QFT&COSMO

Quantum Field Theory and Cosmology

 Coordinatore FRIEDRICH-SCHILLER-UNIVERSITAT JENA 

 Organization address address: FURSTENGRABEN 1
city: JENA
postcode: 7743

contact info
Titolo: Prof.
Nome: Andreas
Cognome: Wipf
Email: send email
Telefono: -950722
Fax: -950694

 Nazionalità Coordinatore Germany [DE]
 Totale costo 100˙000 €
 EC contributo 100˙000 €
 Programma FP7-PEOPLE
Specific programme "People" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call FP7-PEOPLE-2009-RG
 Funding Scheme MC-IRG
 Anno di inizio 2009
 Periodo (anno-mese-giorno) 2009-12-15   -   2013-12-14

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    FRIEDRICH-SCHILLER-UNIVERSITAT JENA

 Organization address address: FURSTENGRABEN 1
city: JENA
postcode: 7743

contact info
Titolo: Prof.
Nome: Andreas
Cognome: Wipf
Email: send email
Telefono: -950722
Fax: -950694

DE (JENA) coordinator 100˙000.00

Mappa


 Word cloud

Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.

he    scalars    conformally    cosmology    mmc    coupled    particle    time    equations    higgs    inflaton    corrected    quantum    going    models    inflation    guide    gravity    modified   

 Obiettivo del progetto (Objective)

Dr. Kahya will undertake research in Quantum Field Theory and Cosmology. He will investigate four research topics in the project. Topic I: Quantum Corrected Field Equations of Conformally Coupled Scalars He aims to solve the quantum corrected linearized effective field equations of conformally coupled scalars during Inflation. Topic II: Is the Standard Model Higgs really the Inflaton? He is going to investigate the quantum effects during Inflation on Higgs particle and check whether it can be the Inflaton particle. Topic III: Stochastic Formulation of Massless Minimally Coupled (MMC) Scalars during Inflation He aims to extend Starobisky's nonperturbative resummation technique to MMC scalars coupled to gravity and to explore the consequences for late time cosmology. Topic IV: A guide for GW detectors to test the Modified Gravity Models He proposes to produce a rough graph of the time lag of gravitational waves vs. photons/neutrinos as a function of position in the Milky Way-Andromeda neighborhood which could serve as a guide for observers. It is going to be done in the context of models where gravity is modified to do away with dark matter.

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