Exploring dark forces with multimessenger studies of extreme mass ratio inspirals
The exploration of dark sector interactions via gravitational waves (GWs) from binary inspirals has been a subject of recent interest. We study dark forces using extreme mass ratio inspirals (EMRIs), pointing out two issues of interest. Firstly, the innermost stable circular orbit (ISCO) of the EMRI...
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| Published in | Journal of cosmology and astroparticle physics Vol. 2024; no. 9; pp. 23 - 48 |
|---|---|
| Main Authors | , , |
| Format | Journal Article |
| Language | English |
| Published |
Bristol
IOP Publishing
01.09.2024
Institute of Physics (IOP) |
| Subjects | |
| Online Access | Get full text |
| ISSN | 1475-7516 1475-7516 |
| DOI | 10.1088/1475-7516/2024/09/023 |
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| Abstract | The exploration of dark sector interactions via gravitational waves (GWs) from binary inspirals has been a subject of recent interest. We study dark forces using extreme mass ratio inspirals (EMRIs), pointing out two issues of interest. Firstly, the innermost stable circular orbit (ISCO) of the EMRI, which sets the characteristic length scale of the system and hence the dark force range to which it exhibits enhanced sensitivity, probes force mediator masses that complement those studied with supermassive black hole (SMBH) or neutron star binaries. The LISA mission (the proposed
μ
Ares detector) will probe mediators with masses
m
V
∼ 10
-16
eV (
m
V
∼ 10
-18
eV), corresponding to ISCOs of 10
6
M
⊙
(10
8
M
⊙
) central SMBHs. Secondly, while the sensitivity to dark couplings is typically limited by the uncertainty in the binary component masses, independent mass measurements of the central SMBH through reverberation mapping campaigns or the motion of dynamical tracers enable one to break this degeneracy. Our results therefore highlight the necessity for coordinated studies, loosely referred to as “multimessenger”, between future
μ
Hz- mHz GW observatories and ongoing and forthcoming SMBH mass measurement campaigns, including OzDES-RM, SDSS-RM, and SDSS-V Black Hole Mapper. |
|---|---|
| AbstractList | The exploration of dark sector interactions via gravitational waves (GWs) from binary inspirals has been a subject of recent interest. We study dark forces using extreme mass ratio inspirals (EMRIs), pointing out two issues of interest. Firstly, the innermost stable circular orbit (ISCO) of the EMRI, which sets the characteristic length scale of the system and hence the dark force range to which it exhibits enhanced sensitivity, probes force mediator masses that complement those studied with supermassive black hole (SMBH) or neutron star binaries. The LISA mission (the proposed μAres detector) will probe mediators with masses mV ∼ 10-16 eV (mV ∼ 10-18 eV), corresponding to ISCOs of 106M⊙ (108M⊙) central SMBHs. Secondly, while the sensitivity to dark couplings is typically limited by the uncertainty in the binary component masses, independent mass measurements of the central SMBH through reverberation mapping campaigns or the motion of dynamical tracers enable one to break this degeneracy. Our results therefore highlight the necessity for coordinated studies, loosely referred to as “multimessenger”, between future μHz- mHz GW observatories and ongoing and forthcoming SMBH mass measurement campaigns, including OzDES-RM, SDSS-RM, and SDSS-V Black Hole Mapper. Abstract The exploration of dark sector interactions via gravitational waves (GWs) from binary inspirals has been a subject of recent interest. We study dark forces using extreme mass ratio inspirals (EMRIs), pointing out two issues of interest. Firstly, the innermost stable circular orbit (ISCO) of the EMRI, which sets the characteristic length scale of the system and hence the dark force range to which it exhibits enhanced sensitivity, probes force mediator masses that complement those studied with supermassive black hole (SMBH) or neutron star binaries. The LISA mission (the proposedμAres detector) will probe mediators with massesmV∼ 10-16 eV (mV∼ 10-18 eV), corresponding to ISCOs of 106M⊙(108M⊙) central SMBHs. Secondly, while the sensitivity to dark couplings is typically limited by the uncertainty in the binary component masses, independent mass measurements of the central SMBH through reverberation mapping campaigns or the motion of dynamical tracers enable one to break this degeneracy. Our results therefore highlight the necessity for coordinated studies, loosely referred to as “multimessenger”, between futureμHz- mHz GW observatories and ongoing and forthcoming SMBH mass measurement campaigns, including OzDES-RM, SDSS-RM, and SDSS-V Black Hole Mapper. The exploration of dark sector interactions via gravitational waves (GWs) from binary inspirals has been a subject of recent interest. We study dark forces using extreme mass ratio inspirals (EMRIs), pointing out two issues of interest. Firstly, the innermost stable circular orbit (ISCO) of the EMRI, which sets the characteristic length scale of the system and hence the dark force range to which it exhibits enhanced sensitivity, probes force mediator masses that complement those studied with supermassive black hole (SMBH) or neutron star binaries. The LISA mission (the proposed μ Ares detector) will probe mediators with masses m V ∼ 10 -16 eV ( m V ∼ 10 -18 eV), corresponding to ISCOs of 10 6 M ⊙ (10 8 M ⊙ ) central SMBHs. Secondly, while the sensitivity to dark couplings is typically limited by the uncertainty in the binary component masses, independent mass measurements of the central SMBH through reverberation mapping campaigns or the motion of dynamical tracers enable one to break this degeneracy. Our results therefore highlight the necessity for coordinated studies, loosely referred to as “multimessenger”, between future μ Hz- mHz GW observatories and ongoing and forthcoming SMBH mass measurement campaigns, including OzDES-RM, SDSS-RM, and SDSS-V Black Hole Mapper. |
| Author | Sinha, Kuver Bhalla, Badal Xu, Tao |
| Author_xml | – sequence: 1 givenname: Badal orcidid: 0000-0003-0488-6649 surname: Bhalla fullname: Bhalla, Badal organization: Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, U.S.A – sequence: 2 givenname: Kuver surname: Sinha fullname: Sinha, Kuver organization: Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, U.S.A – sequence: 3 givenname: Tao orcidid: 0000-0002-1193-8470 surname: Xu fullname: Xu, Tao organization: Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, U.S.A |
| BackLink | https://www.osti.gov/biblio/2578797$$D View this record in Osti.gov |
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| Snippet | The exploration of dark sector interactions via gravitational waves (GWs) from binary inspirals has been a subject of recent interest. We study dark forces... The exploration of dark sector interactions via gravitational waves (GWs) from binary inspirals has been a subject of recent interest. We study dark forces... Abstract The exploration of dark sector interactions via gravitational waves (GWs) from binary inspirals has been a subject of recent interest. We study dark... |
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| SubjectTerms | Astronomy & Astrophysics astrophysical black holes Binary stars Circular orbits Couplings Gravitational waves gravitational waves / sources massive black holes Neutron stars Observatories Orbital stability Physics Supermassive black holes |
| Title | Exploring dark forces with multimessenger studies of extreme mass ratio inspirals |
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