[물리천문학과] 콜로퀴움 전문가 초청 특강

  • 전체 학생/대학원생
  • 전체 학년/전체 성별
  • 전체 학과
  • phydpt@sejong.ac.kr
  • 02-3408-3316
  • 영실관 601호
전문가 초청 특강을 통한 다양한 지식의 습득과 학부생들과 대학원생들의 자발적이고 활발한 질의응답시간을 기대합니다.
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물리천문학과 콜로퀴움


‧강연 제목 : Exploring Cosmic Tensions and Beyond: A model-independent approach 

‧연사 : 한국천문연구원 RODRIGO CALDERÓN 

‧일시 : 2023년 11월 15일 (수요일) 17:00~18:30

‧진행 방법 : 영실관 601호

‧신청 가능 대상 : 세종대학교 재학생 누구나

‧신청기간 : 11월 14일 ~ 11월15일


‧강의 초록

Cosmology has entered an era of unprecedented precision, with an abundance of high-quality observational data. However, the increasing accuracy of measurements has unveiled tensions among different cosmological probes, potentially hinting at new physics or systematic uncertainties. This talk presents a powerful model-independent approach to look for new physics and systematics in the measurements.

In the first part of my talk, I will focus on the most recent measurements of the cosmic microwave background (CMB) by the Planck, ACT, and SPT collaborations.  We will explore the internal consistency of the different CMB experiments and show that despite the overall agreement with the standard model predictions, there are still some indications of mild discrepancies between them. I will summarize some of the key results in our non-parametric analysis, and discuss some implications for model building.

In the second part of my talk, I will forecast the upcoming surveys’ capability to reconstruct the time-dependence of the phenomenological functions that describe the departures from LCDM, in a data-driven manner. We use forward-modeling and Gaussian Processes to reconstruct the Universe’s growth and expansion histories jointly and show that, in General Relativity, stage IV surveys can successfully distinguish various dark energy models from LCDM with high significance. In addition, we show that forthcoming surveys such as DESI can also detect deviations from general relativity if the dark energy behavior is accurately determined. I will also show how incorrectly assuming a LCDM expansion history naturally leads to severely biased inferences of the matter density and amplitude of fluctuations today.

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  • [물리천문학과] 콜로퀴움 전문가 초청 특강

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