Euclid preparation - LIV.: sensitivity to neutrino parameters
Context. The Euclid mission of the European Space Agency will deliver weak gravitational lensing and galaxy clustering surveys that can be used to constrain the standard cosmological model and extensions thereof. Aims. We present forecasts from the combination of the Euclid photometric galaxy survey...
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
January 2025
|
| In: |
Astronomy and astrophysics
Year: 2025, Jahrgang: 693, Pages: 1-36 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/202450859 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: https://doi.org/10.1051/0004-6361/202450859 Verlag, kostenfrei, Volltext: https://www.aanda.org/articles/aa/abs/2025/01/aa50859-24/aa50859-24.html 
|
| Verfasserangaben: | Euclid Collaboration |
MARC
| LEADER | 00000naa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1936253151 | ||
| 003 | DE-627 | ||
| 005 | 20250919141939.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 250919s2025 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1051/0004-6361/202450859 |2 doi | |
| 035 | |a (DE-627)1936253151 | ||
| 035 | |a (DE-599)KXP1936253151 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Archidiacono, Maria |e VerfasserIn |0 (DE-588)1376931923 |0 (DE-627)1936253925 |4 aut | |
| 245 | 1 | 0 | |a Euclid preparation - LIV. |b sensitivity to neutrino parameters |c Euclid Collaboration |
| 264 | 1 | |c January 2025 | |
| 300 | |b Illustrationen | ||
| 300 | |a 36 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Online verfügbar: 03. Januar 2025 | ||
| 500 | |a Euclid Collaboration: M. Archidiacono, K. Jahnke, G. Seidel [und 245 weitere] | ||
| 500 | |a Gesehen am 19.09.2025 | ||
| 520 | |a Context. The Euclid mission of the European Space Agency will deliver weak gravitational lensing and galaxy clustering surveys that can be used to constrain the standard cosmological model and extensions thereof. Aims. We present forecasts from the combination of the Euclid photometric galaxy surveys (weak lensing, galaxy clustering, and their cross-correlations) and its spectroscopic redshift survey with respect to their sensitivity to cosmological parameters. We include the summed neutrino mass, ∑mν, and the effective number of relativistic species, Neff, in the standard ΛCDM scenario and in the dynamical dark energy (w0waCDM) scenario. Methods. We compared the accuracy of different algorithms predicting the non-linear matter power spectrum for such models. We then validated several pipelines for Fisher matrix and Markov chain Monte Carlo (MCMC) forecasts, using different theory codes, algorithms for numerical derivatives, and assumptions on the non-linear cut-off scale. Results. The Euclid primary probes alone will reach a sensitivity of σ(∑mν = 60 meV) = 56 meV in the ΛCDM+∑mν model, whereas the combination with cosmic microwave background (CMB) data from Planck is expected to achieve σ(∑mν) = 23 meV, offering evidence of a non-zero neutrino mass to at least the 2.6 σ level. This could be pushed to a 4 σ detection if future CMB data from LiteBIRD and CMB Stage-IV were included. In combination with Planck, Euclid will also deliver tight constraints on ΔNeff < 0.144 (95%CL) in the ΛCDM+∑mν+Neff model or even ΔNeff < 0.063 when future CMB data are included. When floating the dark energy parameters, we find that the sensitivity to Neff remains stable, but for ∑mν, it gets degraded by up to a factor of 2, at most. Conclusions. This work illustrates the complementarity among the Euclid spectroscopic and photometric surveys and among Euclid and CMB constraints. Euclid will offer great potential in measuring the neutrino mass and excluding well-motivated scenarios with additional relativistic particles. | ||
| 700 | 1 | |a Jahnke, Knud |e VerfasserIn |0 (DE-588)1200875141 |0 (DE-627)1683870255 |4 aut | |
| 700 | 1 | |a Seidel, Gregor |d 1977- |e VerfasserIn |0 (DE-588)139967559 |0 (DE-627)703521993 |0 (DE-576)314004769 |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Astronomy and astrophysics |d Les Ulis : EDP Sciences, 1969 |g 693(2025) vom: Jan., Artikel-ID A58, Seite 1-36 |h Online-Ressource |w (DE-627)253390222 |w (DE-600)1458466-9 |w (DE-576)072283351 |x 1432-0746 |7 nnas |a Euclid preparation - LIV. sensitivity to neutrino parameters |
| 773 | 1 | 8 | |g volume:693 |g year:2025 |g month:01 |g elocationid:A58 |g pages:1-36 |g extent:36 |a Euclid preparation - LIV. sensitivity to neutrino parameters |
| 856 | 4 | 0 | |u https://doi.org/10.1051/0004-6361/202450859 |x Verlag |x Resolving-System |z kostenfrei |3 Volltext |
| 856 | 4 | 0 | |u https://www.aanda.org/articles/aa/abs/2025/01/aa50859-24/aa50859-24.html |x Verlag |z kostenfrei |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20250919 | ||
| 993 | |a Article | ||
| 994 | |a 2025 | ||
| 998 | |g 139967559 |a Seidel, Gregor |m 139967559:Seidel, Gregor |d 130000 |e 130000PS139967559 |k 0/130000/ |p 127 | ||
| 998 | |g 1200875141 |a Jahnke, Knud |m 1200875141:Jahnke, Knud |d 130000 |e 130000PJ1200875141 |k 0/130000/ |p 66 | ||
| 999 | |a KXP-PPN1936253151 |e 4773717637 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"physDesc":[{"extent":"36 S.","noteIll":"Illustrationen"}],"origin":[{"dateIssuedDisp":"January 2025","dateIssuedKey":"2025"}],"recId":"1936253151","relHost":[{"pubHistory":["1.1969 -"],"type":{"bibl":"periodical","media":"Online-Ressource"},"language":["eng"],"title":[{"title_sort":"Astronomy and astrophysics","title":"Astronomy and astrophysics","subtitle":"an international weekly journal"}],"recId":"253390222","disp":"Euclid preparation - LIV. sensitivity to neutrino parametersAstronomy and astrophysics","origin":[{"dateIssuedDisp":"1969-","dateIssuedKey":"1969","publisher":"EDP Sciences ; Springer","publisherPlace":"Les Ulis ; Berlin ; Heidelberg"}],"physDesc":[{"extent":"Online-Ressource"}],"note":["Gesehen am 21.06.2024","Erscheint 36mal jährlich in 12 Bänden zu je 3 Ausgaben","Fortsetzung der Druck-Ausgabe"],"name":{"displayForm":["European Southern Observatory (ESO)"]},"titleAlt":[{"title":"Astronomy & astrophysics"},{"title":"a European journal"}],"part":{"extent":"36","volume":"693","year":"2025","pages":"1-36","text":"693(2025) vom: Jan., Artikel-ID A58, Seite 1-36"},"id":{"issn":["1432-0746"],"zdb":["1458466-9"],"eki":["253390222"]},"corporate":[{"display":"European Southern Observatory","roleDisplay":"Herausgebendes Organ","role":"isb"}]}],"title":[{"title":"Euclid preparation - LIV.","subtitle":"sensitivity to neutrino parameters","title_sort":"Euclid preparation - LIV."}],"type":{"media":"Online-Ressource","bibl":"article-journal"},"language":["eng"],"id":{"doi":["10.1051/0004-6361/202450859"],"eki":["1936253151"]},"person":[{"family":"Archidiacono","given":"Maria","display":"Archidiacono, Maria","roleDisplay":"VerfasserIn","role":"aut"},{"family":"Jahnke","display":"Jahnke, Knud","role":"aut","roleDisplay":"VerfasserIn","given":"Knud"},{"display":"Seidel, Gregor","role":"aut","roleDisplay":"VerfasserIn","given":"Gregor","family":"Seidel"}],"name":{"displayForm":["Euclid Collaboration"]},"note":["Online verfügbar: 03. Januar 2025","Euclid Collaboration: M. Archidiacono, K. Jahnke, G. Seidel [und 245 weitere]","Gesehen am 19.09.2025"]} | ||
| SRT | |a ARCHIDIACOEUCLIDPREP2025 | ||