Generation of Gravitational Waves by a Standing Electromagnetic Wave

Morozov, A. N.; Пустовойт, В. И.; Фомин, И. В.

doi:10.1134/s020228932101014x

Cited by 12 publications

(6 citation statements)

References 29 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…laser-plasma interactions [1031] or optical media [1032]. Using linearised gravity (sufficient given the tiny signal sizes), one can straightforwardly calculate metric perturbations due to laser-accelerated relativistic ions [1033], standing waves of light [1034], or laser pulses themselves [1035]. The latter were found to give slightly better prospects for detection than waves generated by acceleration of matter through laser-driven ablation of foil targets [1036].…”

Section: Gravitational Wavesmentioning

confidence: 99%

Advances in QED with intense background fields

Fedotov¹,

Ilderton²,

Karbstein³

et al. 2022

Preprint

View full text Add to dashboard Cite

Upcoming and planned experiments combining increasingly intense lasers and energetic particle beams will access new regimes of nonlinear, relativistic, quantum effects. This improved experimental capability has driven substantial progress in QED in intense background fields. We review here the advances made during the last decade, with a focus on theory and phenomenology. As ever higher intensities are reached, it becomes necessary to consider processes at higher orders in both the number of scattered particles and the number of loops, and to account for non-perturbative physics (e.g. the Schwinger effect), with extreme intensities requiring resummation of the loop expansion. In addition to increased intensity, experiments will reach higher accuracy, and these improvements are being matched by developments in theory such as in approximation frameworks, the description of finite-size effects, and the range of physical phenomena analysed. Topics on which there has been substantial progress include: radiation reaction, spin and polarisation, nonlinear quantum vacuum effects and connections to other fields including physics beyond the Standard Model.

show abstract

Section: Gravitational Wavesmentioning

confidence: 99%

Advances in QED with intense background fields

Fedotov¹,

Ilderton²,

Karbstein³

et al. 2022

Preprint

View full text Add to dashboard Cite

show abstract

“…laser-plasma interactions [1050] or optical media [1051]. Using linearised gravity (sufficient given the tiny signal sizes), one can straightforwardly calculate metric perturbations due to laser-accelerated relativistic ions [1052], standing waves of light [1053], or laser pulses themselves [1054]. The latter were found to give slightly better prospects for detection than waves generated by acceleration of matter through laser-driven ablation of foil targets [1055].…”

Section: Gravitational Wavesmentioning

confidence: 99%

Advances in QED with intense background fields

et al. 2023

View full text Add to dashboard Cite

“…But LISA (Fig 21 ), can listen to distance sources like compact supermassive black holes in the galactic core, primordial black holes to low-frequency sensitive signals sources like a binary white dwarf merger, sources from the early universe (Moore et al, 2014) [48] . And also, other techniques used for detection of wave (Morozov et al, 2021; Mensky et al, 2009) [49,50] .…”

Section: Fig 21mentioning

confidence: 99%

Gravitational waves: A review on the future astronomy

Swain¹,

Panda²,

Lima³

et al. 2022

IJMRGE

View full text Add to dashboard Cite

Detection of Gravitational waves opened a new path for cosmological study in a new approach. From the detection of gravitational waves signal by advanced LIGO, its research climbed the peak. After the collaboration of LIGO and Virgo, several observations get collected from different sources of binary systems like black holes, binary neutron stars even both binary black hole and neutron star. The rigorous detection of gravitational signals may provide an additional thrust in the study of complex binary systems, dark matter, dark energy, Hubble constant, etc. In this review paper, we went through multiple research manuscripts to analyze gravitational wave signals. Here we have reviewed the history and current situation of gravitational waves detection, and we explained the concept and process of detection. Also, we go through different parts of a detector and their working. Then multiple gravitational wave signals are focused, originated from various sources and then found correlation between them. From this, the contribution of gravitational waves in different fields like complex binary systems (black holes, neutron stars), dark matter, dark energy and Hubble Constant have been discussed in this manuscript.

show abstract

Generation of Gravitational Waves by a Standing Electromagnetic Wave

Cited by 12 publications

References 29 publications

Advances in QED with intense background fields

Advances in QED with intense background fields

Advances in QED with intense background fields

Gravitational waves: A review on the future astronomy

Contact Info

Product

Resources

About