Test of Lorentz Invariance for Photons with Optical Ring Cavity

光环腔光子洛伦兹不变性测试

• 批准号: 18J21016
• 负责人: 武田 紘樹
• 金额: $ 1.79万
• 依托单位: The University of Tokyo
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for JSPS Fellows
• 财政年份: 2018
• 资助国家: 日本
• 起止时间: 2018-04-25 至 2021-03-31
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-18J21016/
• 关键词: ローレンツ不変性; 異方性; 光速; 光共振器; 相対性理論; 干渉計; 対称性; 拡張標準模型

本研究は光リング共振器を用いて光速の異方性を探査することで光子のローレンツ不変性を高精度検証することを目的としている。我々はこれまで簡易な信号変調のための非連続回転系と光学系を用いて、6e-15レベルでの世界最高精度で奇パリティの異方性探査を行ってきた。その感度は回転に伴う振動雑音で制限されていたため、振動感度を低減することでさらなる高精度検証を目指している。 当年度は、ローレンツ不変性の破れが示唆されている光速差で-17乗の世界最高精度で片道光速の異方性を検証するために、回転機構の調整を行うことが目的であった。本年度は回転台部の傾きを調整するなどして雑音源の把握に努めた。また、ある種のローレンツ不変性の破れが許されている重力理論においては重力波は非テンソル的な偏極成分を持つことが許される。重力波の自由度の性質はこのように重力理論を反映するので、重力波の偏極モード検証によって重力理論検証が可能となる。本年度は本研究課題を派生させ、GW170814やGW170817といったコンパクト連星合体からの重力波イベントに対して、重力波の偏極モードを二つの枠組みで解析した。1つ目はコンパクト連星合体からの重力波の純偏極モード探査解析である。コンパクト連星合体からの重力波観測データを、軌道傾斜角依存性を考慮して再解析し、テンソルモードが支配的であることを示した。得られた制限は先行研究を大きく上回るものであり強く一般相対論を支持する結果が得られた。2つ目はスカラー・テンソル理論などで予言されているようなスカラーとテンソルモードの混合偏極モード探査解析である。その結果、スカラーモード振幅に強重力場で最も強い一般相対性理論に無矛盾な制限を与えた。合体直前の強い重力場で付加的なスカラーモード振幅に制限を与えたのは初めてであり、現実の拡張重力理論に対する観測的知見を得た。

This study aims to investigate the anisotropy of photons in optical resonators. We have the world's highest precision in the field of signal modulation, non-continuous loop system and optical system, 6e-15 loop system and anisotropic detection. The sensitivity of the vibration sensor is limited by the vibration sensor. The sensitivity of the vibration sensor is reduced by the vibration sensor. The accuracy of the vibration sensor is high. In the same year, the speed difference of light is-17, which is the highest accuracy in the world. The speed difference of light is-17. This year, we will continue to improve the quality of our products. The gravity theory is based on the polarization of gravity waves. The properties of the degrees of freedom of gravity waves are reflected in the theory of gravity, and the polarization of gravity waves is proved to be possible. This year, the research topic is derived from GW170814 and GW 170817, and the gravity wave polarization is analyzed in two groups. 1. The analysis of gravity wave and pure polarization of star combination. The gravity wave measurement data of the satellite system and the dependence of the orbit inclination angle are taken into account in the analysis and the control of the satellite system. The results of this study are as follows: 2. The analysis of mixed polarization in the theory of polarization and polarization The results show that there is no contradiction between the strong gravity field and the general relativity theory. The strong gravitational field is added to the amplitude limit, and the initial gravitational field is measured.

项目成果

Polarization tests of GW170814 and GW170817 using waveforms consistent with alternative theories of gravity

使用与替代重力理论​​一致的波形对 GW170814 和 GW170817 进行偏振测试

• 发表时间: 2020
• 作者: Hiroki Takeda;Soichiro Morisaki;Atsushi Nishizawa
• 通讯作者: Atsushi Nishizawa

デシヘルツ重力波天文学における Ia型超新星起源の探査

分赫兹引力波天文学中Ia型超新星起源的探索

• 发表时间: 2020
• 作者: 武田 紘樹;衣川 智弥;山口 弘悦
• 通讯作者: 山口 弘悦

First cryogenic test operation of underground km-scale gravitational-wave observatory KAGRA

• DOI: 10.1088/1361-6382/ab28a9
• 发表时间: 2019-01
• 期刊: Classical and Quantum Gravity
• 影响因子: 3.5
• 作者: T. Akutsu;M. Ando;K. Arai;Y. Arai;S. Araki;A. Araya;N. Aritomi;H. Asada;Y. Aso;S. Atsuta;K. Awai;S. Bae;L. Baiotti;M. Barton;K. Cannon;E. Capocasa;C. Chen;Ting-Wai Chiu;K. Cho;Y. Chu;K. Craig;W. Creus;K. Doi;K. Eda;Y. Enomoto;R. Flaminio;Y. Fujii;M. Fujimoto;M. Fukunaga;M. Fukushima;T. Furuhata;A. Hagiwara;S. Haino;K. Hasegawa;K. Hashino;K. Hayama;S. Hirobayashi;E. Hirose;B. Hsieh;C-Z. Huang;B. Ikenoue;Y. Inoue;K. Ioka;Y. Itoh;K. Izumi;T. Kaji;T. Kajita;M. Kakizaki;M. Kamiizumi;S. Kanbara;N. Kanda;S. Kanemura;M. Kaneyama;G. Kang;J. Kasuya;Y. Kataoka;N. Kawai;Seiji Kawamura;T. Kawasaki;Chunglee Kim;J. Kim;Jimin Kim;W. Kim;Y. M. Kim;Nobuhiro Kimura;T. Kinugawa;S. Kirii;Y. Kitaoka;H. Kitazawa;Y. Kojima;K. Kokeyama;K. Komori;A. Kong;K. Kotake;R. Kozu;R. Kumar;H. Kuo;S. Kuroyanagi;Hyun Kyu Lee;Ho Lee;H. W. Lee;M. Leonardi;C. Lin;F. Lin;F. Lin;Guo-Chin Liu;Y. Liu;E. Majorana;S. Mano;M. Marchiò;T. Matsui;F. Matsushima;Y. Michimura;N. Mio;O. Miyakawa;A. Miyamoto;T. Miyamoto;K. Miyo;S. Miyoki;W. Morii;S. Morisaki;Y. Moriwaki;T. Morozumi;I. Murakami;M. Musha;K. Nagano;S. Nagano;Kouji Nakamura;Takashi Nakamura;Hiroyuki Nakano;M. Nakano;K. Nakao;Y. Namai;T. Narikawa;L. Naticchioni;L. Quynh;W. Ni;W. Ni;Atsushi Nishizawa;Y. Obuchi;T. Ochi;J. Oh;Seog Oh;M. Ohashi;N. Ohishi;M. Ohkawa;K. Okutomi;K. Ono;K. Oohara;C. Ooi;S. Pan;J. Park;F. Arellano;I. M. Pinto;N. Sago;Motoyuki Saijo;Y. Saito;S. Saitou;K. Sakai;Y. Sakai;M. Sasai;M. Sasaki;Y. Sasaki;N. Sato;S. Sato;Takashi Sato;Y. Sekiguchi;Naoki Seto;Masaru Shibata;T. Shimoda;H. Shinkai;T. Shishido;A. Shoda;K. Somiya;E. Son;A. Suemasa;T. Suzuki;H. Tagoshi;H. Tahara;H. Takahashi;R. Takahashi;A. Takamori;H. Takeda;Hidekazu Tanaka;K. Tanaka;Toshiyuki Tanaka;S. Tanioka;E. Martín;D. Tatsumi;S. Terashima;T. Tomaru;T. Tomura;F. Travasso;K. Tsubono;S. Tsuchida;N. Uchikata;T. Uchiyama;A. Ueda;T. Uehara;T. Uehara;S. Ueki;K. Ueno;F. Uraguchi;T. Ushiba;M. V. Putten;H. Vocca;S. Wada;T. Wakamatsu;Y. Watanabe;W. R. Xu;Takahiro Yamada;A. Yamamoto;Kazuhiro Yamamoto;S. Yamamoto;Takahiro Yamamoto;K. Yokogawa;J. Yokoyama;T. Yokozawa;T. Yoon;T. Yoshioka;H. Yuzurihara;S. Zeidler;Z. H. Zhu

Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA.

• DOI: 10.1007/s41114-018-0012-9
• 发表时间: 2018
• 期刊: Living reviews in relativity
• 影响因子: 40.6
• 作者: Abbott BP;Abbott R;Abbott TD;Abernathy MR;Acernese F;Ackley K;Adams C;Adams T;Addesso P;Adhikari RX;Adya VB;Affeldt C;Agathos M;Agatsuma K;Aggarwal N;Aguiar OD;Aiello L;Ain A;Ajith P;Akutsu T;Allen B;Allocca A;Altin PA;Ananyeva A;Anderson SB;Anderson WG;Ando M;Appert S;Arai K;Araya A;Araya MC;Areeda JS;Arnaud N;Arun KG;Asada H;Ascenzi S;Ashton G;Aso Y;Ast M;Aston SM;Astone P;Atsuta S;Aufmuth P;Aulbert C;Avila-Alvarez A;Awai K;Babak S;Bacon P;Bader MKM;Baiotti L;Baker PT;Baldaccini F;Ballardin G;Ballmer SW;Barayoga JC;Barclay SE;Barish BC;Barker D;Barone F;Barr B;Barsotti L;Barsuglia M;Barta D;Bartlett J;Barton MA;Bartos I;Bassiri R;Basti A;Batch JC;Baune C;Bavigadda V;Bazzan M;Bécsy B;Beer C;Bejger M;Belahcene I;Belgin M;Bell AS;Berger BK;Bergmann G;Berry CPL;Bersanetti D;Bertolini A;Betzwieser J;Bhagwat S;Bhandare R;Bilenko IA;Billingsley G;Billman CR;Birch J;Birney R;Birnholtz O;Biscans S;Bisht A;Bitossi M;Biwer C;Bizouard MA;Blackburn JK;Blackman J;Blair CD;Blair DG;Blair RM;Bloemen S;Bock O;Boer M;Bogaert G;Bohe A;Bondu F;Bonnand R;Boom BA;Bork R;Boschi V;Bose S;Bouffanais Y;Bozzi A;Bradaschia C;Brady PR;Braginsky VB;Branchesi M;Brau JE;Briant T;Brillet A;Brinkmann M;Brisson V;Brockill P;Broida JE;Brooks AF;Brown DA;Brown DD;Brown NM;Brunett S;Buchanan CC;Buikema A;Bulik T;Bulten HJ;Buonanno A;Buskulic D;Buy C;Byer RL;Cabero M;Cadonati L;Cagnoli G;Cahillane C;Calderón Bustillo J;Callister TA;Calloni E;Camp JB;Cannon KC;Cao H;Cao J;Capano CD;Capocasa E;Carbognani F;Caride S;Casanueva Diaz J;Casentini C;Caudill S;Cavaglià M;Cavalier F;Cavalieri R;Cella G;Cepeda CB;Cerboni Baiardi L;Cerretani G;Cesarini E;Chamberlin SJ;Chan M;Chao S;Charlton P;Chassande-Mottin E;Cheeseboro BD;Chen HY;Chen Y;Cheng HP;Chincarini A;Chiummo A;Chmiel T;Cho HS;Cho M;Chow JH;Christensen N;Chu Q;Chua AJK;Chua S;Chung S;Ciani G;Clara F;Clark JA;Cleva F;Cocchieri C;Coccia E;Cohadon PF;Colla A;Collette CG;Cominsky L;Constancio M Jr;Conti L;Cooper SJ;Corbitt TR;Cornish N;Corsi A;Cortese S;Costa CA;Coughlin MW;Coughlin SB;Coulon JP;Countryman ST;Couvares P;Covas PB;Cowan EE;Coward DM;Cowart MJ;Coyne DC;Coyne R;Creighton JDE;Creighton TD;Cripe J;Crowder SG;Cullen TJ;Cumming A;Cunningham L;Cuoco E;Canton TD;Danilishin SL;D'Antonio S;Danzmann K;Dasgupta A;Da Silva Costa CF;Dattilo V;Dave I;Davier M;Davies GS;Davis D;Daw EJ;Day B;Day R;De S;DeBra D;Debreczeni G;Degallaix J;De Laurentis M;Deléglise S;Del Pozzo W;Denker T;Dent T;Dergachev V;De Rosa R;DeRosa RT;DeSalvo R;Devine RC;Dhurandhar S;Díaz MC;Fiore LD;Giovanni MD;Girolamo TD;Lieto AD;Pace SD;Palma ID;Virgilio AD;Doctor Z;Doi K;Dolique V;Donovan F;Dooley KL;Doravari S;Dorrington I;Douglas R;Dovale Álvarez M;Downes TP;Drago M;Drever RWP;Driggers JC;Du Z;Ducrot M;Dwyer SE;Eda K;Edo TB;Edwards MC;Effler A;Eggenstein HB;Ehrens P;Eichholz J;Eikenberry SS;Eisenstein RA;Essick RC;Etienne Z;Etzel T;Evans M;Evans TM;Everett R;Factourovich M;Fafone V;Fair H;Fairhurst S;Fan X;Farinon S;Farr B;Farr WM;Fauchon-Jones EJ;Favata M;Fays M;Fehrmann H;Fejer MM;Fernández Galiana A;Ferrante I;Ferreira EC;Ferrini F;Fidecaro F;Fiori I;Fiorucci D;Fisher RP;Flaminio R;Fletcher M;Fong H;Forsyth SS;Fournier JD;Frasca S;Frasconi F;Frei Z;Freise A;Frey R;Frey V;Fries EM;Fritschel P;Frolov VV;Fujii Y;Fujimoto MK;Fulda P;Fyffe M;Gabbard H;Gadre BU;Gaebel SM;Gair JR;Gammaitoni L;Gaonkar SG;Garufi F;Gaur G;Gayathri V;Gehrels N;Gemme G;Genin E;Gennai A;George J;Gergely L;Germain V;Ghonge S;Ghosh A;Ghosh A;Ghosh S;Giaime JA;Giardina KD;Giazotto A;Gill K;Glaefke A;Goetz E;Goetz R;Gondan L;González G;Gonzalez Castro JM;Gopakumar A;Gorodetsky ML;Gossan SE;Gosselin M;Gouaty R;Grado A;Graef C;Granata M;Grant A;Gras S;Gray C;Greco G;Green AC;Groot P;Grote H;Grunewald S;Guidi GM;Guo X;Gupta A;Gupta MK;Gushwa KE;Gustafson EK;Gustafson R;Hacker JJ;Hagiwara A;Hall BR;Hall ED;Hammond G;Haney M;Hanke MM;Hanks J;Hanna C;Hannam MD;Hanson J;Hardwick T;Harms J;Harry GM;Harry IW;Hart MJ;Hartman MT;Haster CJ;Haughian K;Hayama K;Healy 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V;Razzano M;Re V;Read J;Regimbau T;Rei L;Reid S;Reitze DH;Rew H;Reyes SD;Rhoades E;Ricci F;Riles K;Rizzo M;Robertson NA;Robie R;Robinet F;Rocchi A;Rolland L;Rollins JG;Roma VJ;Romano R;Romie JH;Rosińska D;Rowan S;Rüdiger A;Ruggi P;Ryan K;Sachdev S;Sadecki T;Sadeghian L;Sago N;Saijo M;Saito Y;Sakai K;Sakellariadou M;Salconi L;Saleem M;Salemi F;Samajdar A;Sammut L;Sampson LM;Sanchez EJ;Sandberg V;Sanders JR;Sasaki Y;Sassolas B;Sathyaprakash BS;Sato S;Sato T;Saulson PR;Sauter O;Savage RL;Sawadsky A;Schale P;Scheuer J;Schmidt E;Schmidt J;Schmidt P;Schnabel R;Schofield RMS;Schönbeck A;Schreiber E;Schuette D;Schutz BF;Schwalbe SG;Scott J;Scott SM;Sekiguchi T;Sekiguchi Y;Sellers D;Sengupta AS;Sentenac D;Sequino V;Sergeev A;Setyawati Y;Shaddock DA;Shaffer TJ;Shahriar MS;Shapiro B;Shawhan P;Sheperd A;Shibata M;Shikano Y;Shimoda T;Shoda A;Shoemaker DH;Shoemaker DM;Siellez K;Siemens X;Sieniawska M;Sigg D;Silva AD;Singer A;Singer LP;Singh A;Singh R;Singhal A;Sintes AM;Slagmolen BJJ;Smith B;Smith JR;Smith RJE;Somiya K;Son EJ;Sorazu B;Sorrentino F;Souradeep T;Spencer AP;Srivastava AK;Staley A;Steinke M;Steinlechner J;Steinlechner S;Steinmeyer D;Stephens BC;Stevenson SP;Stone R;Strain KA;Straniero N;Stratta G;Strigin SE;Sturani R;Stuver AL;Sugimoto Y;Summerscales TZ;Sun L;Sunil S;Sutton PJ;Suzuki T;Swinkels BL;Szczepańczyk MJ;Tacca M;Tagoshi H;Takada S;Takahashi H;Takahashi R;Takamori A;Talukder D;Tanaka H;Tanaka K;Tanaka T;Tanner DB;Tápai M;Taracchini A;Tatsumi D;Taylor R;Telada S;Theeg T;Thomas EG;Thomas M;Thomas P;Thorne KA;Thrane E;Tippens T;Tiwari S;Tiwari V;Tokmakov KV;Toland K;Tomaru T;Tomlinson C;Tonelli M;Tornasi Z;Torrie CI;Töyrä D;Travasso F;Traylor G;Trifirò D;Trinastic J;Tringali MC;Trozzo L;Tse M;Tso R;Tsubono K;Tsuzuki T;Turconi M;Tuyenbayev D;Uchiyama T;Uehara T;Ueki S;Ueno K;Ugolini D;Unnikrishnan CS;Urban AL;Ushiba T;Usman SA;Vahlbruch H;Vajente G;Valdes G;van Bakel N;van Beuzekom M;van den Brand JFJ;Van Den Broeck C;Vander-Hyde DC;van der Schaaf L;van 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Collaboration
• 通讯作者: KAGRA Collaboration, LIGO Scientific Collaboration and Virgo Collaboration

インスパイラル重力波のスカラーテンソル混合偏極探査

螺旋引力波的标量张量混合偏振探索

• 发表时间: 2021
• 作者: 武田紘樹;森崎宗一郎;西澤篤志
• 通讯作者: 西澤篤志