{"title":"How Does the Quantum Structure of Electromagnetic Waves Describe Dark Matter?","authors":"Bahram Kalhor, Farzaneh Mehrparvar, Behnam Kalhor","doi":"10.2139/ssrn.3730715","DOIUrl":"https://doi.org/10.2139/ssrn.3730715","url":null,"abstract":"Dark matter is a kind of matter that we cannot see directly. Scientists have detected dark matter by analyzing the relationship between mass and velocity of the stars in galaxies. The higher speed of the stars implies more mass in the galaxies. However, they cannot describe it and its behavior clearly. Here we show that faster conversion of the dark matters spectrum to the Cosmic Microwave Background (CMB) is the reason why they are hidden. We found that observers out of the 72 light-years of dark matters do not receive their light. Hence, an emitter could be visible for nearby observers, while more distance observers might detect it as a dark matter.","PeriodicalId":122228,"journal":{"name":"PlanetSciRN: Dark Matter & Dark Energy (Topic)","volume":"119 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2020-11-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"115601397","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Challenges in Detection of Dark Matter Candidates","authors":"Rakesh Sharma, G. K. Upadhyaya, S. Sharma","doi":"10.2139/ssrn.3449960","DOIUrl":"https://doi.org/10.2139/ssrn.3449960","url":null,"abstract":"The challenge for search of dark matter reached a new stage and the theorists and experimentalists in the field are still struggling to find an absolute signature of the dark matter candidates of any species by direct or indirect methods of detection. Many mathematical formulations and ideas were proposed but till today the results are negative. Various experimentalist groups and theorist groups of the field are making ceaseless efforts to take the research to its high level but there is something missing in their work. In the present paper we examine why any of dark matter candidates are not detectable in the detectors either by direct or indirect techniques and what will be the most suitable candidates to be detected in near future on the machines. Rindler’s coordinates are also examined to understand dynamics of normal matter with coexistence of dark matter. The Cosmic Microwave Background (CMB) simulator is also produced here in suggestion for existence of dark matter in our universe.","PeriodicalId":122228,"journal":{"name":"PlanetSciRN: Dark Matter & Dark Energy (Topic)","volume":"104 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2019-09-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"132977612","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}