Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy

Autores
Zajnulina, M.; Chavez Boggio, J. M.; Böhm, M.; Rieznik, Andrés Anibal; Fremberg, T.; Haynes, R.; Roth, M. M.
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We investigate the generation of optical frequency combs through a cascade of four-wave mixing processes in nonlinear fibres with optimised parameters. The initial optical field consists of two continuous-wave lasers with frequency separation larger than 40 GHz (312.7 pm at 1531 nm). It propagates through three nonlinear fibres. The first fibre serves to pulse shape the initial sinusoidal-square pulse, while a strong pulse compression down to sub-100 fs takes place in the second fibre which is an amplifying erbium-doped fibre. The last stage is a low-dispersion highly nonlinear fibre where the frequency comb bandwidth is increased and the line intensity is equalised. We model this system using the generalised nonlinear Schrödinger equation and investigate it in terms of fibre lengths, fibre dispersion, laser frequency separation and input powers with the aim to minimise the frequency comb noise. With the support of the numerical results, a frequency comb is experimentally generated, first in the near infra-red and then it is frequency-doubled into the visible spectral range. Using a MUSE-type spectrograph, we evaluate the comb performance for astronomical wavelength calibration in terms of equidistancy of the comb lines and their stability.
Fil: Zajnulina, M.. Leibniz Institute for Astrophysics Potsdam; Alemania
Fil: Chavez Boggio, J. M.. Leibniz Institute for Astrophysics Potsdam; Alemania
Fil: Böhm, M.. Universitat Potsdam; Alemania
Fil: Rieznik, Andrés Anibal. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Instituto Tecnológico de Buenos Aires; Argentina
Fil: Fremberg, T.. Leibniz Institute for Astrophysics Potsdam; Alemania
Fil: Haynes, R.. Leibniz Institute for Astrophysics Potsdam; Alemania
Fil: Roth, M. M.. Leibniz Institute for Astrophysics Potsdam; Alemania
Materia
Soliton
Intensity Noise
Optical Pulse
Frequency Comb
Optical Frequency Comb
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/41665
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomyZajnulina, M.Chavez Boggio, J. M.Böhm, M.Rieznik, Andrés AnibalFremberg, T.Haynes, R.Roth, M. M.SolitonIntensity NoiseOptical PulseFrequency CombOptical Frequency Combhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We investigate the generation of optical frequency combs through a cascade of four-wave mixing processes in nonlinear fibres with optimised parameters. The initial optical field consists of two continuous-wave lasers with frequency separation larger than 40 GHz (312.7 pm at 1531 nm). It propagates through three nonlinear fibres. The first fibre serves to pulse shape the initial sinusoidal-square pulse, while a strong pulse compression down to sub-100 fs takes place in the second fibre which is an amplifying erbium-doped fibre. The last stage is a low-dispersion highly nonlinear fibre where the frequency comb bandwidth is increased and the line intensity is equalised. We model this system using the generalised nonlinear Schrödinger equation and investigate it in terms of fibre lengths, fibre dispersion, laser frequency separation and input powers with the aim to minimise the frequency comb noise. With the support of the numerical results, a frequency comb is experimentally generated, first in the near infra-red and then it is frequency-doubled into the visible spectral range. Using a MUSE-type spectrograph, we evaluate the comb performance for astronomical wavelength calibration in terms of equidistancy of the comb lines and their stability.Fil: Zajnulina, M.. Leibniz Institute for Astrophysics Potsdam; AlemaniaFil: Chavez Boggio, J. M.. Leibniz Institute for Astrophysics Potsdam; AlemaniaFil: Böhm, M.. Universitat Potsdam; AlemaniaFil: Rieznik, Andrés Anibal. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Instituto Tecnológico de Buenos Aires; ArgentinaFil: Fremberg, T.. Leibniz Institute for Astrophysics Potsdam; AlemaniaFil: Haynes, R.. Leibniz Institute for Astrophysics Potsdam; AlemaniaFil: Roth, M. M.. Leibniz Institute for Astrophysics Potsdam; AlemaniaSpringer2015-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/41665Zajnulina, M.; Chavez Boggio, J. M.; Böhm, M.; Rieznik, Andrés Anibal; Fremberg, T.; et al.; Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy; Springer; Applied Physics B: Lasers and Optics; 120; 1; 5-2015; 171-1840946-2171CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s00340-015-6121-1info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2Fs00340-015-6121-1info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:56:04Zoai:ri.conicet.gov.ar:11336/41665instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-03 09:56:04.331CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy
title Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy
spellingShingle Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy
Zajnulina, M.
Soliton
Intensity Noise
Optical Pulse
Frequency Comb
Optical Frequency Comb
title_short Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy
title_full Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy
title_fullStr Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy
title_full_unstemmed Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy
title_sort Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy
dc.creator.none.fl_str_mv Zajnulina, M.
Chavez Boggio, J. M.
Böhm, M.
Rieznik, Andrés Anibal
Fremberg, T.
Haynes, R.
Roth, M. M.
author Zajnulina, M.
author_facet Zajnulina, M.
Chavez Boggio, J. M.
Böhm, M.
Rieznik, Andrés Anibal
Fremberg, T.
Haynes, R.
Roth, M. M.
author_role author
author2 Chavez Boggio, J. M.
Böhm, M.
Rieznik, Andrés Anibal
Fremberg, T.
Haynes, R.
Roth, M. M.
author2_role author
author
author
author
author
author
dc.subject.none.fl_str_mv Soliton
Intensity Noise
Optical Pulse
Frequency Comb
Optical Frequency Comb
topic Soliton
Intensity Noise
Optical Pulse
Frequency Comb
Optical Frequency Comb
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We investigate the generation of optical frequency combs through a cascade of four-wave mixing processes in nonlinear fibres with optimised parameters. The initial optical field consists of two continuous-wave lasers with frequency separation larger than 40 GHz (312.7 pm at 1531 nm). It propagates through three nonlinear fibres. The first fibre serves to pulse shape the initial sinusoidal-square pulse, while a strong pulse compression down to sub-100 fs takes place in the second fibre which is an amplifying erbium-doped fibre. The last stage is a low-dispersion highly nonlinear fibre where the frequency comb bandwidth is increased and the line intensity is equalised. We model this system using the generalised nonlinear Schrödinger equation and investigate it in terms of fibre lengths, fibre dispersion, laser frequency separation and input powers with the aim to minimise the frequency comb noise. With the support of the numerical results, a frequency comb is experimentally generated, first in the near infra-red and then it is frequency-doubled into the visible spectral range. Using a MUSE-type spectrograph, we evaluate the comb performance for astronomical wavelength calibration in terms of equidistancy of the comb lines and their stability.
Fil: Zajnulina, M.. Leibniz Institute for Astrophysics Potsdam; Alemania
Fil: Chavez Boggio, J. M.. Leibniz Institute for Astrophysics Potsdam; Alemania
Fil: Böhm, M.. Universitat Potsdam; Alemania
Fil: Rieznik, Andrés Anibal. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Instituto Tecnológico de Buenos Aires; Argentina
Fil: Fremberg, T.. Leibniz Institute for Astrophysics Potsdam; Alemania
Fil: Haynes, R.. Leibniz Institute for Astrophysics Potsdam; Alemania
Fil: Roth, M. M.. Leibniz Institute for Astrophysics Potsdam; Alemania
description We investigate the generation of optical frequency combs through a cascade of four-wave mixing processes in nonlinear fibres with optimised parameters. The initial optical field consists of two continuous-wave lasers with frequency separation larger than 40 GHz (312.7 pm at 1531 nm). It propagates through three nonlinear fibres. The first fibre serves to pulse shape the initial sinusoidal-square pulse, while a strong pulse compression down to sub-100 fs takes place in the second fibre which is an amplifying erbium-doped fibre. The last stage is a low-dispersion highly nonlinear fibre where the frequency comb bandwidth is increased and the line intensity is equalised. We model this system using the generalised nonlinear Schrödinger equation and investigate it in terms of fibre lengths, fibre dispersion, laser frequency separation and input powers with the aim to minimise the frequency comb noise. With the support of the numerical results, a frequency comb is experimentally generated, first in the near infra-red and then it is frequency-doubled into the visible spectral range. Using a MUSE-type spectrograph, we evaluate the comb performance for astronomical wavelength calibration in terms of equidistancy of the comb lines and their stability.
publishDate 2015
dc.date.none.fl_str_mv 2015-05
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/41665
Zajnulina, M.; Chavez Boggio, J. M.; Böhm, M.; Rieznik, Andrés Anibal; Fremberg, T.; et al.; Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy; Springer; Applied Physics B: Lasers and Optics; 120; 1; 5-2015; 171-184
0946-2171
CONICET Digital
CONICET
url http://hdl.handle.net/11336/41665
identifier_str_mv Zajnulina, M.; Chavez Boggio, J. M.; Böhm, M.; Rieznik, Andrés Anibal; Fremberg, T.; et al.; Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy; Springer; Applied Physics B: Lasers and Optics; 120; 1; 5-2015; 171-184
0946-2171
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1007/s00340-015-6121-1
info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2Fs00340-015-6121-1
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1842269382089113600
score 13.13397

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