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Cosmological parameter estimation using Particle Swarm
Optimization (PSO)
Jayanti Prasad
in colloboration with Tarun Souradeep
Inter-University Centre for Astronomy & Astrophysics (IUCAA)
Pune, India (411007)
August 11, 2011
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
August 11, 2011
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CMBR data analysis pipeline
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
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“In theory at least, individual members of the school can profit from the
discoveries and previous experience of all other members of the school
during the search for food. This advantage can become decisive,
outweighing the disadvantages of competition for food items, whenever
the resource is unpedictably distributed in patches”
[in reference to fish schooling]
- E. O. Wilson, 1975, Sociobiology: The new synthesis
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
August 11, 2011
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Searching for the global maximum
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
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Parameter estimation
Search for the maximum likelihood point (ML).
Grid based methods - computational cost - exponentially
Stochastic methods - computational cost - linearly (MCMC)
Artificial Intelligence (AI) based optimization methods - Artificial
Neural Network [Phillips & Kogut (2001) ], Genetic Algorithm [ Yao &
Sethares (1994)], Particle Swarm Optimization [ Kennedy & Eberhart
(1995)]
We demonstrate the application of PSO for parameter estimation
from WMAP 7 years data.
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
August 11, 2011
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Particle Swarm Optimization (PSO)
Particle Swarm Optimization (PSO)
Equation of Motion :
i
i
Xt+1
= Xti + Vt+1
(1)
i
i
Vt+1
= wVti + c1 ξ1 (Xti − XPbest
) + c2 ξ2 (Xti − XGbest )
(2)
Velocity :
w:
c1 , c2 :
ξ1 , ξ2 :
XPbest :
XGbest :
inertia weight
acceleration coefficients
random numbers
location of Pbest
location of Gbest
[Kennedy & Eberhart (1995); Wang & Mohanty (2010)]
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
August 11, 2011
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Particle Swarm Optimization (PSO)
Implementation
Initial conditions:
i
i
i
X i (t = 1) = Xmin
+ ξ(Xmax
− Xmin
)
i
V i (t = 1) = ξVmax
(3)
where
i
i
i
Vmax
= cv (Xmax
− Xmin
)
(4)
Boundary conditions (reflecting boundary):
Vti = −Vti
(
i
i
Xmax
, if Xti > Xmax
and Xti =
i
i
Xmin
, if Xti < Xmin
(5)
− F(XGbest ,t )| < for t = 1, nstop
(6)
Stopping criteria:
|F(XGbest
Jayanti Prasad (IUCAA-PUNE)
,t+1
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August 11, 2011
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Results
Sampling
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
August 11, 2011
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Results
Gbest
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
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Results
Gbest
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
August 11, 2011
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Results
Power spectrum
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
August 11, 2011
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Results
Parameters
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
August 11, 2011
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summary
Summary & conclusions
Parameter estimation is an important exercise in current cosmological
research.
We have demonstrated that PSO also can be used for parameter
estimation from CMBR data.
Parameters which we have estimated using PSO are consistent with
that obtained from other commonly used methods like MCMC.
Due to simple algorithm and few design parameters, PSO can be
easily implemented and parallelized on a cluster system for
accelerated search of parameters.
PSO can be very useful in situations when the dimensionality of the
search space is very high and/or there are a large number of local
maxima present.
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
August 11, 2011
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summary
Thank You !
Jayanti Prasad (IUCAA-PUNE)
Parameter estimating using PSO
August 11, 2011
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summary
References
Kennedy, J., & Eberhart, R. 1995, IEEE, 1942
Phillips, N. G., & Kogut, A. 2001, ArXiv Astrophysics e-prints
Wang, Y., & Mohanty, S. D. 2010, Phys. Rev. D , 81, 063002
Yao, L., & Sethares, W. A. 1994, IEEE Transactions on Signal Processing, 927
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August 11, 2011
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