-
1
-
-
0004210614
-
-
Addison-Wesley, Redwood City, CA
-
See, e.g., E. W. Kolb and M. S. Turner, The Early Universe (Addison-Wesley, Redwood City, CA, 1990), Chap. 8.
-
(1990)
The Early Universe
-
-
Kolb, E.W.1
Turner, M.S.2
-
4
-
-
24944489366
-
-
A. A. Starobinskii, 117B, 175 (1982);
-
(1982)
, vol.117B
, pp. 175
-
-
Starobinskii, A.A.1
-
13
-
-
3743118751
-
-
E. J. Copeland, E. W. Kolb, A. R. Liddle, and J. E. Lidsey, Phys. Rev. Lett.71, 219 (1993);
-
(1993)
Phys. Rev. Lett.
, vol.71
, pp. 219
-
-
Copeland, E.J.1
Kolb, E.W.2
Liddle, A.R.3
Lidsey, J.E.4
-
14
-
-
33748830721
-
-
Phys. Rev. D48, 2529 (1993);
-
(1993)
Phys. Rev. D
, vol.48
, pp. 2529
-
-
-
15
-
-
0000811930
-
-
M. S. Turner, 48, 3502 (1993);
-
(1993)
, vol.48
, pp. 3502
-
-
Turner, M.S.1
-
16
-
-
85038341049
-
-
48, 5539 (1993).
-
(1993)
, vol.48
, pp. 5539
-
-
-
17
-
-
85038302932
-
-
One opinion has it that inflation-produced gravity waves are undetectably small in any reasonable model of inflation [D. Lyth, Report No. hep-ph/9606387 (unpublished)]
-
One opinion has it that inflation-produced gravity waves are undetectably small in any reasonable model of inflation [D. Lyth, Report No. hep-ph/9606387 (unpublished)].
-
-
-
-
18
-
-
0000660728
-
-
All formulas are given to lowest order in the deviation from scale invariance and are strictly applicable to single-field models with smooth potentials; see A. R. Liddle and M. S. Turner, Phys. Rev. D50, 758 (1994).
-
(1994)
Phys. Rev. D
, vol.50
, pp. 758
-
-
Liddle, A.R.1
Turner, M.S.2
-
19
-
-
0000502742
-
-
In addition, they assume (Formula presented)=1; the formulas for (Formula presented)≠1 are given in M. S. Turner and M. White, Phys. Rev. D53, 6822 (1996).
-
(1996)
Phys. Rev. D
, vol.53
, pp. 6822
-
-
Turner, M.S.1
White, M.2
-
26
-
-
85038307316
-
-
Isotropy in the mean implies that (Formula presented); the Gaussian nature of the inflationary metric fluctuations implies that the multipole amplitudes have Gaussian distributions, fully specified by their predicted variances
-
Isotropy in the mean implies that (Formula presented); the Gaussian nature of the inflationary metric fluctuations implies that the multipole amplitudes have Gaussian distributions, fully specified by their predicted variances.
-
-
-
-
28
-
-
85038285470
-
-
U. Seljak, Report No. astro-ph/9608131 (unpublished);, M. Kamionkowski, A. Kosowsky, and A. Stebbins, Report No. astro-ph/9609132 (unpublished)
-
U. Seljak, Report No. astro-ph/9608131 (unpublished);M. Kamionkowski, A. Kosowsky, and A. Stebbins, Report No. astro-ph/9609132 (unpublished).
-
-
-
-
30
-
-
85038308484
-
-
The energy density in gravitational waves can be expressed in terms of a rms strain, (Formula presented): (Formula presented). Note, for fixed strain sensitivity, the energy-density sensitivity varies with the square of the frequency
-
The energy density in gravitational waves can be expressed in terms of a rms strain, (Formula presented): (Formula presented). Note, for fixed strain sensitivity, the energy-density sensitivity varies with the square of the frequency.
-
-
-
-
31
-
-
0001797535
-
-
K. Gorski et al., Astrophys. J.464, L11 (1996). The normalization depends upon both (Formula presented) and (Formula presented); for the accuracy needed here, this complication can be ignored.
-
(1996)
Astrophys. J.
, vol.464
-
-
Gorski, K.1
-
34
-
-
85038281664
-
-
This is simple to understand: the drop in energy density from the Hubble scale to the plateau is given by the redshift of matter—radiation equality, which is inversely proportional to the energy density in radiation
-
This is simple to understand: the drop in energy density from the Hubble scale to the plateau is given by the redshift of matter—radiation equality, which is inversely proportional to the energy density in radiation.
-
-
-
-
36
-
-
85038293208
-
-
Given the inflationary potential the gravity-wave spectrum can be computed without assuming a power law; we have done this for chaotic inflation models, (Formula presented), to judge the accuracy of our approximation. It is typically better than 33%. In addition, since there is no standard model of inflation, the use of (Formula presented) and (Formula presented) to extrapolate the gravity-wave spectrum from very large scales offers the advantage of generality
-
Given the inflationary potential the gravity-wave spectrum can be computed without assuming a power law; we have done this for chaotic inflation models, (Formula presented), to judge the accuracy of our approximation. It is typically better than 33%. In addition, since there is no standard model of inflation, the use of (Formula presented) and (Formula presented) to extrapolate the gravity-wave spectrum from very large scales offers the advantage of generality.
-
-
-
-
37
-
-
0011490655
-
-
Particle and Nuclear Astrophysics and Cosmology in the Next Millennium, edited by E. W. Kolb and R. D. Peccei (World Scientific, Singapore, 1995), p. 398
-
See e.g., A. Abramovici et al., Science256, 325 (1992), and in Particle and Nuclear Astrophysics and Cosmology in the Next Millennium, edited by E. W. Kolb and R. D. Peccei (World Scientific, Singapore, 1995), p. 398;
-
(1992)
Science
, vol.256
, pp. 325
-
-
Abramovici, A.1
-
39
-
-
0001047640
-
-
E. Flanagan, 48, 2389 (1993).
-
(1993)
, vol.48
, pp. 2389
-
-
Flanagan, E.1
-
40
-
-
85038303295
-
-
B. Allen, Report No. qr-gc/9604033 (unpublished)
-
B. Allen, Report No. qr-gc/9604033 (unpublished).
-
-
-
-
41
-
-
85038311478
-
-
Prephase A design study for LISA
-
Prephase A design study for LISA.
-
-
-
-
42
-
-
0003811646
-
-
edited by S. W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1987), p. 330
-
K. S. Thorne, in 300 Years of Gravitation, edited by S. W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1987), p. 330.
-
300 Years of Gravitation
-
-
Thorne, K.S.1
-
44
-
-
13844323292
-
-
B. Allen and R. Brustein, Report No. gr-qc/9609013 (unpublished)
-
R. Brustein, M. Gasperini, M. Giovannini, and G. Veneziano, Phys. Lett. B361, 45 (1995); B. Allen and R. Brustein, Report No. gr-qc/9609013 (unpublished).
-
(1995)
Phys. Lett. B
, vol.361
, pp. 45
-
-
Brustein, R.1
Gasperini, M.2
Giovannini, M.3
Veneziano, G.4
-
45
-
-
0001750184
-
-
S. P. Grishchuk, Zh. Éksp. Teor. Fiz. 67, 825 (1974) [Sov. Phys. JETP40, 409 (1975)].
-
(1975)
Sov. Phys. JETP
, vol.40
, pp. 409
-
-
Grishchuk, S.P.1
|