We study the cross-correlation between the 21-cm and cosmic microwave background (CMB) B mode fluctuations which are induced by the cosmic birefringence when the nonconstant scalar field couples to the electromagnetic field strength. Such multiwavelength signals can potentially probe the reionization history of the Universe and also explore the nature of fundamental physics such as the parity violation and the scalar field dynamics in the early Universe. We illustrate the feasibility to detect such 21-cm-B mode cross-correlations through commonly discussed scalar field models, the quintessence-like scalar field which is responsible for the current dark energy and the axionlike scalar field which is responsible for the current dark matter de...
The measurement of the brightness temperature fluctuations of neutral hydrogen 21-cm lines from the ...
The measurement of the brightness temperature fluctuations of neutral hydrogen 21-cm lines from the ...
The measurement of the brightness temperature fluctuations of neutral hydrogen 21-cm lines from the ...
We study the cross-correlation between the 21-cm and cosmic microwave background (CMB) B mode fluc...
The cosmic microwave background (CMB) polarization and the 21-cm line fluctuations are powerful prob...
The cosmic microwave background (CMB) polarization and the 21-cm line fluctuations are powerful prob...
The cosmic microwave background (CMB) polarization and the 21-cm line fluctuations are powerful prob...
The 21-cm line fluctuations and the cosmic microwave background (CMB) are powerful probes of the epo...
The cosmic microwave background (CMB) polarization and the 21-cm line fluctuations are powerful prob...
The 21-cm line fluctuations and the cosmic microwave background (CMB) are powerful probes of the epo...
The 21-cm line fluctuations and the cosmic microwave background (CMB) are powerful probes of the epo...
Theories for new particle and early-Universe physics abound with pseudo-Nambu-Goldstone fields that ...
Theories for new particle and early-Universe physics abound with pseudo-Nambu-Goldstone fields that ...
The cosmic microwave background (CMB) polarization and the 21-cm line fluctuations are powerful prob...
We study the detectability of the cross-correlation between 21 cm emission from the intergalactic me...
The measurement of the brightness temperature fluctuations of neutral hydrogen 21-cm lines from the ...
The measurement of the brightness temperature fluctuations of neutral hydrogen 21-cm lines from the ...
The measurement of the brightness temperature fluctuations of neutral hydrogen 21-cm lines from the ...
We study the cross-correlation between the 21-cm and cosmic microwave background (CMB) B mode fluc...
The cosmic microwave background (CMB) polarization and the 21-cm line fluctuations are powerful prob...
The cosmic microwave background (CMB) polarization and the 21-cm line fluctuations are powerful prob...
The cosmic microwave background (CMB) polarization and the 21-cm line fluctuations are powerful prob...
The 21-cm line fluctuations and the cosmic microwave background (CMB) are powerful probes of the epo...
The cosmic microwave background (CMB) polarization and the 21-cm line fluctuations are powerful prob...
The 21-cm line fluctuations and the cosmic microwave background (CMB) are powerful probes of the epo...
The 21-cm line fluctuations and the cosmic microwave background (CMB) are powerful probes of the epo...
Theories for new particle and early-Universe physics abound with pseudo-Nambu-Goldstone fields that ...
Theories for new particle and early-Universe physics abound with pseudo-Nambu-Goldstone fields that ...
The cosmic microwave background (CMB) polarization and the 21-cm line fluctuations are powerful prob...
We study the detectability of the cross-correlation between 21 cm emission from the intergalactic me...
The measurement of the brightness temperature fluctuations of neutral hydrogen 21-cm lines from the ...
The measurement of the brightness temperature fluctuations of neutral hydrogen 21-cm lines from the ...
The measurement of the brightness temperature fluctuations of neutral hydrogen 21-cm lines from the ...