omega = \frac{qB}{m}

15
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quantum efficiency

QE=number of photons detectednumber of incident photonsQE = \frac{\text{number of photons detected}}{\text{number of incident photons}}

16
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error propagation for z=xnz=x^{n} , where xx is the measured value

Δzz=nΔxx\frac{\Delta z }{z} = |n| \frac{\Delta x}{x} , i.e. multiply the relative uncertainty by nn

17
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Hooke’s law

F=kΔxF = -k\Delta x

18
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energy stored in a displaced spring

U=12kx2U = \frac{1}{2} k x²

19
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resolving power of grating spectrometer

P=λΔλP = \frac{ \lambda}{\Delta \lambda}

20
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What equation would you use to calculate the index of refraction for a gas in a Michelson interferometer?

2d(n1)=mλ2d(n-1) = m \lambda

dd = path length

nn = index of refraction

mm = number of fringes counted

λ\lambda = laser wavelength

21
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What are the Pauli spin matrices?

σx=(0110)\sigma_x = \begin{pmatrix} 0 & 1 \\ 1 & 0\end{pmatrix} , σy=(0ii0)\sigma_y = \begin{pmatrix} 0 & -i \\ i & 0 \end{pmatrix} , σz=(1001)\sigma_z = \begin{pmatrix} 1 & 0 \\ 0 & -1 \end{pmatrix}

22
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binding energy per nucleon

binding energy per nucleon=Δmc2A\text{binding energy per nucleon} = \frac{\Delta m \cdot c²}{A} ,

Δm(mass defect)=(Zmp+Nmn)mnucleus\Delta m \text{(mass defect)} = (Z \cdot m_p + N \cdot m_n ) - m_{nucleus}

AA = mass number

23
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What are fermions?

Half-integer spin (1/2, 3/2, etc.) particles including leptons and quarks.

24
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What are leptons?

The class of particles (specifically fermions) which includes the electron (ee^-), negative muon (μ\mu^-), and tau (τ\tau^-) particles and their respective neutrinos (νe,νμ,ντ\nu_e,\nu_\mu,\nu_\tau).

25
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What are hadrons?

Hadrons are the composite subatomic particles made of quarks and antiquarks. The subclasses of hadrons are the mesons and baryons.

26
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What are mesons?

Short-lived particles made from a quark-antiquark pair.

27
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What are baryons?

Composite subatomic particles composed of three quarks. Protons and neutrons are both baryons.

28
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What are bosons?

Integer spin subatomic particles that typically carry the fundamental forces. They do not obey the Pauli exclusion principle.

29
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Gauss’s law for electricity

E=ρϵ0\nabla \cdot E = \frac{\rho}{\epsilon_0}

30
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Gauss’s law for magnetism

B=0\nabla \cdot B = 0

31
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Faraday’s law of induction

×E=Bt\nabla \times E = -\frac{\partial B}{\partial t}

32
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Ampere-Maxwell’s law

×B=μ0J+μ0Et\nabla \times B = \mu_0 J + \mu_0 \frac{\partial E}{\partial t}

33
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[x^,p^][\hat{x}, \hat{p}] = ?. What does it mean for the commutator of two operators to be zero?

[x^,p^]=i[\hat{x}, \hat{p}] = i \hbar

If [A^,B^]=0[ \hat{A}, \hat{B} ] = 0, then the observables AA and BB can be measured simultaneously without uncertainty.

34
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Heisenberg’s uncertainty relation (What is the uncertainty bound of σxσp\sigma_x\sigma_p?)

σxσp2\sigma_x\sigma_p \ge \frac{\hbar}{2}

35
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What is the general (time-dependent) Schrödinger equation?

Eψ(x,t)=H^ψ(x,t)E \psi(x,t) = \hat{H} \psi(x,t)

itψ(x,t)=(p^22m+V^(x))ψ(x,t)i\hbar\frac{\partial}{\partial t}\psi(x,t)=\Big(\frac{\hat{p}^{2}}{2m}+\hat{V}(x)\Big)\psi(x,t)

36
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What are the position and momentum operators?

x^=x,p^=ix\hat{x} = x, \hat{p} = -i\hbar \frac{\partial}{\partial x}

37
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What is the definition of Hermitian operators and what are three useful facts?

Definition: f(x)(A^g(x))dx=(A^f(x))g(x)dx\int_{-\infty}^\infty f(x)^* \Big( \hat{A} g(x) \Big) dx = \int_{-\infty}^\infty \Big( \hat{A} f(x) \Big) ^* g(x) dx

1.) All the eigenvalues of A^\hat{A} are real.

2.) Eigenfunctions corresponding to different eigenvalues are orthogonal:

f(x)g(x)dx=0\int_{-\infty}^\infty f(x)^* g(x) dx = 0

3.) A^=A^\hat{A} = \hat{A}^\dagger

38
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[AB,C]=?[AB, C] = \, ?

[AB,C]=A[B,C]+[A,C]B[AB, C] = A[B,C] + [A,C]B

39
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[A,BC]=?[A, BC] = \, ?

[A,BC]=[A,B]C+B[A,C][A, BC] = [A,B]C + B[A,C]

40
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What are the three laws of Thermodynamics?

1.) Energy cannot be created or destroyed. ΔU=QU\Delta U = Q - U

2.) There is no process in which the sole effect is to transfer heat from a body at a lower temperature to a body at a higher temperature. ΔSδQT\Delta S \ge \int \frac{\delta Q}{T} . The entropy of a thermally isolated system cannot decrease.

3.) Entropy is 0 at absolute zero temperature.

41
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What is the ideal gas law and what are the assumptions that are made? What is the van der Waals correction?

PV=NkBTPV = N k_B T . Gas molecules of zero size which do not interact with each other. van der Waals: (P+N2aV2)(VNb)=NkbT( P + \frac{N² a }{V²} ) ( V - Nb ) = N k_b T

42
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What is a reversible thermodynamic process? What are some examples? How do work and entropy change in a reversible process?

Reversible thermodynamic processes proceed in “infinitesimal” steps such that the system is in equilibrium in each step and can be reversed by changing the state of the system (ex. heating a gas within a container of flexible size).

δW=PdV\delta W = P dV (for gasses)

The total entropy change of the system and its surroundings must be zero. The entropy of the system can change by itself:

δQ=TdS\delta Q = T dS

ΔS=δQT\Delta S = \int \frac{\delta Q }{T} (reversible)

43
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quasistatic process

A process that happens infinitely slowly so that at each instant the system is in thermodynamic equilibrium. (Reversible processes are a subset of quasistatic processes)

44
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adiabatic process

A process for which δQ=0\delta Q = 0 ; no heat is exchanged between the system and its surroundings.

45
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What is an isentropic process? What is the entropy change for such processes? What is the gas equation specific to isentropic processes?

A process that is both adiabatic and reversible (ex. compressing a gas with a piston). The entropy change is 0 for the system and therefore the entropy change for the surroundings is also zero. For a gas undergoing an isentropic process,

PVγ=constantPV^\gamma = constant

where γ=CpCV\gamma = \frac{C_p}{C_V}

46
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iso-”something” process

A process for which some state variable is held constant. (isobaric = constant pressure, isothermal = constant temperature, isochoric = constant volume).

47
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What is free expansion of a gas?

A irreversible process where a gas suddenly expands (like after popping a balloon). The temperature change during free expansion is constant, so

PV=PVPV = P’V’. There is an entropy change even though δQ=0\delta Q = 0 ; the equation ΔSδQT\Delta S \ge \int \frac{\delta Q }{T} does not apply to irreversible processes. The gas also does no work.

48
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What is the Fundamental Thermodynamic Identity? What does it apply to?

dU=TdSPdVdU = T dS - PdV

This applies to all infinitesimal changes of state.

49
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heat capacity

the amount of heat it takes to change the temperature of an object

50
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heat capacity of constant volume

CV=(QT)V=UTC_{V}=(\frac{\partial Q}{\partial T})_{V}=\frac{\partial U} {\partial T }

51
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heat capacity of constant pressure

Cp=(QT)PC_p = ( \frac{\partial Q }{\partial T} ) _P

52
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What is the relation of CPC_P and CVC_V for ideal gasses?

CPCV=NkBC_P - C_V = N k_B

53
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specific heat capacity

“intrinsic heat capacity” with units of J g1^{-1}K1^{-1} . It is the amount of heat needed to raise the temperature of an object by one degree.

Q=mcΔTQ = m c \Delta T

54
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What is entropy and what is Boltzmann’s equation for it?

It is a measure of the number of microstate corresponding to the system’s macrostate.

S=kBlnΩS = k_B \ln \Omega

55
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What is the partition function, ZZ? Why is it useful?

Z=jeβEjZ = \sum_j e^{-\beta E_j} where β=1kBT\beta = \frac{1}{k_B T}.

If you know the partition function, you can compute all state variables.

56
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What is the canonical ensemble of thermodynamics?

The canonical ensemble consists of all possible states of a system with

1.) fixed particle number, NN

2.) fixed volume, VV

3.) fixed temperature, TT

57
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What is the form of the entropy of a monoatomic ideal gas?

S=NkBln(VT3/2N)+some constantsS = N k_B \ln (\frac{V T^{3/2} } { N} ) + \text{some constants}

58
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What is the Equipartition Theorem?

Each quadratic term (degree of freedom) in the Hamiltonian for a particle contributes 12kBT\frac{1}{2} k_B T to the internal energy of the particle.

59
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Stirling’s formula for ln(n!)\ln(n!)

ln(n!)=n(ln(n)1) for large n\ln(n!) = n(\ln(n) - 1) \text{ for large } n