%0 Generic %1 pruett2022primordial %A Pruett, K. %A Dawson, W. %A Medford, M. S. %A Lam, C. %A Lu, J. R. %A Golovich, N. %A Chapline, G. %D 2022 %K library %T Primordial Black Hole Dark Matter Simulations Using PopSyCLE %U http://arxiv.org/abs/2211.06771 %X Primordial black holes (PBHs), theorized to have originated in the early universe, are speculated to be a viable form of dark matter. If they exist, they should be detectable through photometric and astrometric signals resulting from gravitational microlensing of stars in the Milky Way. Population Synthesis for Compact-object Lensing Events, or PopSyCLE, is a simulation code that enables users to simulate microlensing surveys, and is the first of its kind to include both photometric and astrometric microlensing effects, which are important for potential PBH detection and characterization. To estimate the number of observable PBH microlensing events we modify PopSyCLE to include a dark matter halo consisting of PBHs. We detail our PBH population model, and demonstrate our PopSyCLE + PBH results through simulations of the OGLE-IV and Roman microlensing surveys. We provide a proof-of-concept analysis for adding PBHs into PopSyCLE, and thus include many simplifying assumptions, such as $f_DM$, the fraction of dark matter composed of PBHs, and $m_PBH$, mean PBH mass. Assuming $m_PBH=30$ $M_ødot$, we find $\sim$4$f_DM$ times as many PBH microlensing events than stellar evolved black hole events, a PBH average peak Einstein crossing time of $\sim$89 days, and estimate Roman to detect on the order of $10^3f_DM$ PBH microlensing events throughout its planned microlensing survey.

@misc{pruett2022primordial, abstract = {Primordial black holes (PBHs), theorized to have originated in the early universe, are speculated to be a viable form of dark matter. If they exist, they should be detectable through photometric and astrometric signals resulting from gravitational microlensing of stars in the Milky Way. Population Synthesis for Compact-object Lensing Events, or PopSyCLE, is a simulation code that enables users to simulate microlensing surveys, and is the first of its kind to include both photometric and astrometric microlensing effects, which are important for potential PBH detection and characterization. To estimate the number of observable PBH microlensing events we modify PopSyCLE to include a dark matter halo consisting of PBHs. We detail our PBH population model, and demonstrate our PopSyCLE + PBH results through simulations of the OGLE-IV and Roman microlensing surveys. We provide a proof-of-concept analysis for adding PBHs into PopSyCLE, and thus include many simplifying assumptions, such as $f_{\text{DM}}$, the fraction of dark matter composed of PBHs, and $\bar{m}_{\text{PBH}}$, mean PBH mass. Assuming $\bar{m}_{\text{PBH}}=30$ $M_{\odot}$, we find $\sim$4$f_{\text{DM}}$ times as many PBH microlensing events than stellar evolved black hole events, a PBH average peak Einstein crossing time of $\sim$89 days, and estimate Roman to detect on the order of $10^3f_{\text{DM}}$ PBH microlensing events throughout its planned microlensing survey.}, added-at = {2022-11-15T11:25:24.000+0100}, author = {Pruett, K. and Dawson, W. and Medford, M. S. and Lam, C. and Lu, J. R. and Golovich, N. and Chapline, G.}, biburl = {https://www.bibsonomy.org/bibtex/2a3d41390611857785f4820a8f2cca86c/gpkulkarni}, description = {Primordial Black Hole Dark Matter Simulations Using PopSyCLE}, interhash = {84e1dfe4755fc70109ac3e819fec727a}, intrahash = {a3d41390611857785f4820a8f2cca86c}, keywords = {library}, note = {cite arxiv:2211.06771}, timestamp = {2022-11-15T11:25:24.000+0100}, title = {Primordial Black Hole Dark Matter Simulations Using PopSyCLE}, url = {http://arxiv.org/abs/2211.06771}, year = 2022 }