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Title: Cosmology with the Laser Interferometer Space Antenna

Journal Article · · Living Rev.Rel.
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  1. APC, Paris
  2. Portsmouth U., ICG
  3. Queen Mary, U. of London (main)
  4. Lusofona U.
  5. Padua U.; INFN, Padua; Padua Observ.
  6. Utrecht U.
  7. U. Texas, Austin (main)
  8. Ariel U. Ctr., Samaria; BCCP, Berkeley; UC, Berkeley
  9. IRFU, Saclay, DPP
  10. IKERBASQUE, Bilbao; Basque U., Bilbao
  11. Barcelona, IFAE
  12. ARTEMIS, Nice
  13. Madrid, Inst. Estructura Materia
  14. Dartmouth Coll.
  15. APC, Paris; Geneva U.; CERN
  16. IASF, Milan
  17. UC, Riverside
  18. MIT; MIT, MKI
  19. Brussels U.
  20. INFN, Ferrara
  21. Edinburgh U., Inst. Astron.
  22. Imperial Coll., London
  23. SISSA, Trieste; INFN, Trieste; IFPU, Trieste
  24. TRIUMF; Durham U., IPPP
  25. Geneva U.
  26. U. Helsinki (main)
  27. Pisa U.; INFN, Pisa
  28. Technion
  29. New South Wales U.; Groningen U.
  30. Minas Gerais U.
  31. Chicago U., EFI; Chicago U., KICP
  32. Portsmouth U., ICG; Madrid, IFT
  33. Valencia U., IFIC
  34. UC, San Diego
  35. Lisbon U., CAAUL
  36. Madrid, IFT; Paris U. VI, GRECO
  37. Madrid, IFT
  38. Nottingham U.
  39. Bangalore, Indian Inst. Sci.
  40. University Coll. London; King's Coll. London
  41. Madrid, IFT; DESY
  42. Louvain U., CP3
  43. Aristotle U., Thessaloniki
  44. DESY
  45. L2IT, Toulouse
  46. Warsaw U.
  47. Weizmann Inst.
  48. New South Wales U.
  49. Minnesota U.
  50. Groningen U.
  51. Perimeter Inst. Theor. Phys.; U. Amsterdam, GRAPPA; Amsterdam U.; Leiden U.
  52. Rome U.; INFN, Rome
  53. Stavanger U.
  54. Padua U.; INFN, Padua
  55. U. Aquila (main)
  56. Paris U. VI, GRECO
  57. LIGO Lab., Caltech; Caltech, Pasadena (main)
  58. Texas Tech.
  59. INFN, Florence; Florence U.
  60. APC, Paris; Ilia State U.
  61. Madrid, Polytechnic U.
  62. King's Coll. London
  63. Prague, Inst. Phys.
  64. Munich, Max Planck Inst.
  65. CERN
  66. U. Mainz, PRISMA; Mainz U., Inst. Phys.
  67. Kyiv Astron. Observ.; Kiev Observ.
  68. DESY; Hamburg U., Inst. Theor. Phys. II
  69. Massachusetts U., Amherst
  70. Porto U., Astron. Dept.; Porto U.
  71. Potsdam, Max Planck Inst.; Nijmegen U., IMAPP
  72. Swansea U.
  73. RWTH Aachen U.
  74. Prague, Inst. Phys.; Ben Gurion U. of Negev
  75. Naples U.
  76. IPhT, Saclay
  77. Skidmore Coll.
  78. Fermilab
  79. TRIUMF; Sussex U.
  80. Porto U.; Porto U., Astron. Dept.
  81. Juiz de Fora U.
  82. Lethbridge U.
  83. Turin Observ.; ITC-IRST, Trento
  84. Johns Hopkins U.
  85. Madrid U.; UCM, Somosaguas
  86. Granada U., Theor. Phys. Astrophys.
  87. Cornell U.
  88. Queen Mary, U. of London, Math. Sci.
  89. Lisbon U., CAAUL; Lisbon U.
  90. Kapteyn Astron. Inst., Groningen
  91. CERN; LPHE, Lausanne
  92. Auckland U.
  93. Marseille, CPPM
  94. Georgia Tech
  95. Los Alamos
  96. Canterbury U.
  97. Glasgow U.
  98. CERN; U. Mainz, PRISMA; Mainz U., Inst. Phys.
  99. Brown U.
  100. Ariel U. Ctr., Samaria
  101. Columbia U.; Columbia U., Astron. Astrophys.
  102. SYRTE, Paris
  103. Basque U., Bilbao
  104. Auckland U., Dept. Statistics
  105. Aristotle U., Thessaloniki; Tomsk Pedagogical Inst.
  106. Harvard U.; Harvard U. (main)
  107. BCCP, Berkeley; UC, Berkeley
  108. APC, Paris; IRFU, Saclay, DPP
  109. Leiden Observ.
  110. Birmingham U.
  111. York U., Canada
  112. Marseille, Lab. Astrophys.
  113. Milan Bicocca U.
  114. ICE, Bellaterra; CSIC, Catalunya; Barcelona, IEEC
  115. NCSU, Raleigh; Kuwait U.
  116. Hamilton Math. Inst., Dublin
  117. Tokyo U., IPMU
  118. Kyiv Astron. Observ.

The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational-wave observations extends well beyond these two objectives. This publication presents a summary of the state of the art in LISA cosmology, theory and methods, and identifies new opportunities to use gravitational-wave observations by LISA to probe the universe.

Research Organization:
APC, Paris; ARTEMIS, Nice; Amsterdam U.; Ariel U. Ctr., Samaria; Aristotle U., Thessaloniki; Auckland U.; Auckland U., Dept. Statistics; BCCP, Berkeley; Bangalore, Indian Inst. Sci.; Barcelona, IEEC; Barcelona, IFAE; Basque U., Bilbao; Ben Gurion U. of Negev; Birmingham U.; Brown U.; Brussels U.; CERN; CSIC, Catalunya; Caltech, Pasadena (main); Canterbury U.; Chicago U., EFI; Chicago U., KICP; Columbia U.; Columbia U., Astron. Astrophys.; Cornell U.; DESY; Dartmouth Coll.; Durham U., IPPP; Edinburgh U., Inst. Astron.; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Florence U.; Geneva U.; Georgia Tech; Glasgow U.; Granada U., Theor. Phys. Astrophys.; Groningen U.; Hamburg U., Inst. Theor. Phys. II; Hamilton Math. Inst., Dublin; Harvard U.; Harvard U. (main); IASF, Milan; ICE, Bellaterra; IFPU, Trieste; IKERBASQUE, Bilbao; INFN, Ferrara; INFN, Florence; INFN, Padua; INFN, Pisa; INFN, Rome; INFN, Trieste; IPhT, Saclay; IRFU, Saclay, DPP; ITC-IRST, Trento; Ilia State U.; Imperial Coll., London; Johns Hopkins U.; Juiz de Fora U.; Kapteyn Astron. Inst., Groningen; Kiev Observ.; King's Coll. London; Kuwait U.; Kyiv Astron. Observ.; L2IT, Toulouse; LIGO Lab., Caltech; LPHE, Lausanne; Leiden Observ.; Leiden U.; Lethbridge U.; Lisbon U.; Lisbon U., CAAUL; Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); Louvain U., CP3; Lusofona U.; MIT; MIT, MKI; Madrid U.; Madrid, IFT; Madrid, Inst. Estructura Materia; Madrid, Polytechnic U.; Mainz U., Inst. Phys.; Marseille, CPPM; Marseille, Lab. Astrophys.; Massachusetts U., Amherst; Milan Bicocca U.; Minas Gerais U.; Minnesota U.; Munich, Max Planck Inst.; NCSU, Raleigh; Naples U.; New South Wales U.; Nijmegen U., IMAPP; Nottingham U.; Padua Observ.; Padua U.; Paris U. VI, GRECO; Perimeter Inst. Theor. Phys.; Pisa U.; Porto U.; Porto U., Astron. Dept.; Portsmouth U., ICG; Potsdam, Max Planck Inst.; Prague, Inst. Phys.; Queen Mary, U. of London (main); Queen Mary, U. of London, Math. Sci.; RWTH Aachen U.; Rome U.; SISSA, Trieste; SYRTE, Paris; Skidmore Coll.; Stavanger U.; Sussex U.; Swansea U.; TRIUMF; Technion; Texas Tech.; Tokyo U., IPMU; Tomsk Pedagogical Inst.; Turin Observ.; U. Amsterdam, GRAPPA; U. Aquila (main); U. Helsinki (main); U. Mainz, PRISMA; U. Texas, Austin (main); UC, Berkeley; UC, Riverside; UC, San Diego; UCM, Somosaguas; University Coll. London; Utrecht U.; Valencia U., IFIC; Warsaw U.; Weizmann Inst.; York U., Canada
Sponsoring Organization:
US Department of Energy
Grant/Contract Number:
89243024CSC000002; AC02-07CH11359
OSTI ID:
1873706
Report Number(s):
FERMILAB-PUB-22-349-SCD; LISA CosWG-22-03; arXiv:2204.05434; oai:inspirehep.net:2066207
Journal Information:
Living Rev.Rel., Journal Name: Living Rev.Rel. Journal Issue: 1 Vol. 26
Country of Publication:
United States
Language:
English

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