BibTex format
@article{Armano:2025:10.1103/PhysRevLett.134.071401,
author = {Armano, M and Audley, H and Baird, J and Binetruy, P and Born, M and Bortoluzzi, D and Castelli, E and Cavalleri, A and Cesarini, A and Cruise, AM and Danzmann, K and de, Deus Silva M and Diepholz, I and Dixon, G and Dolesi, R and Ferraioli, L and Ferroni, V and Fitzsimons, ED and Freschi, M and Gesa, L and Giardini, D and Gibert, F and Giusteri, R and Grimani, C and Grzymisch, J and Harrison, I and Hartig, M-S and Heinzel, G and Hewitson, M and Hollington, D and Hoyland, D and Hueller, M and Inchauspé, H and Jennrich, O and Jetzer, P and Karnesis, N and Kaune, B and Korsakova, N and Killow, CJ and Liu, L and Lobo, JA and López-Zaragoza, JP and Maarschalkerweerd, R and Mance, D and Martín, V and Martin-Polo, L and Martin-Porqueras, F and Martino, J and McNamara, PW and Mendes, J and Mendes, L and Meshksar, N and Nofrarias, M and Paczkowski, S and Perreur-Lloyd, M and Petiteau, A and Pivato, P and Plagnol, E and Ramos-Castro, J and Reiche, J and Rivas, F and Robertson, DI and Russano, G},
doi = {10.1103/PhysRevLett.134.071401},
journal = {Phys Rev Lett},
title = {Magnetic-Induced Force Noise in LISA Pathfinder Free-Falling Test Masses.},
url = {http://dx.doi.org/10.1103/PhysRevLett.134.071401},
volume = {134},
year = {2025}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - LISA Pathfinder was a mission designed to test key technologies required for gravitational wave detection in space. Magnetically driven forces play a key role in the instrument sensitivity in the low-frequency regime, which corresponds to the measurement band of interest for future space-borne gravitational wave observatories. Magnetically induced forces couple to the test mass motion, introducing a contribution to the relative acceleration noise between the free-falling test masses. In this Letter we present the first complete estimate of this term of the instrument performance model. Our results set the magnetic-induced acceleration noise during the February 2017 noise run of 0.25_{-0.08}^{+0.15} fm s^{-2}/sqrt[Hz] at 1 mHz and 1.01_{-0.24}^{+0.73} fm s^{-2}/sqrt[Hz] at 0.1 mHz. We also discuss how the nonstationarities of the interplanetary magnetic field can affect these values during extreme space weather conditions.
AU - Armano,M
AU - Audley,H
AU - Baird,J
AU - Binetruy,P
AU - Born,M
AU - Bortoluzzi,D
AU - Castelli,E
AU - Cavalleri,A
AU - Cesarini,A
AU - Cruise,AM
AU - Danzmann,K
AU - de,Deus Silva M
AU - Diepholz,I
AU - Dixon,G
AU - Dolesi,R
AU - Ferraioli,L
AU - Ferroni,V
AU - Fitzsimons,ED
AU - Freschi,M
AU - Gesa,L
AU - Giardini,D
AU - Gibert,F
AU - Giusteri,R
AU - Grimani,C
AU - Grzymisch,J
AU - Harrison,I
AU - Hartig,M-S
AU - Heinzel,G
AU - Hewitson,M
AU - Hollington,D
AU - Hoyland,D
AU - Hueller,M
AU - Inchauspé,H
AU - Jennrich,O
AU - Jetzer,P
AU - Karnesis,N
AU - Kaune,B
AU - Korsakova,N
AU - Killow,CJ
AU - Liu,L
AU - Lobo,JA
AU - López-Zaragoza,JP
AU - Maarschalkerweerd,R
AU - Mance,D
AU - Martín,V
AU - Martin-Polo,L
AU - Martin-Porqueras,F
AU - Martino,J
AU - McNamara,PW
AU - Mendes,J
AU - Mendes,L
AU - Meshksar,N
AU - Nofrarias,M
AU - Paczkowski,S
AU - Perreur-Lloyd,M
AU - Petiteau,A
AU - Pivato,P
AU - Plagnol,E
AU - Ramos-Castro,J
AU - Reiche,J
AU - Rivas,F
AU - Robertson,DI
AU - Russano,G
AU - Sala,L
AU - Serrano,D
AU - Slutsky,J
AU - Sopuerta,CF
AU - Sumner,T
AU - Texier,D
AU - Thorpe,JI
AU - Vetrugno,D
AU - Vitale,S
AU - Wanner,G
AU - Ward,H
AU - Wass,PJ
AU - Weber,WJ
AU - Wissel,L
AU - Wittchen,A
AU - Zweifel,P
DO - 10.1103/PhysRevLett.134.071401
PY - 2025///
TI - Magnetic-Induced Force Noise in LISA Pathfinder Free-Falling Test Masses.
T2 - Phys Rev Lett
UR - http://dx.doi.org/10.1103/PhysRevLett.134.071401
UR - https://www.ncbi.nlm.nih.gov/pubmed/40053989
VL - 134
ER -