BIOMARKERS

Molecular Biopsy of Human Tumors

- a resource for Precision Medicine *

222 related articles for article (PubMed ID: 28784809)

  • 1. Stabilization of ammonia-rich hydrate inside icy planets.
    Naden Robinson V; Wang Y; Ma Y; Hermann A
    Proc Natl Acad Sci U S A; 2017 Aug; 114(34):9003-9008. PubMed ID: 28784809
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Novel phases in ammonia-water mixtures under pressure.
    Naden Robinson V; Marqués M; Wang Y; Ma Y; Hermann A
    J Chem Phys; 2018 Dec; 149(23):234501. PubMed ID: 30579307
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Ionic Phases of Ammonia-Rich Hydrate at High Densities.
    Xu W; Robinson VN; Zhang X; Zhang HC; Donnelly ME; Dalladay-Simpson P; Hermann A; Liu XD; Gregoryanz E
    Phys Rev Lett; 2021 Jan; 126(1):015702. PubMed ID: 33480773
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Plastic and superionic phases in ammonia-water mixtures at high pressures and temperatures.
    Naden Robinson V; Hermann A
    J Phys Condens Matter; 2020 May; 32(18):184004. PubMed ID: 31914434
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Diamond formation from methane hydrate under the internal conditions of giant icy planets.
    Kadobayashi H; Ohnishi S; Ohfuji H; Yamamoto Y; Muraoka M; Yoshida S; Hirao N; Kawaguchi-Imada S; Hirai H
    Sci Rep; 2021 Apr; 11(1):8165. PubMed ID: 33854182
    [TBL] [Abstract][Full Text] [Related]  

  • 6. Superionic and metallic states of water and ammonia at giant planet conditions.
    Cavazzoni C; Chiarotti GL; Scandolo S; Tosatti E; Bernasconi M; Parrinello M
    Science; 1999 Jan; 283(5398):44-6. PubMed ID: 9872734
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Topologically frustrated ionisation in a water-ammonia ice mixture.
    Liu C; Mafety A; Queyroux JA; Wilson CW; Zhang H; Béneut K; Le Marchand G; Baptiste B; Dumas P; Garbarino G; Finocchi F; Loveday JS; Pietrucci F; Saitta AM; Datchi F; Ninet S
    Nat Commun; 2017 Oct; 8(1):1065. PubMed ID: 29051485
    [TBL] [Abstract][Full Text] [Related]  

  • 8. Large H
    Nisr C; Chen H; Leinenweber K; Chizmeshya A; Prakapenka VB; Prescher C; Tkachev SN; Meng Y; Liu Z; Shim SH
    Proc Natl Acad Sci U S A; 2020 May; 117(18):9747-9754. PubMed ID: 32312811
    [TBL] [Abstract][Full Text] [Related]  

  • 9. External supply of oxygen to the atmospheres of the giant planets.
    Feuchtgruber H; Lellouch E; de Graauw T; Bézard B; Encrenaz T; Griffin M
    Nature; 1997 Sep; 389(6647):159-62. PubMed ID: 9296492
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Double superionicity in icy compounds at planetary interior conditions.
    de Villa K; González-Cataldo F; Militzer B
    Nat Commun; 2023 Nov; 14(1):7580. PubMed ID: 37990010
    [TBL] [Abstract][Full Text] [Related]  

  • 11. Superionic Phases of the 1:1 Water-Ammonia Mixture.
    Bethkenhagen M; Cebulla D; Redmer R; Hamel S
    J Phys Chem A; 2015 Oct; 119(42):10582-8. PubMed ID: 26390374
    [TBL] [Abstract][Full Text] [Related]  

  • 12. Mineralogy, Structure, and Habitability of Carbon-Enriched Rocky Exoplanets: A Laboratory Approach.
    Hakim K; Spaargaren R; Grewal DS; Rohrbach A; Berndt J; Dominik C; van Westrenen W
    Astrobiology; 2019 Jul; 19(7):867-884. PubMed ID: 30994366
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Complexities in the structural evolution with pressure of water-ammonia mixtures.
    Berni S; Scelta D; Fanetti S; Bini R
    J Chem Phys; 2023 May; 158(18):. PubMed ID: 37154278
    [TBL] [Abstract][Full Text] [Related]  

  • 14. Laser-driven shock compression of "synthetic planetary mixtures" of water, ethanol, and ammonia.
    Guarguaglini M; Hernandez JA; Okuchi T; Barroso P; Benuzzi-Mounaix A; Bethkenhagen M; Bolis R; Brambrink E; French M; Fujimoto Y; Kodama R; Koenig M; Lefevre F; Miyanishi K; Ozaki N; Redmer R; Sano T; Umeda Y; Vinci T; Ravasio A
    Sci Rep; 2019 Jul; 9(1):10155. PubMed ID: 31300690
    [TBL] [Abstract][Full Text] [Related]  

  • 15. In situ Raman and X-ray diffraction studies on the high pressure and temperature stability of methane hydrate up to 55 GPa.
    Kadobayashi H; Hirai H; Ohfuji H; Ohtake M; Yamamoto Y
    J Chem Phys; 2018 Apr; 148(16):164503. PubMed ID: 29716198
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Stability of high-temperature salty ice suggests electrolyte permeability in water-rich exoplanet icy mantles.
    Hernandez JA; Caracas R; Labrosse S
    Nat Commun; 2022 Jun; 13(1):3303. PubMed ID: 35729158
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Condensation of methane, ammonia, and water and the inhibition of convection in giant planets.
    Guillot T
    Science; 1995 Sep; 269(5231):1697-9. PubMed ID: 7569896
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Equation of state and phase diagram of ammonia at high pressures from ab initio simulations.
    Bethkenhagen M; French M; Redmer R
    J Chem Phys; 2013 Jun; 138(23):234504. PubMed ID: 23802968
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Superionic Silica-Water and Silica-Hydrogen Compounds in the Deep Interiors of Uranus and Neptune.
    Gao H; Liu C; Shi J; Pan S; Huang T; Lu X; Wang HT; Xing D; Sun J
    Phys Rev Lett; 2022 Jan; 128(3):035702. PubMed ID: 35119900
    [TBL] [Abstract][Full Text] [Related]  

  • 20. First principles study of dense and metallic nitric sulfur hydrides.
    Li X; Lowe A; Conway L; Miao M; Hermann A
    Commun Chem; 2021 Jun; 4(1):83. PubMed ID: 36697602
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 12.