Radiation pressure induced instabilities in laser interferometric detectors of gravitational waves View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2000-02-01

AUTHORS

A. Pai, S. V. Dhurandhar, P. Hello, J. -Y. Vinet

ABSTRACT

The large scale interferometric gravitational wave detectors consist of Fabry-Perot cavities operating at very high powers ranging from tens of kW to MW for next generations. The high powers may result in several nonlinear effects which would affect the performance of the detector. In this paper, we investigate the effects of radiation pressure, which tend to displace the mirrors from their resonant position resulting in the detuning of the cavity. We observe a remarkable effect, namely, that the freely hanging mirrors gain energy continuously and swing with increasing amplitude. It is found that the “time delay”, that is, the time taken for the field to adjust to its instantaneous equilibrium value, when the mirrors are in motion, is responsible for this effect. This effect is likely to be important in the optimal operation of the full-scale interferometers such as VIRGO and LIGO. More... »

PAGES

333

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s100530050043

DOI

http://dx.doi.org/10.1007/s100530050043

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1052924246


Indexing Status Check whether this publication has been indexed by Scopus and Web Of Science using the SN Indexing Status Tool
Incoming Citations Browse incoming citations for this publication using opencitations.net

JSON-LD is the canonical representation for SciGraph data.

TIP: You can open this SciGraph record using an external JSON-LD service: JSON-LD Playground Google SDTT

[
  {
    "@context": "https://springernature.github.io/scigraph/jsonld/sgcontext.json", 
    "about": [
      {
        "id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/02", 
        "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
        "name": "Physical Sciences", 
        "type": "DefinedTerm"
      }, 
      {
        "id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/0299", 
        "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
        "name": "Other Physical Sciences", 
        "type": "DefinedTerm"
      }
    ], 
    "author": [
      {
        "affiliation": {
          "alternateName": "Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, 411007, Ganeshkhind, Pune, India", 
          "id": "http://www.grid.ac/institutes/grid.249801.6", 
          "name": [
            "Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, 411007, Ganeshkhind, Pune, India"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Pai", 
        "givenName": "A.", 
        "id": "sg:person.010400664501.26", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.010400664501.26"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Department of Physics and Astronomy, UWCC, P.O. Box 913, Cardiff, CF2 3YB, Cardiff, UK", 
          "id": "http://www.grid.ac/institutes/grid.5600.3", 
          "name": [
            "Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, 411007, Ganeshkhind, Pune, India", 
            "Department of Physics and Astronomy, UWCC, P.O. Box 913, Cardiff, CF2 3YB, Cardiff, UK"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Dhurandhar", 
        "givenName": "S. V.", 
        "id": "sg:person.015721607447.72", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.015721607447.72"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Groupe Virgo, Laboratoire de l\u2019Acc\u00e9l\u00e9rateur Lin\u00e9aire, Centre d\u2019Orsay, b\u00e2timent 200, 91405, Orsay, France", 
          "id": "http://www.grid.ac/institutes/None", 
          "name": [
            "Groupe Virgo, Laboratoire de l\u2019Acc\u00e9l\u00e9rateur Lin\u00e9aire, Centre d\u2019Orsay, b\u00e2timent 200, 91405, Orsay, France"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Hello", 
        "givenName": "P.", 
        "id": "sg:person.07351661773.52", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.07351661773.52"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Groupe Virgo, Laboratoire de l\u2019Acc\u00e9l\u00e9rateur Lin\u00e9aire, Centre d\u2019Orsay, b\u00e2timent 200, 91405, Orsay, France", 
          "id": "http://www.grid.ac/institutes/None", 
          "name": [
            "Groupe Virgo, Laboratoire de l\u2019Acc\u00e9l\u00e9rateur Lin\u00e9aire, Centre d\u2019Orsay, b\u00e2timent 200, 91405, Orsay, France"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Vinet", 
        "givenName": "J. -Y.", 
        "id": "sg:person.011505147731.76", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.011505147731.76"
        ], 
        "type": "Person"
      }
    ], 
    "datePublished": "2000-02-01", 
    "datePublishedReg": "2000-02-01", 
    "description": "The large scale interferometric gravitational wave detectors consist of Fabry-Perot cavities operating at very high powers ranging from tens of kW to MW for next generations. The high powers may result in several nonlinear effects which would affect the performance of the detector. In this paper, we investigate the effects of radiation pressure, which tend to displace the mirrors from their resonant position resulting in the detuning of the cavity. We observe a remarkable effect, namely, that the freely hanging mirrors gain energy continuously and swing with increasing amplitude. It is found that the \u201ctime delay\u201d, that is, the time taken for the field to adjust to its instantaneous equilibrium value, when the mirrors are in motion, is responsible for this effect. This effect is likely to be important in the optimal operation of the full-scale interferometers such as VIRGO and LIGO.", 
    "genre": "article", 
    "id": "sg:pub.10.1007/s100530050043", 
    "inLanguage": "en", 
    "isAccessibleForFree": true, 
    "isPartOf": [
      {
        "id": "sg:journal.1398043", 
        "issn": [
          "1155-4312", 
          "1286-4870"
        ], 
        "name": "The European Physical Journal D", 
        "publisher": "Springer Nature", 
        "type": "Periodical"
      }, 
      {
        "issueNumber": "3", 
        "type": "PublicationIssue"
      }, 
      {
        "type": "PublicationVolume", 
        "volumeNumber": "8"
      }
    ], 
    "keywords": [
      "radiation pressure", 
      "interferometric gravitational wave detectors", 
      "gravitational wave detectors", 
      "Fabry-Perot cavity", 
      "laser interferometric detectors", 
      "high power", 
      "wave detectors", 
      "interferometric detectors", 
      "gravitational waves", 
      "tens of kW", 
      "resonant position", 
      "nonlinear effects", 
      "mirror", 
      "detector", 
      "LIGO", 
      "Virgo", 
      "detuning", 
      "interferometer", 
      "equilibrium value", 
      "time delay", 
      "next generation", 
      "cavity", 
      "energy", 
      "waves", 
      "tens", 
      "field", 
      "kW", 
      "mW", 
      "power", 
      "remarkable effect", 
      "instability", 
      "amplitude", 
      "motion", 
      "generation", 
      "effect", 
      "pressure", 
      "position", 
      "operation", 
      "values", 
      "time", 
      "performance", 
      "delay", 
      "paper", 
      "optimal operation", 
      "large scale interferometric gravitational wave detectors", 
      "scale interferometric gravitational wave detectors", 
      "instantaneous equilibrium value", 
      "full-scale interferometers"
    ], 
    "name": "Radiation pressure induced instabilities in laser interferometric detectors of gravitational waves", 
    "pagination": "333", 
    "productId": [
      {
        "name": "dimensions_id", 
        "type": "PropertyValue", 
        "value": [
          "pub.1052924246"
        ]
      }, 
      {
        "name": "doi", 
        "type": "PropertyValue", 
        "value": [
          "10.1007/s100530050043"
        ]
      }
    ], 
    "sameAs": [
      "https://doi.org/10.1007/s100530050043", 
      "https://app.dimensions.ai/details/publication/pub.1052924246"
    ], 
    "sdDataset": "articles", 
    "sdDatePublished": "2021-11-01T18:04", 
    "sdLicense": "https://scigraph.springernature.com/explorer/license/", 
    "sdPublisher": {
      "name": "Springer Nature - SN SciGraph project", 
      "type": "Organization"
    }, 
    "sdSource": "s3://com-springernature-scigraph/baseset/20211101/entities/gbq_results/article/article_334.jsonl", 
    "type": "ScholarlyArticle", 
    "url": "https://doi.org/10.1007/s100530050043"
  }
]
 

Download the RDF metadata as:  json-ld nt turtle xml License info

HOW TO GET THIS DATA PROGRAMMATICALLY:

JSON-LD is a popular format for linked data which is fully compatible with JSON.

curl -H 'Accept: application/ld+json' 'https://scigraph.springernature.com/pub.10.1007/s100530050043'

N-Triples is a line-based linked data format ideal for batch operations.

curl -H 'Accept: application/n-triples' 'https://scigraph.springernature.com/pub.10.1007/s100530050043'

Turtle is a human-readable linked data format.

curl -H 'Accept: text/turtle' 'https://scigraph.springernature.com/pub.10.1007/s100530050043'

RDF/XML is a standard XML format for linked data.

curl -H 'Accept: application/rdf+xml' 'https://scigraph.springernature.com/pub.10.1007/s100530050043'


 

This table displays all metadata directly associated to this object as RDF triples.

134 TRIPLES      21 PREDICATES      73 URIs      65 LITERALS      6 BLANK NODES

Subject Predicate Object
1 sg:pub.10.1007/s100530050043 schema:about anzsrc-for:02
2 anzsrc-for:0299
3 schema:author N5f1edb0df78249e2a7fb10d4865cedb8
4 schema:datePublished 2000-02-01
5 schema:datePublishedReg 2000-02-01
6 schema:description The large scale interferometric gravitational wave detectors consist of Fabry-Perot cavities operating at very high powers ranging from tens of kW to MW for next generations. The high powers may result in several nonlinear effects which would affect the performance of the detector. In this paper, we investigate the effects of radiation pressure, which tend to displace the mirrors from their resonant position resulting in the detuning of the cavity. We observe a remarkable effect, namely, that the freely hanging mirrors gain energy continuously and swing with increasing amplitude. It is found that the “time delay”, that is, the time taken for the field to adjust to its instantaneous equilibrium value, when the mirrors are in motion, is responsible for this effect. This effect is likely to be important in the optimal operation of the full-scale interferometers such as VIRGO and LIGO.
7 schema:genre article
8 schema:inLanguage en
9 schema:isAccessibleForFree true
10 schema:isPartOf N7fa345ec5e3d4c1eb0a734e20840950b
11 Nc5444197aa5543b3a8a32b9978f9224c
12 sg:journal.1398043
13 schema:keywords Fabry-Perot cavity
14 LIGO
15 Virgo
16 amplitude
17 cavity
18 delay
19 detector
20 detuning
21 effect
22 energy
23 equilibrium value
24 field
25 full-scale interferometers
26 generation
27 gravitational wave detectors
28 gravitational waves
29 high power
30 instability
31 instantaneous equilibrium value
32 interferometer
33 interferometric detectors
34 interferometric gravitational wave detectors
35 kW
36 large scale interferometric gravitational wave detectors
37 laser interferometric detectors
38 mW
39 mirror
40 motion
41 next generation
42 nonlinear effects
43 operation
44 optimal operation
45 paper
46 performance
47 position
48 power
49 pressure
50 radiation pressure
51 remarkable effect
52 resonant position
53 scale interferometric gravitational wave detectors
54 tens
55 tens of kW
56 time
57 time delay
58 values
59 wave detectors
60 waves
61 schema:name Radiation pressure induced instabilities in laser interferometric detectors of gravitational waves
62 schema:pagination 333
63 schema:productId Nccb7eece53cc4f9aaabb15e916469bea
64 Nec88a05667334bee97d99f5546d94cf5
65 schema:sameAs https://app.dimensions.ai/details/publication/pub.1052924246
66 https://doi.org/10.1007/s100530050043
67 schema:sdDatePublished 2021-11-01T18:04
68 schema:sdLicense https://scigraph.springernature.com/explorer/license/
69 schema:sdPublisher Naafa598b38a34af99a784a5fa9a5d279
70 schema:url https://doi.org/10.1007/s100530050043
71 sgo:license sg:explorer/license/
72 sgo:sdDataset articles
73 rdf:type schema:ScholarlyArticle
74 N1f39ba019fea40bb988846f2a2cbfd8b rdf:first sg:person.011505147731.76
75 rdf:rest rdf:nil
76 N5f1edb0df78249e2a7fb10d4865cedb8 rdf:first sg:person.010400664501.26
77 rdf:rest Nb3119150d67847f7a99e9181b9e3e89e
78 N7fa345ec5e3d4c1eb0a734e20840950b schema:issueNumber 3
79 rdf:type schema:PublicationIssue
80 Naafa598b38a34af99a784a5fa9a5d279 schema:name Springer Nature - SN SciGraph project
81 rdf:type schema:Organization
82 Nb3119150d67847f7a99e9181b9e3e89e rdf:first sg:person.015721607447.72
83 rdf:rest Nedfac7b2054a41fc8016acf2680f45c1
84 Nc5444197aa5543b3a8a32b9978f9224c schema:volumeNumber 8
85 rdf:type schema:PublicationVolume
86 Nccb7eece53cc4f9aaabb15e916469bea schema:name dimensions_id
87 schema:value pub.1052924246
88 rdf:type schema:PropertyValue
89 Nec88a05667334bee97d99f5546d94cf5 schema:name doi
90 schema:value 10.1007/s100530050043
91 rdf:type schema:PropertyValue
92 Nedfac7b2054a41fc8016acf2680f45c1 rdf:first sg:person.07351661773.52
93 rdf:rest N1f39ba019fea40bb988846f2a2cbfd8b
94 anzsrc-for:02 schema:inDefinedTermSet anzsrc-for:
95 schema:name Physical Sciences
96 rdf:type schema:DefinedTerm
97 anzsrc-for:0299 schema:inDefinedTermSet anzsrc-for:
98 schema:name Other Physical Sciences
99 rdf:type schema:DefinedTerm
100 sg:journal.1398043 schema:issn 1155-4312
101 1286-4870
102 schema:name The European Physical Journal D
103 schema:publisher Springer Nature
104 rdf:type schema:Periodical
105 sg:person.010400664501.26 schema:affiliation grid-institutes:grid.249801.6
106 schema:familyName Pai
107 schema:givenName A.
108 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.010400664501.26
109 rdf:type schema:Person
110 sg:person.011505147731.76 schema:affiliation grid-institutes:None
111 schema:familyName Vinet
112 schema:givenName J. -Y.
113 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.011505147731.76
114 rdf:type schema:Person
115 sg:person.015721607447.72 schema:affiliation grid-institutes:grid.5600.3
116 schema:familyName Dhurandhar
117 schema:givenName S. V.
118 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.015721607447.72
119 rdf:type schema:Person
120 sg:person.07351661773.52 schema:affiliation grid-institutes:None
121 schema:familyName Hello
122 schema:givenName P.
123 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.07351661773.52
124 rdf:type schema:Person
125 grid-institutes:None schema:alternateName Groupe Virgo, Laboratoire de l’Accélérateur Linéaire, Centre d’Orsay, bâtiment 200, 91405, Orsay, France
126 schema:name Groupe Virgo, Laboratoire de l’Accélérateur Linéaire, Centre d’Orsay, bâtiment 200, 91405, Orsay, France
127 rdf:type schema:Organization
128 grid-institutes:grid.249801.6 schema:alternateName Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, 411007, Ganeshkhind, Pune, India
129 schema:name Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, 411007, Ganeshkhind, Pune, India
130 rdf:type schema:Organization
131 grid-institutes:grid.5600.3 schema:alternateName Department of Physics and Astronomy, UWCC, P.O. Box 913, Cardiff, CF2 3YB, Cardiff, UK
132 schema:name Department of Physics and Astronomy, UWCC, P.O. Box 913, Cardiff, CF2 3YB, Cardiff, UK
133 Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, 411007, Ganeshkhind, Pune, India
134 rdf:type schema:Organization
 




Preview window. Press ESC to close (or click here)


...