Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μhz

M. Armano; H. Audley; J. Baird; P. Binetruy; M. Born; D. Bortoluzzi; E. Castelli; A. Cavalleri; A. Cesarini; A. M. Cruise; K. Danzmann; M. De Deus Silva; I. Diepholz; G. Dixon; R. Dolesi; L. Ferraioli; V. Ferroni; E. D. Fitzsimons; M. Freschi; L. Gesa; F. Gibert; D. Giardini; R. Giusteri; C. Grimani; J. Grzymisch; I. Harrison; G. Heinzel; M. Hewitson; D. Hollington; D. Hoyland; M. Hueller; H. Inchauspé; O. Jennrich; P. Jetzer; N. Karnesis; B. Kaune; N. Korsakova; C. J. Killow; J. A. Lobo; I. Lloro; L. Liu; J. P. López-Zaragoza; R. Maarschalkerweerd; D. Mance; N. Meshksar; V. Martín; L. Martin-Polo; J. Martino; F. Martin-Porqueras; I. Mateos; P. W. McNamara; J. Mendes; L. Mendes; M. Nofrarias; S. Paczkowski; M. Perreur-Lloyd; A. Petiteau; P. Pivato; E. Plagnol; J. Ramos-Castro; J. Reiche; D. I. Robertson; F. Rivas; G. Russano; J. Slutsky; C. F. Sopuerta; T. Sumner; D. Texier; J. I. Thorpe; D. Vetrugno; S. Vitale; G. Wanner; H. Ward; P. J. Wass; W. J. Weber; L. Wissel; A. Wittchen; P. Zweifel

doi:10.1103/PhysRevLett.120.061101

Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μhz

M. Armano, H. Audley, J. Baird, P. Binetruy, M. Born, D. Bortoluzzi, E. Castelli, A. Cavalleri, A. Cesarini, A. M. Cruise, K. Danzmann, M. De Deus Silva, I. Diepholz, G. Dixon, R. Dolesi, L. Ferraioli, V. Ferroni, E. D. Fitzsimons, M. Freschi, L. GesaF. Gibert, D. Giardini, R. Giusteri, C. Grimani, J. Grzymisch, I. Harrison, G. Heinzel, M. Hewitson, D. Hollington, D. Hoyland, M. Hueller, H. Inchauspé, O. Jennrich, P. Jetzer, N. Karnesis, B. Kaune, N. Korsakova, C. J. Killow, J. A. Lobo, I. Lloro, L. Liu, J. P. López-Zaragoza, R. Maarschalkerweerd, D. Mance, N. Meshksar, V. Martín, L. Martin-Polo, J. Martino, F. Martin-Porqueras, I. Mateos, P. W. McNamara, J. Mendes, L. Mendes, M. Nofrarias, S. Paczkowski, M. Perreur-Lloyd, A. Petiteau, P. Pivato, E. Plagnol, J. Ramos-Castro, J. Reiche, D. I. Robertson, F. Rivas, G. Russano, J. Slutsky, C. F. Sopuerta, T. Sumner, D. Texier, J. I. Thorpe, D. Vetrugno, S. Vitale, G. Wanner, H. Ward, P. J. Wass, W. J. Weber, L. Wissel, A. Wittchen, P. Zweifel

Research output: Contribution to journal › Article › Research › peer-review

103 Citations (Scopus)

Abstract

© 2018 authors. Published by the American Physical Society. In the months since the publication of the first results, the noise performance of LISA Pathfinder has improved because of reduced Brownian noise due to the continued decrease in pressure around the test masses, from a better correction of noninertial effects, and from a better calibration of the electrostatic force actuation. In addition, the availability of numerous long noise measurement runs, during which no perturbation is purposely applied to the test masses, has allowed the measurement of noise with good statistics down to 20 μHz. The Letter presents the measured differential acceleration noise figure, which is at (1.74±0.01) fm s-2/Hz above 2 mHz and (6±1)×10 fm s-2/Hz at 20 μHz, and discusses the physical sources for the measured noise. This performance provides an experimental benchmark demonstrating the ability to realize the low-frequency science potential of the LISA mission, recently selected by the European Space Agency.

Original language	English
Article number	061101
Journal	Physical Review Letters
Volume	120
Issue number	6
DOIs	https://doi.org/10.1103/PhysRevLett.120.061101
Publication status	Published - 5 Feb 2018

Access to Document

10.1103/PhysRevLett.120.061101

Fingerprint Dive into the research topics of 'Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μhz'. Together they form a unique fingerprint.

Cite this

Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., De Deus Silva, M., Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Freschi, M., ... Zweifel, P. (2018). Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μhz. Physical Review Letters, 120(6), [061101]. https://doi.org/10.1103/PhysRevLett.120.061101

Armano, M. ; Audley, H. ; Baird, J. ; Binetruy, P. ; Born, M. ; Bortoluzzi, D. ; Castelli, E. ; Cavalleri, A. ; Cesarini, A. ; Cruise, A. M. ; Danzmann, K. ; De Deus Silva, M. ; Diepholz, I. ; Dixon, G. ; Dolesi, R. ; Ferraioli, L. ; Ferroni, V. ; Fitzsimons, E. D. ; Freschi, M. ; Gesa, L. ; Gibert, F. ; Giardini, D. ; Giusteri, R. ; Grimani, C. ; Grzymisch, J. ; Harrison, I. ; Heinzel, G. ; Hewitson, M. ; Hollington, D. ; Hoyland, D. ; Hueller, M. ; Inchauspé, H. ; Jennrich, O. ; Jetzer, P. ; Karnesis, N. ; Kaune, B. ; Korsakova, N. ; Killow, C. J. ; Lobo, J. A. ; Lloro, I. ; Liu, L. ; López-Zaragoza, J. P. ; Maarschalkerweerd, R. ; Mance, D. ; Meshksar, N. ; Martín, V. ; Martin-Polo, L. ; Martino, J. ; Martin-Porqueras, F. ; Mateos, I. ; McNamara, P. W. ; Mendes, J. ; Mendes, L. ; Nofrarias, M. ; Paczkowski, S. ; Perreur-Lloyd, M. ; Petiteau, A. ; Pivato, P. ; Plagnol, E. ; Ramos-Castro, J. ; Reiche, J. ; Robertson, D. I. ; Rivas, F. ; Russano, G. ; Slutsky, J. ; Sopuerta, C. F. ; Sumner, T. ; Texier, D. ; Thorpe, J. I. ; Vetrugno, D. ; Vitale, S. ; Wanner, G. ; Ward, H. ; Wass, P. J. ; Weber, W. J. ; Wissel, L. ; Wittchen, A. ; Zweifel, P. / Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μhz. In: Physical Review Letters. 2018 ; Vol. 120, No. 6.

@article{27a7a862483944e38ba76e493b22e528,

title = "Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μhz",

abstract = "{\textcopyright} 2018 authors. Published by the American Physical Society. In the months since the publication of the first results, the noise performance of LISA Pathfinder has improved because of reduced Brownian noise due to the continued decrease in pressure around the test masses, from a better correction of noninertial effects, and from a better calibration of the electrostatic force actuation. In addition, the availability of numerous long noise measurement runs, during which no perturbation is purposely applied to the test masses, has allowed the measurement of noise with good statistics down to 20 μHz. The Letter presents the measured differential acceleration noise figure, which is at (1.74±0.01) fm s-2/Hz above 2 mHz and (6±1)×10 fm s-2/Hz at 20 μHz, and discusses the physical sources for the measured noise. This performance provides an experimental benchmark demonstrating the ability to realize the low-frequency science potential of the LISA mission, recently selected by the European Space Agency.",

author = "M. Armano and H. Audley and J. Baird and P. Binetruy and M. Born and D. Bortoluzzi and E. Castelli and A. Cavalleri and A. Cesarini and Cruise, {A. M.} and K. Danzmann and {De Deus Silva}, M. and I. Diepholz and G. Dixon and R. Dolesi and L. Ferraioli and V. Ferroni and Fitzsimons, {E. D.} and M. Freschi and L. Gesa and F. Gibert and D. Giardini and R. Giusteri and C. Grimani and J. Grzymisch and I. Harrison and G. Heinzel and M. Hewitson and D. Hollington and D. Hoyland and M. Hueller and H. Inchausp{\'e} and O. Jennrich and P. Jetzer and N. Karnesis and B. Kaune and N. Korsakova and Killow, {C. J.} and Lobo, {J. A.} and I. Lloro and L. Liu and L{\'o}pez-Zaragoza, {J. P.} and R. Maarschalkerweerd and D. Mance and N. Meshksar and V. Mart{\'i}n and L. Martin-Polo and J. Martino and F. Martin-Porqueras and I. Mateos and McNamara, {P. W.} and J. Mendes and L. Mendes and M. Nofrarias and S. Paczkowski and M. Perreur-Lloyd and A. Petiteau and P. Pivato and E. Plagnol and J. Ramos-Castro and J. Reiche and Robertson, {D. I.} and F. Rivas and G. Russano and J. Slutsky and Sopuerta, {C. F.} and T. Sumner and D. Texier and Thorpe, {J. I.} and D. Vetrugno and S. Vitale and G. Wanner and H. Ward and Wass, {P. J.} and Weber, {W. J.} and L. Wissel and A. Wittchen and P. Zweifel",

year = "2018",

month = feb,

day = "5",

doi = "10.1103/PhysRevLett.120.061101",

language = "English",

volume = "120",

number = "6",

}

Armano, M, Audley, H, Baird, J, Binetruy, P, Born, M, Bortoluzzi, D, Castelli, E, Cavalleri, A, Cesarini, A, Cruise, AM, Danzmann, K, De Deus Silva, M, Diepholz, I, Dixon, G, Dolesi, R, Ferraioli, L, Ferroni, V, Fitzsimons, ED, Freschi, M, Gesa, L, Gibert, F, Giardini, D, Giusteri, R, Grimani, C, Grzymisch, J, Harrison, I, Heinzel, G, Hewitson, M, Hollington, D, Hoyland, D, Hueller, M, Inchauspé, H, Jennrich, O, Jetzer, P, Karnesis, N, Kaune, B, Korsakova, N, Killow, CJ, Lobo, JA, Lloro, I, Liu, L, López-Zaragoza, JP, Maarschalkerweerd, R, Mance, D, Meshksar, N, Martín, V, Martin-Polo, L, Martino, J, Martin-Porqueras, F, Mateos, I, McNamara, PW, Mendes, J, Mendes, L, Nofrarias, M, Paczkowski, S, Perreur-Lloyd, M, Petiteau, A, Pivato, P, Plagnol, E, Ramos-Castro, J, Reiche, J, Robertson, DI, Rivas, F, Russano, G, Slutsky, J, Sopuerta, CF, Sumner, T, Texier, D, Thorpe, JI, Vetrugno, D, Vitale, S, Wanner, G, Ward, H, Wass, PJ, Weber, WJ, Wissel, L, Wittchen, A & Zweifel, P 2018, 'Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μhz', Physical Review Letters, vol. 120, no. 6, 061101. https://doi.org/10.1103/PhysRevLett.120.061101

Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μhz. / Armano, M.; Audley, H.; Baird, J.; Binetruy, P.; Born, M.; Bortoluzzi, D.; Castelli, E.; Cavalleri, A.; Cesarini, A.; Cruise, A. M.; Danzmann, K.; De Deus Silva, M.; Diepholz, I.; Dixon, G.; Dolesi, R.; Ferraioli, L.; Ferroni, V.; Fitzsimons, E. D.; Freschi, M.; Gesa, L.; Gibert, F.; Giardini, D.; Giusteri, R.; Grimani, C.; Grzymisch, J.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hoyland, D.; Hueller, M.; Inchauspé, H.; Jennrich, O.; Jetzer, P.; Karnesis, N.; Kaune, B.; Korsakova, N.; Killow, C. J.; Lobo, J. A.; Lloro, I.; Liu, L.; López-Zaragoza, J. P.; Maarschalkerweerd, R.; Mance, D.; Meshksar, N.; Martín, V.; Martin-Polo, L.; Martino, J.; Martin-Porqueras, F.; Mateos, I.; McNamara, P. W.; Mendes, J.; Mendes, L.; Nofrarias, M.; Paczkowski, S.; Perreur-Lloyd, M.; Petiteau, A.; Pivato, P.; Plagnol, E.; Ramos-Castro, J.; Reiche, J.; Robertson, D. I.; Rivas, F.; Russano, G.; Slutsky, J.; Sopuerta, C. F.; Sumner, T.; Texier, D.; Thorpe, J. I.; Vetrugno, D.; Vitale, S.; Wanner, G.; Ward, H.; Wass, P. J.; Weber, W. J.; Wissel, L.; Wittchen, A.; Zweifel, P.

In: Physical Review Letters, Vol. 120, No. 6, 061101, 05.02.2018.

Research output: Contribution to journal › Article › Research › peer-review

TY - JOUR

T1 - Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μhz

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, A. M.

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, E. D.

AU - Freschi, M.

AU - Gesa, L.

AU - Gibert, F.

AU - Giardini, D.

AU - Giusteri, R.

AU - Grimani, C.

AU - Grzymisch, J.

AU - Harrison, I.

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, C. J.

AU - Lobo, J. A.

AU - Lloro, I.

AU - Liu, L.

AU - López-Zaragoza, J. P.

AU - Maarschalkerweerd, R.

AU - Mance, D.

AU - Meshksar, N.

AU - Martín, V.

AU - Martin-Polo, L.

AU - Martino, J.

AU - Martin-Porqueras, F.

AU - Mateos, I.

AU - McNamara, P. W.

AU - Mendes, J.

AU - Mendes, L.

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 - Robertson, D. I.

AU - Rivas, F.

AU - Russano, G.

AU - Slutsky, J.

AU - Sopuerta, C. F.

AU - Sumner, T.

AU - Texier, D.

AU - Thorpe, J. I.

AU - Vetrugno, D.

AU - Vitale, S.

AU - Wanner, G.

AU - Ward, H.

AU - Wass, P. J.

AU - Weber, W. J.

AU - Wissel, L.

AU - Wittchen, A.

AU - Zweifel, P.

PY - 2018/2/5

Y1 - 2018/2/5

N2 - © 2018 authors. Published by the American Physical Society. In the months since the publication of the first results, the noise performance of LISA Pathfinder has improved because of reduced Brownian noise due to the continued decrease in pressure around the test masses, from a better correction of noninertial effects, and from a better calibration of the electrostatic force actuation. In addition, the availability of numerous long noise measurement runs, during which no perturbation is purposely applied to the test masses, has allowed the measurement of noise with good statistics down to 20 μHz. The Letter presents the measured differential acceleration noise figure, which is at (1.74±0.01) fm s-2/Hz above 2 mHz and (6±1)×10 fm s-2/Hz at 20 μHz, and discusses the physical sources for the measured noise. This performance provides an experimental benchmark demonstrating the ability to realize the low-frequency science potential of the LISA mission, recently selected by the European Space Agency.

AB - © 2018 authors. Published by the American Physical Society. In the months since the publication of the first results, the noise performance of LISA Pathfinder has improved because of reduced Brownian noise due to the continued decrease in pressure around the test masses, from a better correction of noninertial effects, and from a better calibration of the electrostatic force actuation. In addition, the availability of numerous long noise measurement runs, during which no perturbation is purposely applied to the test masses, has allowed the measurement of noise with good statistics down to 20 μHz. The Letter presents the measured differential acceleration noise figure, which is at (1.74±0.01) fm s-2/Hz above 2 mHz and (6±1)×10 fm s-2/Hz at 20 μHz, and discusses the physical sources for the measured noise. This performance provides an experimental benchmark demonstrating the ability to realize the low-frequency science potential of the LISA mission, recently selected by the European Space Agency.

U2 - 10.1103/PhysRevLett.120.061101

DO - 10.1103/PhysRevLett.120.061101

M3 - Article

VL - 120

IS - 6

M1 - 061101

ER -