Quick search Find article
Quick search
Find article

Ground-based interferometric gravitational-wave detectors in the LISA epoch

David Shoemaker

Show affiliations


Ground-based interferometry for gravitational-wave detection is in a state of rapid evolution. First-generation systems (LIGO, GEO, TAMA, VIRGO) are now (summer 2002) starting or will soon start observations, and second-generation instruments are well into the planning phases. By the time LISA joins the network of gravitational-wave detectors, we will have a mixture of second- and third-generation ground-based instruments observing. We give a description of some probable configurations for the ground-based instruments in that epoch.


PACS

95.55.Ym Gravitational radiation detectors; mass spectrometers; and other instrumentation and techniques

95.55.Br Astrometric and interferometric instruments

04.80.Nn Gravitational wave detectors and experiments

95.30.Sf Relativity and gravitation

MSC

85A99 Miscellaneous topics

83C35 Gravitational waves

Subjects

Instrumentation and measurement

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 10 (21 May 2003)

Received 13 December 2002

Published 25 April 2003



  1. Ground-based interferometric gravitational-wave detectors in the LISA epoch

    David Shoemaker 2003 Class. Quantum Grav. 20 S11

  2. Ageing properties of critical systems

    Pasquale Calabrese and Andrea Gambassi 2005 J. Phys. A: Math. Gen. 38 R133

  3. Scattering properties of ferroelectric domain walls

    D A Bruce 1981 J. Phys. C: Solid State Phys. 14 5195

  4. Quantum graphs: II. Some spectral properties of quantum and combinatorial graphs

    Peter Kuchment 2005 J. Phys. A: Math. Gen. 38 4887

  5. The Environmental Dependence of the Fraction of ''Unconventional'' Galaxies: Red Late Types and Blue Early Types

    Xin-Fa Deng et al. 2009 ApJ 699 948

  6. The early days of the journal

    J E Burns 2006 Phys. Med. Biol. 51 R1

  7. Status of the joint LIGO–TAMA300 inspiral analysis

    Stephen Fairhurst et al 2005 Class. Quantum Grav. 22 S1109

  8. Accretion of Dust Grains as a Possible Origin of Metal-poor Stars with Low α/Fe Ratios

    Toshikazu Shigeyama and Takuji Tsujimoto 2003 ApJ 598 L47

  9. Random replicators with asymmetric couplings

    Tobias Galla 2006 J. Phys. A: Math. Gen. 39 3853

  10. Detection of Lead in the Carbon-rich, Very Metal-poor Star LP 625-44: A Strong Constraint on s-Process Nucleosynthesis at Low Metallicity

    Wako Aoki et al 2000 ApJ 536 L97

View by subject




Export








Please login to access our web services, or create an account if you don't yet have one.

You must have cookies enabled in your web browser to be able to login.

Username
Password

Forgotten your password? Get a new one here.