These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.


BIOMARKERS

Molecular Biopsy of Human Tumors

- a resource for Precision Medicine *

140 related articles for article (PubMed ID: 10011770)

  • 1. Gravitational angular fluctuations of the cosmic background radiation produced by cosmological linear perturbations.
    Tomita K
    Phys Rev D Part Fields; 1989 Dec; 40(12):3821-3827. PubMed ID: 10011770
    [No Abstract]   [Full Text] [Related]  

  • 2. Non-gaussianity versus nonlinearity of cosmological perturbations.
    Verde L
    Ann N Y Acad Sci; 2001 Jun; 927():54-69. PubMed ID: 11411156
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Detection of polarization in the cosmic microwave background using DASI. Degree Angular Scale Interferometer.
    Kovac JM; Leitch EM; Pryke C; Carlstrom JE; Halverson NW; Holzapfel WL
    Nature; 2002 Dec 19-26; 420(6917):772-87. PubMed ID: 12490941
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Primordial Anisotropies in the Gravitational Wave Background from Cosmological Phase Transitions.
    Geller M; Hook A; Sundrum R; Tsai Y
    Phys Rev Lett; 2018 Nov; 121(20):201303. PubMed ID: 30500214
    [TBL] [Abstract][Full Text] [Related]  

  • 5. First Predictions of the Angular Power Spectrum of the Astrophysical Gravitational Wave Background.
    Cusin G; Dvorkin I; Pitrou C; Uzan JP
    Phys Rev Lett; 2018 Jun; 120(23):231101. PubMed ID: 29932710
    [TBL] [Abstract][Full Text] [Related]  

  • 6. Cosmological constraints on cosmic-string gravitational radiation.
    Caldwell RR; Allen B
    Phys Rev D Part Fields; 1992 May; 45(10):3447-3468. PubMed ID: 10014241
    [No Abstract]   [Full Text] [Related]  

  • 7. Robust constraint on cosmic textures from the cosmic microwave background.
    Feeney SM; Johnson MC; Mortlock DJ; Peiris HV
    Phys Rev Lett; 2012 Jun; 108(24):241301. PubMed ID: 23004255
    [TBL] [Abstract][Full Text] [Related]  

  • 8. Constraints on cosmological parameters from the analysis of the cosmic lens all sky survey radio-selected gravitational lens statistics.
    Chae KH; Biggs AD; Blandford RD; Browne IW; De Bruyn AG; Fassnacht CD; Helbig P; Jackson NJ; King LJ; Koopmans LV; Mao S; Marlow DR; McKean JP; Myers ST; Norbury M; Pearson TJ; Phillips PM; Readhead AC; Rusin D; Sykes CM; Wilkinson PN; Xanthopoulos E; York T
    Phys Rev Lett; 2002 Oct; 89(15):151301. PubMed ID: 12365978
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Detection of weak gravitational lensing distortions of distant galaxies by cosmic dark matter at large scales.
    Wittman DM; Tyson JA; Kirkman D; Dell'Antonio I; Bernstein G
    Nature; 2000 May; 405(6783):143-8. PubMed ID: 10821262
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Tests for Gaussianity of the MAXIMA-1 cosmic microwave background map.
    Wu JH; Balbi A; Borrill J; Ferreira PG; Hanany S; Jaffe AH; Lee AT; Rabii B; Richards PL; Smoot GF; Stompor R; Winant CD
    Phys Rev Lett; 2001 Dec; 87(25):251303. PubMed ID: 11736557
    [TBL] [Abstract][Full Text] [Related]  

  • 11. Cosmology with cosmic shear observations: a review.
    Kilbinger M
    Rep Prog Phys; 2015 Jul; 78(8):086901. PubMed ID: 26181770
    [TBL] [Abstract][Full Text] [Related]  

  • 12. Rotation of the cosmic microwave background polarization from weak gravitational lensing.
    Dai L
    Phys Rev Lett; 2014 Jan; 112(4):041303. PubMed ID: 24580435
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Reconstructing the nature of the first cosmic sources from the anisotropic 21-cm signal.
    Fialkov A; Barkana R; Cohen A
    Phys Rev Lett; 2015 Mar; 114(10):101303. PubMed ID: 25815921
    [TBL] [Abstract][Full Text] [Related]  

  • 14. Cosmological perturbation theory in slow-roll spacetimes.
    Losic B; Unruh WG
    Phys Rev Lett; 2008 Sep; 101(11):111101. PubMed ID: 18851270
    [TBL] [Abstract][Full Text] [Related]  

  • 15. A correlation between the cosmic microwave background and large-scale structure in the Universe.
    Boughn S; Crittenden R
    Nature; 2004 Jan; 427(6969):45-7. PubMed ID: 14702078
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Constraining isocurvature perturbations with cosmic microwave background polarization.
    Bucher M; Moodley K; Turok N
    Phys Rev Lett; 2001 Nov; 87(19):191301. PubMed ID: 11690402
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Alignment of an interferometric gravitational wave detector.
    Fritschel P; Mavalvala N; Shoemaker D; Sigg D; Zucker M; González G
    Appl Opt; 1998 Oct; 37(28):6734-47. PubMed ID: 18301487
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Cosmological tests of general relativity with future tomographic surveys.
    Zhao GB; Pogosian L; Silvestri A; Zylberberg J
    Phys Rev Lett; 2009 Dec; 103(24):241301. PubMed ID: 20366194
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Gravitational wave bursts from cosmic strings.
    Damour T; Vilenkin A
    Phys Rev Lett; 2000 Oct; 85(18):3761-4. PubMed ID: 11041921
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Cosmic microwave background anisotropies with mixed isocurvature perturbations.
    Trotta R; Riazuelo A; Durrer R
    Phys Rev Lett; 2001 Dec; 87(23):231301. PubMed ID: 11736439
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 7.