General references
193
3. Show that a neutralino with mass m}( ...., 100 GeV scattering from a xenon
nucleus with mXe ...., 130 GeV, with a typical WIMP speed v , . . , . 270 km s-I,
produces a nuclear recoil energy which is below 100 ke V.
6.8 General references
We have found the following article particularly useful in preparing this chapter.
• Jungman G, Kamionkowski M and Griest K 1996 Phys. Rep. 267 195
Bibliography
[I] Weinheimer C 2002 Proc of CUI, Course of Int. School of Physics 'Enrico Fermi'
Varenna, Italy 2002, arXiv:hep-exl0210050
[2] Eguchi K et a/2003 Phys. Rev. Letl. 90 021802, arXiv:hep-exl0212021
[3] Ahmed Q R et al2002 Phys. Rev. Letl. 89011301 arXiv:hep-exl0204008
[4] Spergel D N et al2003 Astrophys. J. Suppl. 148 175, arXiv:astro-phl0302209
[5] Trimble V 1987 Ann. Rev. Astron. Astrophys. 25425
Sadoulet B 1999 Rev. Mod. Phys. 71 S 197
Turner M S and Tyson J a 1999 Rev. Mod. Phys. 71 S 145
[6] Kapteyn J C 1922 Astrophys. J. 55302
[7] Bahcal1 J N et al 2999 Science 284 1481
[8] ZwickY F 1933 Helv. Phys. Acta 6 110
[9] Silk J 2003 Talk given at PASCOS'03. Mumbai. India
[10] Smith P F and Bennen J R J 1979 Nucl. Phys. B 179525
Smith P F et al 1982 Nucl. Phys. B 206 33
Verkerk P et al 1992 Phys. Rev. Letl. 68 1116
[11] Bailin D and Love A 1994 Supersymmetric Field Theory and String Theory (Bristol:
lOP)
[12] Pagels H and Primack J 1982 Phys. Rev. Letl. 48 223
[13] Weinberg S 1982 Phys. Rev. Lett. 481303
[14] Dimopoulos S and Sutter D 1995 Nucl. Phys. B 452 496, arXiv:hep-ph/95044 1 5
Suner D 1997 Stanford PhD Thesis arXiv:hep-ph/970439O
[15] Haber H E 1998 Nud. Phys. B Proc. Suppl. A-C 62 469
[ 16] Particle Data Group 2002 Phys. Rev. D 66 0 I 000 1
[17] Ellis J R, Falk T. Olive K A and Schmin M 1996 Phys. Letl. B 388 97, arXiv:hepph/9607292
[18] Ahlen S etal1987 Phys. Letl. B 195603
Calwel1 D D et al 1988 Phys. Rev. Lett. B 61 510
Beck M et a/l994 Phys. Letl. B 336 141
[19] Ellis J et al 1984 Nucl. Phys. B 238 453
[20] Bernstein J, Brown L and Feinberg G 1985 Phys. Rev. D 323261
Scherrer R and Turner M S 1986 Phys. Rev. D 33 1585
Scherrer R and Turner M S 1986 Phys. Rev. D 34 3263(E)
[21] Griest K and Kamionkowski M 1990 Phys. Rev. Lett. 64 615
[22] See Jungman et al op. cit. section 6
193
3. Show that a neutralino with mass m}( ...., 100 GeV scattering from a xenon
nucleus with mXe ...., 130 GeV, with a typical WIMP speed v , . . , . 270 km s-I,
produces a nuclear recoil energy which is below 100 ke V.
6.8 General references
We have found the following article particularly useful in preparing this chapter.
• Jungman G, Kamionkowski M and Griest K 1996 Phys. Rep. 267 195
Bibliography
[I] Weinheimer C 2002 Proc of CUI, Course of Int. School of Physics 'Enrico Fermi'
Varenna, Italy 2002, arXiv:hep-exl0210050
[2] Eguchi K et a/2003 Phys. Rev. Letl. 90 021802, arXiv:hep-exl0212021
[3] Ahmed Q R et al2002 Phys. Rev. Letl. 89011301 arXiv:hep-exl0204008
[4] Spergel D N et al2003 Astrophys. J. Suppl. 148 175, arXiv:astro-phl0302209
[5] Trimble V 1987 Ann. Rev. Astron. Astrophys. 25425
Sadoulet B 1999 Rev. Mod. Phys. 71 S 197
Turner M S and Tyson J a 1999 Rev. Mod. Phys. 71 S 145
[6] Kapteyn J C 1922 Astrophys. J. 55302
[7] Bahcal1 J N et al 2999 Science 284 1481
[8] ZwickY F 1933 Helv. Phys. Acta 6 110
[9] Silk J 2003 Talk given at PASCOS'03. Mumbai. India
[10] Smith P F and Bennen J R J 1979 Nucl. Phys. B 179525
Smith P F et al 1982 Nucl. Phys. B 206 33
Verkerk P et al 1992 Phys. Rev. Letl. 68 1116
[11] Bailin D and Love A 1994 Supersymmetric Field Theory and String Theory (Bristol:
lOP)
[12] Pagels H and Primack J 1982 Phys. Rev. Letl. 48 223
[13] Weinberg S 1982 Phys. Rev. Lett. 481303
[14] Dimopoulos S and Sutter D 1995 Nucl. Phys. B 452 496, arXiv:hep-ph/95044 1 5
Suner D 1997 Stanford PhD Thesis arXiv:hep-ph/970439O
[15] Haber H E 1998 Nud. Phys. B Proc. Suppl. A-C 62 469
[ 16] Particle Data Group 2002 Phys. Rev. D 66 0 I 000 1
[17] Ellis J R, Falk T. Olive K A and Schmin M 1996 Phys. Letl. B 388 97, arXiv:hepph/9607292
[18] Ahlen S etal1987 Phys. Letl. B 195603
Calwel1 D D et al 1988 Phys. Rev. Lett. B 61 510
Beck M et a/l994 Phys. Letl. B 336 141
[19] Ellis J et al 1984 Nucl. Phys. B 238 453
[20] Bernstein J, Brown L and Feinberg G 1985 Phys. Rev. D 323261
Scherrer R and Turner M S 1986 Phys. Rev. D 33 1585
Scherrer R and Turner M S 1986 Phys. Rev. D 34 3263(E)
[21] Griest K and Kamionkowski M 1990 Phys. Rev. Lett. 64 615
[22] See Jungman et al op. cit. section 6