SCOPUS 정보 검색 플랫폼

Physical Review Letters

Volumn 75, Issue 11, 1995, Pages 2077-2080

Cosmology with ultralight pseudo nambu-goldstone bosons

(4) Frieman, Joshua A a,b Hill, Christopher T c Stebbins, Albert a Waga, Ioav a,d

a NASA FERMILAB ASTROPHYSICS CENTER (United States)

b UNIVERSITY OF CHICAGO (United States)

c FERMI NATIONAL ACCELERATOR LABORATORY (United States)

d FEDERAL UNIVERSITY OF RIO DE JANEIRO (Brazil)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0346555928 PISSN: 00319007 EISSN: None Source Type: Journal
DOI: 10.1103/PhysRevLett.75.2077 Document Type: Article

Times cited : (862)

References (35)

1
- 0001461203
- Dynamical mass estimates on large scales using peculiar velocities have so far been inconclusive, Ωm∼0.2–1.
- (1994) ARAA , vol.32 , pp. 371
- Dekel¹

2
- 0028134725
- (1994) Nature (London) , vol.371 , pp. 757
- Freedman, W.¹

3
- 0028059145
- (1994) Nature (London) , vol.371 , pp. 385
- Pierce, M.¹

4
- 84889886942
- (1992) Pub. Astron. Soc. Pacific , vol.104 , pp. 559
- Jacoby, G.¹

5
- 0002299284
- (1991) Astrophys. J. Lett. , vol.373 , pp. L1
- Tonry, J.¹

6
- 84927478956
- C. Akerlof, M. Srednicki, New York Academy of Sciences, New York
- (1992) Proceedings of the 16th Texas Symposium on Relativistic Astrophysics and 3rd Symposium on Particles, Strings, and Cosmology,
- Renzini, A.¹

7
- 84927491440
- Astrophys. J.
- Shi, X.¹

8
- 11944272679
- (1990) Nature (London) , vol.348 , pp. 705
- Efstathiou, G.¹ Maddox, S.² Sutherland, W.³

9
- 12044251577
- (1993) Astrophys. J. , vol.413 , pp. 1
- Kofman, L.¹ Gnedin, N.² Bahcall, N.³

10
- 85040222664
- Reconstructing the linear power spectrum of cosmological mass fluctuations
- (1994) Monthly Notices of the Royal Astronomical Society , vol.267 , pp. 1020
- Peacock, J.¹ Dodds, S.²

11
- 85029993635
- Gravitational lensing frequencies: galaxy cross-sections and selection effects
- (1991) Monthly Notices of the Royal Astronomical Society , vol.253 , pp. 99
- Fukugita, M.¹ Turner, E.L.²

12
- 12044249413
- (1993) Astrophys. J. , vol.419 , pp. 12
- Kochanek, C.¹

13
- 12044259423
- (1993) Astrophys. J. , vol.416 , pp. 425
- Maoz, D.¹ Rix, H.-W.²

14
- 9344251553
- (1977) Phys. Rev. Lett. , vol.38 , pp. 1440
- Peccei, R.¹ Quinn, H.²

15
- 4243883666
- (1978) Phys. Rev. Lett. , vol.40 , pp. 223
- Weinberg, S.¹

16
- 84927465946
- (1981) Phys. Rev. Lett. , vol.46 , pp. 279
- Wilczek, F.¹

17
- 0043091375
- (1982) Phys. Rev. Lett. , vol.49 , pp. 1549
- Wilczek, F.¹

18
- 0002195815
- (1983) Nucl. Phys. , vol.219 B , pp. 31
- Gelmini, G.¹ Nussinov, S.² Yanagida, T.³

19
- 84927476587
- (1990) Phys. Lett. B , vol.241 , pp. 96
- Chigashige, Y.¹ Mohopatra, R.² Peccei, R.³

20
- 0006200258
- (1988) Phys. Lett. B , vol.208 , pp. 146
- Vorobev, P.¹ Gitarts, Y.²

21
- 0011776755
- (1988) Phys. Rev. D , vol.37 , pp. 2001
- Anselm, A.¹

22
- 0006145619
- (1982) Phys. Lett. , vol.116 B , pp. 161
- Anselm, A.¹ Uraltsev, N.²

23
- 33750739978
- (1988) Nucl. Phys. , vol.311 B , pp. 253
- Hill, C.T.¹ Ross, G.G.²

24
- 33750490291
- (1988) Phys. Lett. B , vol.203 , pp. 125

25
- 0001467354
- Another possibility (discussed there) is an axion that couples to a (hidden) gauge group that becomes strong at the scale Λ∼10-3 eV.
- (1992) Phys. Rev. D , vol.46 , pp. 1226
- Frieman, J.¹ Hill, C.² Watkins, R.³

26
- 0002682851
- (1989) Comments Nucl. Part. Phys. , vol.19 , pp. 25
- Hill, C.T.¹ Schramm, D.N.² Fry, J.³

27
- 4243543380
- (1986) Phys. Rev. Lett. , vol.57 , pp. 2234
- Wasserman, I.¹

28
- 0001687799
- Dynamical evolution of domain walls in an expanding universe
- (1989) The Astrophysical Journal , vol.347 , pp. 590
- Press, W.H.¹ Ryden, B.² Spergel, D.³

29
- 0003567937
- G. 't Hooft, et al., Plenum Press, New York and London
- (1979) Recent Developments in Gauge Theories, , pp. 135
- Hooft¹

30
- 84927474456
- The isocurvature density fluctuation at Hubble-radius crossing is δρ/ρ∼Hi/φi∼Hi/f, where Hi is the Hubble parameter during inflation and φi∼f is the initial value of the field. Constraints from the microwave background anisotropy on the amplitude of adiabatic perturbations in inflation require Hi≲1013 GeV, so the isocurvature amplitude is acceptable if f≳1018 GeV.

31
- 0001067587
- Gravitational instability of scalar fields and formation of primordial black holes
- (1985) Monthly Notices of the Royal Astronomical Society , vol.215 , pp. 575
- Khlopov, M.¹ Malomed, B.² Zel'dovich, Y.³

32
- 84927494535
- By construction, this expression applies where F(k)≤1. If zx

33
- 17044413843
- considered the cosmological consequences of a rolling scalar field, but assumed scalar potentials (exponentials or negative power laws) with different consequences from the model here.
- (1988) Phys. Rev. D , vol.37 , pp. 3406
- Ratra, B.¹ Peebles, P.J.E.²

34
- 12044253808
- (1993) Astrophys. J. , vol.409 , pp. 28
- Maoz, D.¹

35
- 84927461020
- Report No. YITP/K-1098, 1995 (to be published).
- Fukugita, M.¹ Yanagida, T.²

* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.