In [1]:
%matplotlib inline
from scipy.optimize import minimize
import numpy as np
import matplotlib.pyplot as plt
from scipy.constants import pi, Boltzmann
The form of the damping is given as:
$$ \Gamma_0 = \dfrac{6 \pi \eta_{air} r}{m} \dfrac{0.619}{0.619 + K_n} (1+ c_k)$$(Li et al. 2011 - https://arxiv.org/pdf/1101.1283.pdf)
Where:
The mean free path is dependant upon the pressure of the system. The mathematical form the mean free path, is dependant upon whether the particles under study are con- sidered to be hard like spheres colliding or as “soft” spheres following Lennard-Jones Potential. In this case assuming the gas particles to be hard spheres yields the following form,
$$s = \dfrac{k_B T_0}{ \sqrt{2} \pi d_{gas}^2 P_{gas}} $$(Muddassar - Thesis - Cooling and Squeezing in Levitated Optomechanics 2016)
Where:
In [179]:
# constants
k_B = Boltzmann
eta_air = 18.27e-6 # Pa # (J.T.R.Watson (1995)).
d_gas = 0.372e-9 #m #(Sone (2007)), ρSiO2
rho_SiO2 = 1800 # #kg/m^3 - Number told to us by
T0 = 300
R = 50e-9 # m
In [180]:
def mfp(P_gas):
mfp_val = k_B*T0/(2**0.5*pi*d_gas**2*P_gas)
return mfp_val
Alternativity one can use:
$$ s = \dfrac{\eta_{air}}{P_{gas}} \sqrt{\dfrac{\pi k_B T_0}{2m}} $$https://en.wikipedia.org/wiki/Mean_free_path
Where
molecular mass of air is $28.97 g/mol$ and the number of molecules in a mole is Avogadro's Number $6.0221409e^{23}$ therefore we get the molecular mass of air to be $4.81e^{-26} Kg$
In [181]:
m_gas = 4.81e-26
In [182]:
def mfp_2(P_gas):
mfp_val = eta_air/P_gas * (pi*k_B*T0/(2*m_gas))**0.5
return mfp_val
In [183]:
s = mfp(300) # 3mbar = 300 Pascals
print(s)
In [184]:
s2 = mfp_2(300) # 3mbar = 300 Pascals
print(s2)
In [185]:
def Gamma_env(radius, Pressure_mbar):
mass = rho_SiO2 * 4/3*pi*radius**3
Pressure_pascals = 100*Pressure_mbar
s = mfp(Pressure_pascals)
K_n = s/radius
c_K = 0.31*K_n/(0.785 + 1.152*K_n + K_n**2)
Gamma_0 = 6*pi*eta_air*radius/mass * 0.619/(0.619 + K_n) * (1+c_K)
return Gamma_0
In [186]:
Gamma_env(R, 3)
Out[186]:
Muddassar and Gieseler's simplified formula for the environmental damping is:
$$ \Gamma_0 = 0.619 \dfrac{9 \pi}{\sqrt{2}} \dfrac{\eta_{air}d_{gas}^2}{\rho_{SiO_2} k_B T_0} \dfrac{P_{gas}}{r}$$This produces the same result as the full unsimplified form for all pressures in range of interest.
Where:
In [187]:
def Gamma_env_simple(radius, Pressure_mbar):
Pressure_pascals = 100*Pressure_mbar
#Gamma_0 = 0.619*9*pi*eta_air*d_gas**2*Pressure_pascals/(2**0.5*rho_SiO2*k_B*T0*radius)
Gamma_0 = 0.619*9*pi*eta_air*d_gas**2*Pressure_pascals/(2**0.5*rho_SiO2*k_B*T0*radius)
return Gamma_0
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In [188]:
Gamma_env_simple(R, 3)
Out[188]:
In Gieseler's Thermal Nonlinearities paper he has the following equation for $\Gamma_0$
$$ \Gamma_0 = \dfrac{64a^2}{3m\bar{v}}P $$https://www.nature.com/nphys/journal/v9/n12/full/nphys2798.html
This appears to be incorrect as it is exactly double that which you get with Chang's formula and James Millen's formula
Where:
Where we can use the following formula for $\bar{v}$
$$ \bar{v} = \sqrt{\dfrac{8k_B T_0}{\pi \mu}} $$Where:
In [189]:
def Gamma_alternative(radius, Pressure_mbar):
Pressure = 100*Pressure_mbar
ave_velocity = (8*k_B*T0/(pi*m_gas))**0.5
mass= rho_SiO2*4/3*pi*radius**3
Gamma0 = 64*radius**2*Pressure/(3*mass*ave_velocity)
return Gamma0
In [190]:
Gamma_alternative(R, 3)
Out[190]:
In Chang et al. paper "Cavity opto-mechanics using an optically levitated nanosphere"
They have $\Gamma_0 = \dfrac{\gamma_g}{2} = \dfrac{8}{\pi}\dfrac{P}{\bar{v}r\rho}$
Where
In [191]:
ave_velocity = (8*k_B*T0/(pi*m_gas))**0.5
In [192]:
ave_velocity
Out[192]:
In [193]:
def Gamma_chang(radius, Pressure_mbar):
Pressure = 100*Pressure_mbar
ave_velocity = (8*k_B*T0/(pi*m_gas))**0.5
Gamma0 = 8*Pressure/(pi*ave_velocity*radius*rho_SiO2)/2
return 2*Gamma0
In [194]:
Gamma_chang(R, 3)
Out[194]:
James Millen derives the following form of the damping due to impinging particles:
$$ \Gamma^{imp} = \dfrac{4\pi}{3}\dfrac{mNr^2 \bar{v}_{T_{imp}}}{M} $$https://arxiv.org/abs/1309.3990 - https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.114.123602
However in their earlier paper http://iopscience.iop.org/article/10.1088/1367-2630/15/1/015001/meta they get double this, which is what Gieseler gets in his thermal non-linearities paper.
Where:
Using the ideal gas equation $P = R\rho T$ and $N= \dfrac{\rho}{m}$ with $R=\dfrac{k_B}{m}$ we get $N = \dfrac{P}{k_BT}$
In [195]:
def Gamma_Millen_imp(radius, Pressure_mbar):
Pressure = 100*Pressure_mbar
ave_velocity = (8*k_B*T0/(pi*m_gas))**0.5
mass = rho_SiO2*4/3*pi*radius**3
N = Pressure/(k_B*T0)
Gamma0 = 4*pi*m_gas*N*radius**2*ave_velocity/(3*mass)
return Gamma0
In [196]:
Gamma_Millen_imp(R, 3)
Out[196]:
In [197]:
Gamma_chang(R, 3)
Out[197]:
James Millen derives the following form of the damping due to emerging particles:
$\Gamma^{em} = \dfrac{mNr^2\pi^{\frac{3}{2}}}{3\sqrt{h'}M}$
https://arxiv.org/abs/1309.3990 - https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.114.123602
Where:
Using the ideal gas equation $P = R\rho T$ and $N= \dfrac{\rho}{m}$ with $R=\dfrac{k_B}{m}$ we get $N = \dfrac{P}{k_BT}$
He also says that this leads to $\Gamma^{em} = \dfrac{\pi}{8}\dfrac{T^{em}}{T^{imp}}$
From this you get the total effective damping rate is $$ \Gamma_0 = \Gamma^{em} + \Gamma^{imp} = \dfrac{\pi}{8}\sqrt{\dfrac{T^{em}}{T^{imp}}}\Gamma^{imp} + \Gamma^{imp} $$
In [198]:
def Gamma_Millen_em(radius, Pressure_mbar, T_em):
Pressure = 100*Pressure_mbar
h_prime = m_gas/(k_B*T_em)
mass = rho_SiO2*4/3*pi*radius**3
N = Pressure/(k_B*T_em)
Gamma0 = (m_gas*N*radius**2*pi**(3/2))/(3*np.sqrt(h_prime)*mass)
return Gamma0
In [199]:
def calc_surface_temp_Millen(T_em, T_imp=300):
accomodation_coef = 0.777 # accomodation coefficient of silica (from Nanoscale temp measurement paper)
T_surf = T_imp + (T_em + T_imp)/accomodation_coef
return T_surf
In [200]:
P_exp = np.load("Pressure_mbar.npy")
Gamma_exp = np.load("Gamma_radians.npy")
In [201]:
P_G_Dict = dict(zip(P_exp, Gamma_exp))
In [202]:
r = np.linspace(5e-9, 1000e-9, 1000)
P = 3.6 # mbar
alpha=0.5
plt.figure(figsize=[10, 10])
plt.loglog(r, Gamma_env_simple(r, P), 'k', label="Rashid/Gieseler Full form", alpha=alpha)
#plt.semilogy(r, Gamma_env_simple(r, P), 'grey', label="Rashid/Gieseler simplfied form", alpha=alpha)
plt.loglog(r, Gamma_alternative(r, P), label="Gieseler Thermal Non-linearities form", alpha=alpha)
plt.loglog(r, Gamma_chang(r, P), label="Chang form", alpha=alpha)
plt.loglog(r, Gamma_Millen_imp(r, P), label="Millen (imp) form", alpha=alpha)
plt.xlabel("radius (nm)")
plt.ylabel("Γ (radians/s)")
plt.legend(loc='best')
plt.show()
In [203]:
r = 50e-9
P = np.linspace(1e-2, 1000, 1000)
plt.figure(figsize=[10, 10])
plt.loglog(P, Gamma_env_simple(r, P), 'k', label="Rashid/Gieseler Full form", alpha=alpha)
#plt.loglog(P, Gamma_env_simple(r, P), 'grey', label="Rashid/Gieseler simplfied form", alpha=alpha)
plt.loglog(P, Gamma_alternative(r, P), label="Gieseler Thermal Non-linearities form", alpha=alpha)
plt.loglog(P, Gamma_chang(r, P), label="Chang form", alpha=alpha)
plt.loglog(P, Gamma_Millen_imp(r, P), label="Millen (imp) form", alpha=alpha)
plt.loglog(P_exp, Gamma_exp, label="Experiment", alpha=alpha)
plt.xlabel("P (mbar)")
plt.ylabel("Γ (radians/s)")
plt.legend(loc='best')
plt.show()
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