FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2797030962> ?p ?o ?g. }

• W2797030962 abstract "Primordial magnetic fields (PMFs), being present before the epoch of cosmic recombination, induce small-scale baryonic density fluctuations. These inhomogeneities lead to an inhomogeneous recombination process that alters the peaks and heights of the large-scale anisotropies of the cosmic microwave backround (CMB) radiation. Utilizing numerical compressible MHD calculations and a Monte Carlo Markov chain analysis, which compares calculated CMB anisotropies with those observed by the textit{WMAP} and textit{Planck} satellites, we derive limits on the magnitude of putative PMFs. We find that the {it total} remaining present day field, integrated over all scales, cannot exceed 47 pG for scale-invariant PMFs and 8.9 pG for PMFs with a violet Batchelor spectrum at 95% confidence level. These limits are more than one order of magnitude more stringent than any prior stated limits on PMFs from the CMB which have not accounted for this effect." @default.
• W2797030962 created "2018-04-24" @default.
• W2797030962 creator A5025294763 @default.
• W2797030962 creator A5040427423 @default.
• W2797030962 date "2019-07-10" @default.
• W2797030962 modified "2023-10-05" @default.
• W2797030962 title "Stringent Limit on Primordial Magnetic Fields from the Cosmic Microwave Background Radiation" @default.
• W2797030962 cites W1572424586 @default.
• W2797030962 cites W1609489680 @default.
• W2797030962 cites W1820960327 @default.
• W2797030962 cites W1904282058 @default.
• W2797030962 cites W1912969557 @default.
• W2797030962 cites W1944901286 @default.
• W2797030962 cites W1963716574 @default.
• W2797030962 cites W1970279692 @default.
• W2797030962 cites W1971745428 @default.
• W2797030962 cites W1973605451 @default.
• W2797030962 cites W1975067476 @default.
• W2797030962 cites W1975486999 @default.
• W2797030962 cites W1975671825 @default.
• W2797030962 cites W1976761078 @default.
• W2797030962 cites W1976946921 @default.
• W2797030962 cites W1980202629 @default.
• W2797030962 cites W1983789674 @default.
• W2797030962 cites W1983922149 @default.
• W2797030962 cites W1988718382 @default.
• W2797030962 cites W1999970756 @default.
• W2797030962 cites W2000775663 @default.
• W2797030962 cites W2001392911 @default.
• W2797030962 cites W2002770518 @default.
• W2797030962 cites W2002906427 @default.
• W2797030962 cites W2005332353 @default.
• W2797030962 cites W2005783817 @default.
• W2797030962 cites W2007025791 @default.
• W2797030962 cites W2007414583 @default.
• W2797030962 cites W2010763777 @default.
• W2797030962 cites W2015849884 @default.
• W2797030962 cites W2018984913 @default.
• W2797030962 cites W2020266637 @default.
• W2797030962 cites W2021748604 @default.
• W2797030962 cites W2024428904 @default.
• W2797030962 cites W2026608779 @default.
• W2797030962 cites W2028122289 @default.
• W2797030962 cites W2029434930 @default.
• W2797030962 cites W2030729573 @default.
• W2797030962 cites W2031117379 @default.
• W2797030962 cites W2035266558 @default.
• W2797030962 cites W2037168510 @default.
• W2797030962 cites W2041495695 @default.
• W2797030962 cites W2051314207 @default.
• W2797030962 cites W2053836599 @default.
• W2797030962 cites W2055213474 @default.
• W2797030962 cites W2055307167 @default.
• W2797030962 cites W2056296716 @default.
• W2797030962 cites W2057539390 @default.
• W2797030962 cites W2059622391 @default.
• W2797030962 cites W2067371738 @default.
• W2797030962 cites W2067502964 @default.
• W2797030962 cites W2073033875 @default.
• W2797030962 cites W2074831346 @default.
• W2797030962 cites W2077446475 @default.
• W2797030962 cites W2077762303 @default.
• W2797030962 cites W2086679840 @default.
• W2797030962 cites W2090677236 @default.
• W2797030962 cites W2090689666 @default.
• W2797030962 cites W2098151228 @default.
• W2797030962 cites W2101627212 @default.
• W2797030962 cites W2114083185 @default.
• W2797030962 cites W2126495287 @default.
• W2797030962 cites W2129794644 @default.
• W2797030962 cites W2133881751 @default.
• W2797030962 cites W2135678769 @default.
• W2797030962 cites W2153208487 @default.
• W2797030962 cites W2170761360 @default.
• W2797030962 cites W2173705539 @default.
• W2797030962 cites W2176939917 @default.
• W2797030962 cites W2256734599 @default.
• W2797030962 cites W2548438114 @default.
• W2797030962 cites W2606225158 @default.
• W2797030962 cites W2606932361 @default.
• W2797030962 cites W2790038266 @default.
• W2797030962 cites W2890212253 @default.
• W2797030962 cites W2962698994 @default.
• W2797030962 cites W2963897882 @default.
• W2797030962 cites W3037953573 @default.
• W2797030962 cites W3099197664 @default.
• W2797030962 cites W3100124554 @default.
• W2797030962 cites W3100507939 @default.
• W2797030962 cites W3100537878 @default.
• W2797030962 cites W3100875857 @default.
• W2797030962 cites W3101371361 @default.
• W2797030962 cites W3102541750 @default.
• W2797030962 cites W3103007360 @default.
• W2797030962 cites W3103299465 @default.
• W2797030962 cites W3103827875 @default.
• W2797030962 cites W3104439784 @default.
• W2797030962 cites W3106391903 @default.
• W2797030962 cites W3124806881 @default.
• W2797030962 cites W4295021604 @default.
• W2797030962 doi "https://doi.org/10.1103/physrevlett.123.021301" @default.

• next