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CERN Document Server 19 record trovati  1 - 10successivo  salta al record: La ricerca ha impiegato 0.71 secondi. 
1.
Assessing the Impact of Unequal Noises and Foreground Modeling on SGWB Reconstruction with LISA / Kume, Jun'ya (U. Padua, Dept. Phys. Astron. ; INFN, Padua ; U. Tokyo (main)) ; Peloso, Marco (Padua U. ; INFN, Padua) ; Pieroni, Mauro (CERN) ; Ricciardone, Angelo (Pisa U. ; INFN, Pisa)
In the search for stochastic gravitational wave backgrounds (SGWB) of cosmological origin with LISA, it is crucial to account for realistic complications in the noise and astrophysical foreground modeling that may impact the signal reconstruction. [...]
RESCEU-14/24 ; CERN-TH-2024-170 ; arXiv:2410.10342. - 30.
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2.
Leveraging Time-Dependent Instrumental Noise for LISA SGWB Analysis / Alvey, James (U. Amsterdam, GRAPPA) ; Bhardwaj, Uddipta (U. Amsterdam, GRAPPA ; U. Amsterdam, IHEF) ; Domcke, Valerie (CERN) ; Pieroni, Mauro (CERN) ; Weniger, Christoph (U. Amsterdam, GRAPPA)
Variations in the instrumental noise of the Laser Interferometer Space Antenna (LISA) over time are expected as a result of e.g. [...]
CERN-TH-2024-127 ; arXiv:2408.00832. - 15 p.
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Pulsar timing array sensitivity to anisotropies in the gravitational wave background / Depta, Paul Frederik (Heidelberg, Max Planck Inst.) ; Domcke, Valerie (CERN) ; Franciolini, Gabriele (CERN) ; Pieroni, Mauro (CERN)
Pulsar Timing Array (PTA) observations have recently gathered substantial evidence for the existence of a gravitational wave background in the nHz frequency band. [...]
CERN-TH-2024-116 ; arXiv:2407.14460. - 20 p.
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4.
Gravitational waves from inflation in LISA: reconstruction pipeline and physics interpretation / LISA Cosmology Working Group Collaboration
Various scenarios of cosmic inflation enhance the amplitude of the stochastic gravitational wave background (SGWB) at frequencies detectable by the LISA detector. We develop tools for a template-based analysis of the SGWB and introduce a template databank to describe well-motivated signals from inflation, prototype their template-based searches, and forecast their reconstruction with LISA. [...]
arXiv:2407.04356; LISA-COSWG-24-03; CERN-TH-2024-072.- 2024-11-20 - 82 p. - Published in : JCAP 2411 (2024) 032 Fulltext: PDF;
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5.
Impact of a primordial gravitational wave background on LISA resolvable sources / Braglia, Matteo (New York U., CCPP) ; Pieroni, Mauro (CERN) ; Marsat, Sylvain (L2IT, Toulouse)
The existence of a primordial stochastic gravitational wave background (SGWB) is a common prediction in various models of the early Universe. Despite constraints at different frequency ranges and claims of detection in the nHz range by Pulsar Timing Arrays, the amplitude and spectral dependence of the SGWB in the mHz range remain largely unknown. [...]
arXiv:2406.10048; CERN-TH-2024-073.- 2024-10-15 - 15 p. - Published in : Phys. Rev. D 110 (2024) 083527 Fulltext: 2406.10048 - PDF; Publication - PDF;
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6.
Gravitational waves from cosmic strings in LISA: reconstruction pipeline and physics interpretation / Blanco-Pillado, Jose J. (IKERBASQUE, Bilbao ; Basque U., Bilbao ; U. Basque Country, Leioa) ; Cui, Yanou (UC, Riverside) ; Kuroyanagi, Sachiko (Madrid, IFT ; Nagoya U.) ; Lewicki, Marek (Warsaw U.) ; Nardini, Germano (Stavanger U.) ; Pieroni, Mauro (CERN) ; Rybak, Ivan Yu. (Zaragoza U. ; Porto U., Astron. Dept.) ; Sousa, Lara (Porto U., Astron. Dept.) ; Wachter, Jeremy M. (Wentworth Inst. Tech.)
We initiate the LISA template databank for stochastic gravitational wave backgrounds sourced by cosmic strings. [...]
arXiv:2405.03740 ; LISA-COSWG-24-02 ; CERN-TH-2024-085. - 61 p.
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Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds / Babak, Stanislav (APC, Paris) ; Falxa, Mikel (LPC2E, Orleans ; APC, Paris) ; Franciolini, Gabriele (CERN) ; Pieroni, Mauro (CERN)
Pulsar Timing Array (PTA) observations hinted towards the existence of a stochastic gravitational wave background (SGWB) in the nHz frequency band. Still, the nature of the SGWB signal cannot be confidently inferred from current data, and the leading explanation invokes mergers of supermassive black holes. [...]
arXiv:2404.02864; CERN-TH-2024-039.- 2024-09-11 - 16 p. - Published in : Phys. Rev. D 110 (2024) 063022 Fulltext: Publication - PDF; 2404.02864 - PDF;
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Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation / Caprini, Chiara (Geneva U., Dept. Theor. Phys. ; CERN) ; Jinno, Ryusuke (Tokyo U., RESCEU) ; Lewicki, Marek (Warsaw U.) ; Madge, Eric (Weizmann Inst.) ; Merchand, Marco (Royal Inst. Tech., Stockholm ; Stockholm U., OKC) ; Nardini, Germano (Stavanger U.) ; Pieroni, Mauro (CERN) ; Roper Pol, Alberto (Geneva U., Dept. Theor. Phys.) ; Vaskonen, Ville (INFN, Padua ; INFN, Italy ; Unlisted, EE) /LISA Cosmology Working Group
We develop a tool for the analysis of stochastic gravitational wave backgrounds from cosmological first-order phase transitions with LISA: we initiate a template databank for these signals, prototype their searches, and forecast their reconstruction. The templates encompass the gravitational wave signals sourced by bubble collisions, sound waves and turbulence. [...]
arXiv:2403.03723; LISA-COSWG-24-01; CERN-TH-2024-029.- 2024-10-04 - 54 p. - Published in : JCAP 2410 (2024) 020 Fulltext: document - PDF; 2403.03723 - PDF;
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9.
LISA Definition Study Report / Colpi, Monica (INFN, Milan Bicocca) ; Danzmann, Karsten (Hannover, Max Planck Inst. Grav.) ; Hewitson, Martin (Hannover, Max Planck Inst. Grav.) ; Jetzer, Philippe (U. Zurich (main)) ; Nelemans, Gijs (Nijmegen U., IMAPP) ; Petiteau, Antoine (IRFU, Saclay) ; Shoemaker, David (MIT, MKI) ; Sopuerta, Carlos (ICE, Bellaterra) ; Stebbins, Robin (Colorado U.) ; Tanvir, Nial (Leicester U.) et al.
The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. [...]
arXiv:2402.07571. - 155.
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10.
Probing primordial black holes at high redshift with future gravitational wave detector / Marcoccia, Paolo (Stavanger U.) ; Nardini, Germano (Stavanger U.) ; Pieroni, Mauro (CERN)
We analyze the detection prospects for potential Primordial Black Hole Binary (PBHB) populations buried in the Stellar-Origin Black Hole Binary (SOBHB) population inferred by the LVK collaboration. We consider different PBHB population scenarios and several future Gravitational Wave (GW) detectors. [...]
arXiv:2311.11760; CERN-TH-2023-211.- 2024-06-14 - 32 p. - Published in : Mon. Not. R. Astron. Soc. 531 (2024) 4444-4463 Fulltext: 2311.11760 - PDF; document - PDF;
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CERN Document Server : 19 record trovati   1 - 10successivo  salta al record:
Vedi anche: autori con nomi simili
2 Pieroni, M
2 Pieroni, M.
1 Pieroni, M.P.
1 Pieroni, Mauro,
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