196 research outputs found
Structural Evolution in a Melt-Quenched Zeolitic Imidazolate Framework Glass during Heat-treatment
- Author
- Publication venue
- 'Royal Society of Chemistry (RSC)'
- Publication date
- 04/02/2019
- Field of study
Lepton Flavor Violation in Z and Lepton Decays in Supersymmetric Models
- Author
- A. Dobado
- A. Ilakovac
- A. Pilaftsis
- C.x. Yue
- D. Atwood
- D. Delepine
- D.E. Groom
- D.F. Carvalho
- D.F. Carvalho
- D.W. Bliss
- E.O. Iltan
- F. Borzumati
- F. Gabbiani
- F. Gabbiani
- G. Passarino
- G. ât Hooft
- G.J. van Oldenborgh
- G.W. Bennett
- G.W. Bennett
- H.N. Brown
- I. Blokland
- I. Hinchliffe
- J. Bernabéu
- J. Bijnens
- J. Hisano
- J. Hisano
- J. Hisano
- J. Hisano
- J. I. Illana
- J.I. Illana
- J.L. Feng
- K.W. Edwards
- M. Apollonio
- M. Frank
- M. Frank
- M. Knecht
- M. Knecht
- M. Masip
- M.J. Levine
- M.L. Brooks
- N. Arkani-Hamed
- P. Abreu
- P. Langacker
- R. Akers
- R.N. Mohapatra
- S. Ahmed
- S.w. Baek
- T. Appelquist
- T. Hahn
- T. Moroi
- T. Moroi
- T. Yanagida
- U. Bellgardt
- W. Hollik
- W. Hollik
- Z. Chacko
- Publication venue
- 'American Physical Society (APS)'
- Publication date
- 01/01/2002
- Field of study
The observation of charged lepton flavor non-conservation would be a clear
signature of physics beyond the Standard Model. In particular, supersymmetric
(SUSY) models introduce mixings in the sneutrino and the charged slepton
sectors which could imply flavor-changing processes at rates accessible to
upcoming experiments. In this paper we analyze the possibility to observe Z -->
lep_I lep_J in the GigaZ option of TESLA at DESY. We show that although models
with SUSY masses above the current limits could predict a branching ratio BR(Z
--> mu e) accessible to the experiment, they would imply an unobserved rate of
mu --> e gamma and thus are excluded. In models with a small mixing angle
between the first and the third (or the second and the third) slepton families
GigaZ could observe Z --> tau mu (or Z --> tau e) consistently with present
bounds on lep_J --> lep_I gamma. In contrast, if the mixing angles between the
three slepton families are large the bounds from mu --> e gamma push these
processes below the reach of GigaZ. We show that in this case the masses of the
three slepton families must be strongly degenerated (with mass differences of
order 10^{-3}). We update the limits on the slepton mass insertions
delta_{LL,RR,LR} and discuss the correlation between flavor changing and g_mu-2
in SUSY models.Comment: 23 pages, 6 figures. Version to appear in Phys. Rev.
Cosmological distance indicators
- Author
- A. Agnello
- A. Eigenbrod
- A. Goobar
- A. Hojjati
- A. Hojjati
- A. More
- A. Oscoz
- A.G. Riess
- A.M. Martin
- A.S. Tagore
- B.J. Brewer
- C. Alcock
- C. Grillo
- C. Hazard
- C. McCully
- C. Vanderriest
- C. Vuissoz
- C. Vuissoz
- C.D. Fassnacht
- C.D. Fassnacht
- C.D. Fassnacht
- C.E. Rusu
- C.L. Bennett
- C.S. Kochanek
- C.S. Kochanek
- C.W. Morgan
- D. Paraficz
- D. Sluse
- D. Walsh
- D.A. Goldstein
- D.A. Goldstein
- D.H. Weinberg
- D.J. Eisenstein
- D.J. Eisenstein
- E. Eulaers
- E. Giannini
- E. Jullo
- E.E. Falco
- E.O. Ofek
- E.R. Switzer
- F. Courbin
- F. Courbin
- F. Courbin
- F.B. Abdalla
- G. Dobler
- G. Dobler
- G. Efstathiou
- G. Golse
- G.C.F. Chen
- H. Lin
- H.J. Seo
- H.J. Seo
- I. Burud
- I. Burud
- I. Burud
- I. Jee
- I. Momcheva
- J. Fohlmeister
- J. Fohlmeister
- J. Hjorth
- J. Huchra
- J. Lehar
- J.R. Shaw
- J.R. Shaw
- J.W. Nightingale
- K. Bandura
- K. Liao
- K.C. Wong
- K.S. Dawson
- K.W. Masui
- K.W. Masui
- L. Amendola
- L. Anderson
- L. Oldham
- L.B. Newburgh
- L.J. Hainline
- L.L.R. Williams
- L.V.E. Koopmans
- L.V.E. Koopmans
- L.V.E. Koopmans
- L.V.E. Koopmans
- M. BarnabĂš
- M. BarnabĂš
- M. Cappellari
- M. Jauzac
- M. Oguri
- M. Oguri
- M. Oguri
- M. Schmidt
- M. Sereno
- M. Takada
- M. Tegmark
- M. Tegmark
- M. Tewes
- M. Tewes
- M.A. Zwaan
- M.J. Drinkwater
- N. Cantale
- N. Kaiser
- N.A. Grogin
- O. Wucknitz
- P. Bull
- P. Jakobsson
- P. Magain
- P. Magain
- P. Saha
- P. Schneider
- P. Schneider
- P. Schneider
- P. Schneider
- P. Young
- P.A.R. Ade
- P.J. Marshall
- P.J.E. Peebles
- P.L. Kelly
- P.L. Kelly
- P.L. Kelly
- P.L. Schechter
- R. Adam
- R. Barkana
- R. Blandford
- R. Blandford
- R. Fadely
- R. Gavazzi
- R. Kawamata
- R. Kormann
- R.B. Wayth
- S. Birrer
- S. Cole
- S. Dye
- S. Hilbert
- S. Rathna Kumar
- S. Rathna Kumar
- S. Refsdal
- S. Vegetti
- S. Wallington
- S. Wyithe
- S.A. Rodney
- S.H. Suyu
- S.H. Suyu
- S.H. Suyu
- S.H. Suyu
- S.H. Suyu
- S.H. Suyu
- S.H. Suyu
- S.H. Suyu
- S.J. Warren
- S.S. Tie
- T. KundiÄ
- T. Matsubara
- T. Okumura
- T. Okumura
- T. Treu
- T.C. Chang
- T.C. Chang
- T.E. Collett
- V. Bonvin
- V. Bonvin
- V.N. Shalyapin
- W. Hu
- W.L. Freedman
- W.N. Colley
- X. FernĂĄndez
- Y. Xu
- Y.W. Liao
- Z.S. Greene
- Ă. Aubourg
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- 22/07/2018
- Field of study
We review three distance measurement techniques beyond the local universe:
(1) gravitational lens time delays, (2) baryon acoustic oscillation (BAO), and
(3) HI intensity mapping. We describe the principles and theory behind each
method, the ingredients needed for measuring such distances, the current
observational results, and future prospects. Time delays from strongly lensed
quasars currently provide constraints on H0â with < 4% uncertainty, and with
1% within reach from ongoing surveys and efforts. Recent exciting discoveries
of strongly lensed supernovae hold great promise for time-delay cosmography.
BAO features have been detected in redshift surveys up to z <~ 0.8 with
galaxies and z ~ 2 with Ly-α forest, providing precise distance
measurements and H0â with < 2% uncertainty in flat ÎCDM. Future BAO
surveys will probe the distance scale with percent-level precision. HI
intensity mapping has great potential to map BAO distances at z ~ 0.8 and
beyond with precisions of a few percent. The next years ahead will be exciting
as various cosmological probes reach 1% uncertainty in determining H0â, to
assess the current tension in H0â measurements that could indicate new
physics.Comment: Review article accepted for publication in Space Science Reviews
(Springer), 45 pages, 10 figures. Chapter of a special collection resulting
from the May 2016 ISSI-BJ workshop on Astronomical Distance Determination in
the Space Ag
SARS-CoV-2 mRNA vaccine design enabled by prototype pathogen preparedness
- Author
- Abiona O.M.
- Altaras N.E.
- Alvarado G.S.
- Bahl K.
- Baric R.S.
- Bennett H.
- Bock K.W.
- Boyoglu-Barnum S.
- Carfi A.
- Chang L.A.
- Chappell J.D.
- Corbett K.S.
- Denison M.R.
- Dinnon K.H.
- DiPiazza A.T.
- Doria-Rose N.A.
- Edwards D.K.
- Elbashir S.M.
- Fritch E.J.
- Garcia-Dominguez D.
- Gillespie R.A.
- Graham B.S.
- Gully K.L.
- Henry C.
- Himansu S.
- Hutchinson G.B.
- Kong W.-P.
- Leist S.R.
- Leung K.
- Liu C.
- Loomis R.J.
- Louder M.K.
- Ma L.Z.
- Martinez D.R.
- Mascola J.R.
- McLellan J.S.
- Metkar M.
- Minai M.
- Moore I.N.
- Morabito K.M.
- Nagata B.M.
- Narayanan E.
- Nason M.C.
- Phung E.
- Presnyak V.
- Renzi I.
- Ruckwardt T.J.
- Schmidt S.D.
- SchÀfer A.
- Shaw C.A.
- Shi W.
- Stevens L.J.
- Stewart-Jones G.
- Wang L.
- Wang N.
- West A.
- Woods A.
- Wrapp D.
- Wu K.
- Yang E.S.
- Zhang Y.
- Ziwawo C.T.
- Publication venue
- Publication date
- 01/01/2020
- Field of study
A vaccine for severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2) is needed to control the coronavirus disease 2019 (COVID-19) global pandemic. Structural studies have led to the development of mutations that stabilize Betacoronavirus spike proteins in the prefusion state, improving their expression and increasing immunogenicity1. This principle has been applied to design mRNA-1273, an mRNA vaccine that encodes a SARS-CoV-2 spike protein that is stabilized in the prefusion conformation. Here we show that mRNA-1273 induces potent neutralizing antibody responses to both wild-type (D614) and D614G mutant2 SARS-CoV-2 as well as CD8+ T cell responses, and protects against SARS-CoV-2 infection in the lungs and noses of mice without evidence of immunopathology. mRNA-1273 is currently in a phase III trial to evaluate its efficacy
A survey of research in the application of tolerance analysis to the design of mechanical assemblies
- Author
- A. Mallik
- A. Wirtz
- A.A.G. Requicha
- A.A.G. Requicha
- Alan R. Parkinson
- C.A. Gladman
- D. Wilde
- D.B. Parkinson
- D.B. Parkinson
- D.C. Gossard
- D.H. Evans
- D.H. Evans
- D.H. Evans
- D.H. Evans
- D.H. Evans
- D.H. Evans
- D.H. Evans
- E. Mansoor
- F. Etesami
- F.H. Speckhart
- G. Bennett
- G. H. Sutherland
- I.D. Faux
- J. Baumgarten
- J. Turner
- J. Turner
- J. Turner
- J.C.H. Chung
- K.W. Chase
- K.W. Chase
- Kenneth W. Chase
- M.F. Spotts
- N.D. Cox
- P.F. Ostwald
- R. Fenton
- R. Garrett
- R. Jayaraman
- R. Light
- R.J. Eggert
- S. Dhande
- S. Dhande
- S. Levy
- S. Srikanth
- V. Srinivasan
- W. Lee
- W. Lee
- W. Michael
- W. Michael
- W.H. Greenwood
- W.H. Greenwood
- W.H. Greenwood
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- Field of study
Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3b
- Author
- Abbott R.
- Abbott T.D.
- Acernese F.
- Ackley K.
- Adams C.
- Adhikari N.
- Adhikari R.X.
- Adya V.B.
- Affeldt C.
- Agarwal D.
- Agathos M.
- Agatsuma K.
- Aggarwal N.
- Aguiar O.D.
- Aiello L.
- Ain A.
- Ajith P.
- Akutsu T.
- Albanesi S.
- Allocca A.
- Altin P.A.
- Amato A.
- Anand C.
- Anand S.
- Ananyeva A.
- Anderson S.B.
- Anderson W.G.
- Ando M.
- Andrade T.
- Andres N.
- AndriÄ T.
- Angelova S.V.
- Ansoldi S.
- Antelis J.M.
- Antier S.
- Appert S.
- Arai Koji
- Arai Koya
- Arai Y.
- Araki S.
- Araya A.
- Araya M.C.
- Areeda J.S.
- Arellano F. E. Peña
- Aritomi N.
- Arnaud N.
- Aronson S.M.
- Arun K.G.
- ArĂšne M.
- Asada H.
- Asali Y.
- Ashton G.
- Aso Y.
- Assiduo M.
- Aston S.M.
- Astone P.
- Aubin F.
- Austin C.
- Babak S.
- Badaracco F.
- Bader M.K.M.
- Badger C.
- Bae S.
- Bae Y.
- Baer A.M.
- Bagnasco S.
- Bai Y.
- Baiotti L.
- Baird J.
- Bajpai R.
- Ball M.
- Ballardin G.
- Ballmer S.W.
- Balsamo A.
- Baltus G.
- Banagiri S.
- Bankar D.
- Barayoga J.C.
- Barbieri C.
- Barish B.C.
- Barker D.
- Barneo P.
- Barone F.
- Barr B.
- Barsotti L.
- Barsuglia M.
- Barta D.
- Bartlett J.
- Barton M.A.
- Bartos I.
- Bassiri R.
- Basti A.
- Bawaj M.
- Bayley J.C.
- Baylor A.C.
- Bazzan M.
- Bedakihale V.M.
- Bejger M.
- Belahcene I.
- Benedetto V.
- Beniwal D.
- Bennett T.F.
- Bentley J.D.
- Benyaala M.
- Bergamin F.
- Berger B.K.
- Bernuzzi S.
- Berry C.P.L.
- Bersanetti D.
- Bertolini A.
- Betzwieser J.
- Beveridge D.
- Bhandare R.
- Bhardwaj U.
- Bhattacharjee D.
- Bhaumik S.
- Bilenko I.A.
- Billingsley G.
- Bini S.
- Birney R.
- Birnholtz O.
- Biscans S.
- Bischi M.
- Biscoveanu S.
- Bisht A.
- Biswas B.
- Bitossi M.
- Bizouard M.-A.
- Blackburn J.K.
- Blair C.D.
- Blair D.G.
- Blair R.M.
- Bobba F.
- Bode N.
- Boer M.
- Bogaert G.
- Boldrini M.
- Bonavena L.D.
- Bondu F.
- Bonilla E.
- Bonnand R.
- Booker P.
- Boom B.A.
- Bork R.
- Boschi V.
- Bose N.
- Bose S.
- Bossilkov V.
- Boudart V.
- Bouffanais Y.
- Bozzi A.
- Bradaschia C.
- Brady P.R.
- Bramley A.
- Branch A.
- Branchesi M.
- Brau J.E.
- Breschi M.
- Briant T.
- Briggs J.H.
- Brillet A.
- Brinkmann M.
- Brockill P.
- Brooks A.F.
- Brooks J.
- Brown D.D.
- Brunett S.
- Bruno G.
- Bruntz R.
- Bryant J.
- Bulik T.
- Bulten H.J.
- Buonanno A.
- Buscicchio R.
- Buskulic D.
- Bustillo J. CalderĂłn
- Buy C.
- Byer R.L.
- BĂ©csy B.
- Cadonati L.
- Cagnoli G.
- Cahillane C.
- Callaghan J.D.
- Callister T.A.
- Calloni E.
- Cameron J.
- Camp J.B.
- Canepa M.
- Canevarolo S.
- Cannavacciuolo M.
- Cannon K.C.
- Canton T. Dal
- Cao H.
- Cao Z.
- Capocasa E.
- Capote E.
- Carapella G.
- Carbognani F.
- Carlin J.B.
- Carney M.F.
- Carpinelli M.
- Carrillo G.
- Carullo G.
- Carver T.L.
- Casentini C.
- Castaldi G.
- Caudill S.
- CavagliĂ M.
- Cavalier F.
- Cavalieri R.
- Ceasar M.
- Cella G.
- CerdĂĄ-DurĂĄn P.
- Cesarini E.
- Chaibi W.
- Chakravarti K.
- Champion E.
- Chan C.
- Chan C.-H.
- Chan C.L.
- Chan K.
- Chan M.
- Chandra K.
- Chanial P.
- Chao S.
- Charlton P.
- Chase E.A.
- Chassande-Mottin E.
- Chatterjee C.
- Chatterjee Debarati
- Chatterjee Deep
- Chaturvedi M.
- Chaty S.
- Chatziioannou K.
- Chen C.
- Chen H.Y.
- Chen J.
- Chen K.
- Chen X.
- Chen Y.-B.
- Chen Y.-R.
- Chen Z.
- Cheng H.
- Cheong C.K.
- Cheung H.Y.
- Chia H.Y.
- Chiadini F.
- Chiang C.-Y.
- Chiarini G.
- Chierici R.
- Chincarini A.
- Chiofalo M.L.
- Chiummo A.
- Cho G.
- Cho H.S.
- Choudhary R.K.
- Choudhary S.
- Christensen N.
- Chu H.
- Chu Q.
- Chu Y.-K.
- Chua S.
- Chung K.W.
- Ciani G.
- Ciecielag P.
- CieĆlar M.
- Cifaldi M.
- Ciobanu A.A.
- Ciolfi R.
- Cipriano F.
- Cirone A.
- Clara F.
- Clark E.N.
- Clark J.A.
- Clarke L.
- Clearwater P.
- Clesse S.
- Cleva F.
- Coccia E.
- Codazzo E.
- Cohadon P.-F.
- Cohen D.E.
- Cohen L.
- Colleoni M.
- Collette C.G.
- Colombo A.
- Colpi M.
- Compton C.M.
- Constancio M.
- Conti L.
- Cooper S.J.
- Corban P.
- Corbitt T.R.
- Cordero-CarriĂłn I.
- Corezzi S.
- Corley K.R.
- Cornish N.
- Corre D.
- Corsi A.
- Cortese S.
- Costa C.A.
- Cotesta R.
- Coughlin M.W.
- Coulon J.-P.
- Countryman S.T.
- Cousins B.
- Couvares P.
- Coward D.M.
- Cowart M.J.
- Coyne D.C.
- Coyne R.
- Creighton J.D.E.
- Creighton T.D.
- Criswell A.W.
- Croquette M.
- Crowder S.G.
- Cudell J.R.
- Cullen T.J.
- Cumming A.
- Cummings R.
- Cunningham L.
- Cuoco E.
- CuryĆo M.
- D'Angelo B.
- D'Antonio S.
- D'Emilio V.
- D'Onofrio L.
- D'Urso D.
- Dabadie P.
- Dall'Osso S.
- Dana A.
- Daneshgaranbajastani L.M.
- Danilishin S.
- Danzmann K.
- Darsow-Fromm C.
- Dasgupta A.
- Datrier L.E.H.
- Datta S.
- Dattilo V.
- Dave I.
- Davier M.
- Davies G.S.
- Davis D.
- Davis M.C.
- Daw E.J.
- Dean R.
- Debra D.
- Deenadayalan M.
- Degallaix J.
- Deléglise S.
- Demarchi L.M.
- Demos N.
- Dent T.
- Depasse A.
- Desalvo R.
- Dhurandhar S.
- Diaz J. Casanueva
- Diaz-Ortiz M.
- Didio N.A.
- Dietrich T.
- Ding B.
- Divakarla A.K.
- Dmitriev A.
- Doctor Z.
- Donovan F.
- Dooley K.L.
- Doravari S.
- Dorrington I.
- Drago M.
- Driggers J.C.
- Drori Y.
- Ducoin J.-G.
- Dupej P.
- Durante O.
- Duverne P.-A.
- Dwyer S.E.
- DĂĄlya G.
- DĂaz M.C.
- E Melo I. Tosta
- Eassa C.
- Easter P.J.
- Ebersold M.
- Eckhardt T.
- Eddolls G.
- Edelman B.
- Edo T.B.
- Edy O.
- Effler A.
- Eguchi S.
- Eichholz J.
- Eikenberry S.S.
- Eisenmann M.
- Eisenstein R.A.
- Ejlli A.
- Engelby E.
- Enomoto Y.
- Errico L.
- Essick R.C.
- Estellés H.
- Estevez D.
- Etienne Z.
- Etzel T.
- Evans M.
- Evans T.M.
- Ewing B.E.
- Fafone V.
- Fair H.
- Fairhurst S.
- Farah A.M.
- Farinon S.
- Farr B.
- Farr W.M.
- Farrow N.W.
- Fauchon-Jones E.J.
- Favaro G.
- Favata M.
- Favero V. Del
- Fays M.
- Fazio M.
- Feicht J.
- Fejer M.M.
- Fenyvesi E.
- Ferguson D.L.
- Fernandez-Galiana A.
- Ferrante I.
- Ferreira T.A.
- Fidecaro F.
- Figura P.
- Fiore L. Di
- Fiori I.
- Fishbach M.
- Fisher R.P.
- Fittipaldi R.
- Fiumara V.
- Flaminio R.
- Floden E.
- Fong H.
- Font J.A.
- Fornal B.
- Forsyth P.W.F.
- Franke A.
- Frasca S.
- Frasconi F.
- Frederick C.
- Freed J.P.
- Frei Z.
- Freise A.
- Frey R.
- Fritschel P.
- Frolov V.V.
- Fronzo C. Di
- Fronzé G.G.
- Fujii Y.
- Fujikawa Y.
- Fukunaga M.
- Fukushima M.
- Fulda P.
- Fyffe M.
- Gabbard H.A.
- Gadre B.U.
- Gair J.R.
- Gais J.
- Galaudage S.
- Gamba R.
- Ganapathy D.
- Ganguly A.
- Gao D.
- Gaonkar S.G.
- Garaventa B.
- GarcĂa-NĂșñez C.
- GarcĂa-QuirĂłs C.
- Garufi F.
- Gateley B.
- Gaudio S.
- Gayathri V.
- Ge G.-G.
- Gemme G.
- Gennai A.
- George J.
- Gerberding O.
- Gergely L.
- Gewecke P.
- Ghonge S.
- Ghosh Abhirup
- Ghosh Archisman
- Ghosh Shaon
- Ghosh Shrobana
- Giacomazzo B.
- Giacoppo L.
- Giaime J.A.
- Giardina K.D.
- Gibson D.R.
- Gier C.
- Giesler M.
- Giorgio C. Di
- Giovanni F. Di
- Giovanni M. Di
- Giri P.
- Girolamo T. Di
- Gissi F.
- Glanzer J.
- Gleckl A.E.
- Godwin P.
- Goetz E.
- Goetz R.
- Gohlke N.
- Goncharov B.
- GonzĂĄlez G.
- Gopakumar A.
- Gosselin M.
- Gouaty R.
- Gould D.W.
- Grace B.
- Grado A.
- Granata M.
- Granata V.
- Grant A.
- Gras S.
- Grassia P.
- Gray C.
- Gray R.
- Greco G.
- Green A.C.
- Green R.
- Gretarsson A.M.
- Gretarsson E.M.
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- Xiao L.
- Xu W.-R.
- Yamada T.
- Yamamoto H.
- Yamamoto Kazuhiro
- Yamamoto Kohei
- Yamamoto T.
- Yamashita K.
- Yamazaki R.
- Yang F.W.
- Yang L.
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- Yang Yang
- Yang Z.
- Yap M.J.
- Yeeles D.W.
- Yelikar A.B.
- Ying M.
- Yokogawa K.
- Yokoyama J.
- Yokozawa T.
- Yoo J.
- Yoshioka T.
- Yu Hang
- Yu Haocun
- Yuzurihara H.
- Zadrzny A.
- Zanolin M.
- Zeidler S.
- Zelenova T.
- Zendri J.-P.
- Zevin M.
- Zhan M.
- Zhang H.
- Zhang J.
- Zhang L.
- Zhang T.
- Zhang Y.
- Zhao C.
- Zhao G.
- Zhao Y.
- Zhao Yue
- Zheng Y.
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- Zhou Z.
- Zhu X.J.
- Zhu Z.-H.
- Zimmerman A.B.
- Zucker M.E.
- Zweizig J.
- Publication venue
- London : Institute of Physics Publ.
- Publication date
- 01/01/2022
- Field of study
We search for gravitational-wave signals associated with gamma-ray bursts (GRBs) detected by the Fermi and Swift satellites during the second half of the third observing run of Advanced LIGO and Advanced Virgo (2019 November 1 15:00 UTC-2020 March 27 17:00 UTC). We conduct two independent searches: A generic gravitational-wave transients search to analyze 86 GRBs and an analysis to target binary mergers with at least one neutron star as short GRB progenitors for 17 events. We find no significant evidence for gravitational-wave signals associated with any of these GRBs. A weighted binomial test of the combined results finds no evidence for subthreshold gravitational-wave signals associated with this GRB ensemble either. We use several source types and signal morphologies during the searches, resulting in lower bounds on the estimated distance to each GRB. Finally, we constrain the population of low-luminosity short GRBs using results from the first to the third observing runs of Advanced LIGO and Advanced Virgo. The resulting population is in accordance with the local binary neutron star merger rate. © 2022. The Author(s). Published by the American Astronomical Society
Narrowband Searches for Continuous and Long-duration Transient Gravitational Waves from Known Pulsars in the LIGO-Virgo Third Observing Run
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- Ying M.
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- Yuzurihara H.
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- Zweizig J.
- Publication venue
- London : Institute of Physics Publ.
- Publication date
- 01/01/2022
- Field of study
Isolated neutron stars that are asymmetric with respect to their spin axis are possible sources of detectable continuous gravitational waves. This paper presents a fully coherent search for such signals from eighteen pulsars in data from LIGO and Virgo's third observing run (O3). For known pulsars, efficient and sensitive matched-filter searches can be carried out if one assumes the gravitational radiation is phase-locked to the electromagnetic emission. In the search presented here, we relax this assumption and allow both the frequency and the time derivative of the frequency of the gravitational waves to vary in a small range around those inferred from electromagnetic observations. We find no evidence for continuous gravitational waves, and set upper limits on the strain amplitude for each target. These limits are more constraining for seven of the targets than the spin-down limit defined by ascribing all rotational energy loss to gravitational radiation. In an additional search, we look in O3 data for long-duration (hours-months) transient gravitational waves in the aftermath of pulsar glitches for six targets with a total of nine glitches. We report two marginal outliers from this search, but find no clear evidence for such emission either. The resulting duration-dependent strain upper limits do not surpass indirect energy constraints for any of these targets. © 2022. The Author(s). Published by the American Astronomical Society
Proceedings of the 2016 Childhood Arthritis and Rheumatology Research Alliance (CARRA) Scientific Meeting
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J. Kaprio, S. Ripatti ja M.-L. Lokki työryhmien jÀseniÀ.Peer reviewe
Search for gravitational-wave transients associated with magnetar bursts in advanced LIGO and advanced Virgo data from the third observing run
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- Yeh S.-W
- Yelikar A.B
- Ying M
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- Zhao Yue
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- Zhu X.J
- Zhu Z.-H
- Zucker M.E
- Zweizig J
- Publication venue
- American Astronomical Society
- Publication date
- 01/01/2024
- Field of study
Gravitational waves are expected to be produced from neutron star oscillations associated with magnetar giant f lares and short bursts. We present the results of a search for short-duration (milliseconds to seconds) and longduration (âŒ100 s) transient gravitational waves from 13 magnetar short bursts observed during Advanced LIGO, Advanced Virgo, and KAGRAâs third observation run. These 13 bursts come from two magnetars, SGR1935 +2154 and SwiftJ1818.0â1607. We also include three other electromagnetic burst events detected by FermiGBM which were identified as likely coming from one or more magnetars, but they have no association with a known magnetar. No magnetar giant flares were detected during the analysis period. We find no evidence of gravitational waves associated with any of these 16 bursts. We place upper limits on the rms of the integrated incident gravitational-wave strain that reach 3.6 Ă 10âÂČÂł Hz at 100 Hz for the short-duration search and 1.1 Ă10âÂČÂČ Hz at 450 Hz for the long-duration search. For a ringdown signal at 1590 Hz targeted by the short-duration search the limit is set to 2.3 Ă 10âÂČÂČ Hz. Using the estimated distance to each magnetar, we derive upper limits upper limits on the emitted gravitational-wave energy of 1.5 Ă 1044 erg (1.0 Ă 1044 erg) for SGR 1935+2154 and 9.4 Ă 10^43 erg (1.3 Ă 1044 erg) for Swift J1818.0â1607, for the short-duration (long-duration) search. Assuming isotropic emission of electromagnetic radiation of the burst ïŹuences, we constrain the ratio of gravitational-wave energy to electromagnetic energy for bursts from SGR 1935+2154 with the available ïŹuence information. The lowest of these ratios is 4.5 Ă 103
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