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{{redirect|SIESTA|other uses|Siesta (disambiguation)}}
{{Infobox software
'''SIESTA''' ('''Spanish Initiative for Electronic Simulations with Thousands of Atoms''') is an original method and its computer program implementation, to perform efficient [[electronic structure]] calculations and [[ab initio]] [[molecular dynamics]] simulations of [[molecules]] and solids. SIESTA's efficiency stems from the use of strictly localized basis sets and from the implementation of linear-scaling algorithms which can be applied to suitable systems. A very important feature of the code is that its accuracy and cost can be tuned in a wide range, from quick exploratory calculations to highly accurate simulations matching the quality of other approaches, such as plane-wave and all-electron methods.▼
| name = SIESTA
| logo = SIESTA logo TM.jpg
| logo caption =
| logo alt = SIESTA TM logo
| logo size =
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| released = {{Start date and age|1996|df=yes}}
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| discontinued = <!-- Set to yes, if software is discontinued, otherwise omit. -->
| latest release version = 5.4.0<ref>{{cite web|url=https://siesta-project.org/siesta/news/2025/05/28/release-5.4.0/|title=Release of Siesta-5.4.0}}</ref>
| latest release date = {{Start date and age|2025|05|28|df=yes}}
| repo = {{URL|https://gitlab.com/siesta-project/siesta/}}
| qid = Q7390304
| programming language = [[Fortran]]
| middleware =
| tools =
| engine = <!-- or |engines= -->
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| language = English
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| genre = [[Computational Chemistry]]
| license = [[GPLv3]]
| website = {{URL|siesta-project.org}}
| AsOf = 2025
}}
▲'''SIESTA''' ('''Spanish Initiative for Electronic Simulations with Thousands of Atoms''') is an original method and its computer program implementation, to
SIESTA's [[backronym]] is Spanish Initiative for Electronic Simulations with Thousands of Atoms.▼
▲SIESTA's [[backronym]] is the Spanish Initiative for Electronic Simulations with Thousands of Atoms.
Since 13th May 2016, with the 4.0 version announcement, SIESTA is released under the terms of the [[GPL]] open-source license. Source packages and access to the development versions can be obtained from the [https://launchpad.net/siesta new development and distribution platform].▼
▲Since
== Features ==
SIESTA has these main characteristics
* It uses the standard [[Kohn–Sham equations|Kohn-Sham]]
* It uses norm-conserving [[
* It uses [[
* Projects the electron
* Besides the standard [[Rayleigh–Ritz method|Rayleigh-Ritz eigenstate method]], it allows the use of localized linear combinations of the occupied orbitals (valence-bond or Wannier-like functions), making the computer time and memory scale linearly with the number of atoms. Simulations with several hundred atoms are feasible with modest workstations.
* It is written in [[Fortran 95]] and memory is allocated dynamically.
* It may be compiled for serial or parallel execution (under MPI parallelization, OpenMP threading, and GPU offloading).
SIESTA routinely provides:
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* Stress tensor.
* Electric dipole moment.
* Atomic, orbital, and bond populations ([[Mulliken population analysis|Mulliken]]).
* Electron density.
And also (though not all options are compatible):
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* Constant-temperature molecular dynamics (Nose thermostat).
* Variable cell dynamics (Parrinello-Rahman).
* [[Spin polarization|Spin
* k-sampling of the [[Brillouin zone]].
*
* COOP and COHP curves for chemical bonding analysis.
* [[Dielectric polarization]].
* Vibrations (phonons).
* [[Electronic band structure|Band structure]].
* Ballistic electron transport under non-equilibrium (through TranSIESTA)
* Density functional Bogoliubov-de Gennes theory for superconductors
== Strengths of SIESTA ==
SIESTA's main strengths are:
#
# It can tackle
#
The use of a linear combination of numerical atomic orbitals makes SIESTA a
▲The use of linear combination of numerical atomic orbitals makes SIESTA a flexible and efficient DFT code. SIESTA is able to produce very fast calculations with small basis sets, allowing computing systems with a thousand of atoms. At the same time, the use of more complete and accurate bases allows to achieve accuracies comparable to those of standard plane waves calculations, still at an advantageous computational cost.
== Implemented Solutions ==
SIESTA is in continuous development since it was implemented in 1996. The main solutions implemented in the current version are:
* Collinear and non-collinear spin
* Efficient implementation of Van der Waals functional
* [[Wannier function]] implementation
* TranSIESTA/TBTrans module
* On-site Coulomb corrections (DFT+U
* Description of
* [[Spin-orbit coupling]] (SOC
* Topological insulator, semiconductor structures, and quantum-transport calculations
* NEB (Nudged Elastic Band) (interfacing
== Solutions under development
* [[GW approximation]]
* Time Dependent DFT ([[TDDFT]])
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== Post-processing tools ==
== Applications ==
Since its implementation, SIESTA has
== See also ==
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==References==
* {{Cite journal|doi=10.1063/5.0005077|title=Siesta: Recent developments and applications|year=2020|last1=García|first1=Alberto|last2=Papior|first2=Nick|last3=Akhtar|first3=Arsalan|last4=Artacho|first4=Emilio|last5=Blum|first5=Volker|last6=Bosoni|first6=Emanuele|last7=Brandimarte|first7=Pedro|last8=Brandbyge|first8=Mads|last9=Cerdá|first9=J.I.|last10=Corsetti|first10=Fabiano|last11=Cuadrado|first11=Ramón|last12=Dikan|first12=Vladimir|last13=Ferrer|first13=Jaime|last14=Gale|first14=Julian|last15=García-Fernández|first15=Pablo|last16=García-Suárez|first16=V.M.|last17=García|first17=Sandra|last18=Huhs|first18=Georg|last19=Illera|first19=Sergio|last20=Korytár|first20=Richard|last21=Koval|first21=Peter|last22=Lebedeva|first22=Irina|last23=Lin|first23=Lin|last24=López-Tarifa|first24=Pablo|last25=G. Mayo|first25=Sara|last26=Mohr|first26=Stephan|last27=Ordejón|first27=Pablo|last28=Postnikov|first28=Andrei|last29=Pouillon|first29=Yann|last30=Pruneda|first30=Miguel|last31=Robles|first31=Roberto|last32=Sánchez-Portal|first32=Daniel|last33=Soler|first33=Jose M.|last34=Ullah|first34=Rafi|last35=Yu|first35=Victor Wen-zhe|last36=Junquera|first36=Javier|journal=Journal of Chemical Physics|volume=152|issue=20|pages=204108|pmid=32486661 |hdl=10902/20680|s2cid=219179270 |hdl-access=free|arxiv=2006.01270}} Postprint is available at {{hdl|10261/213028}}.
* {{Cite journal|doi=10.1103/PhysRevB.61.13639|title=Systematic ab initio study of the electronic and magnetic properties of different pure and mixed iron systems|year=2000|last1=Izquierdo|first1=J.|last2=Vega|first2=A.|last3=Balbás|first3=L.|last4=Sánchez-Portal|first4=Daniel|last5=Junquera|first5=Javier|last6=Artacho|first6=Emilio|last7=Soler|first7=Jose|last8=Ordejón|first8=Pablo|journal=Physical Review B|volume=61|issue=20|pages=13639|bibcode = 2000PhRvB..6113639I }}
* {{Cite journal|doi=10.1103/PhysRevB.63.172406|title=All-electron and pseudopotential study of the spin-polarization of the V(001) surface: LDA versus GGA|year=2001|last1=Robles|first1=R.|last2=Izquierdo|first2=J.|last3=Vega|first3=A.|last4=Balbás|first4=L.|journal=Physical Review B|volume=63|issue=17|pages=172406|arxiv = cond-mat/0012064 |bibcode = 2001PhRvB..63q2406R |s2cid=17632035 }}
*{{cite journal
{{Reflist}}
== External links ==
* [http://
* [http://www.home.uni-osnabrueck.de/apostnik/Lectures/SIESTA-tuto.pdf SIESTA tutorial] - an introduction to SIESTA, addressing the tasks for which SIESTA is better suited than other ab initio codes.
* [https://
* [
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