Elliptic Flow of Light Nuclei in Au+Au Collisions at $$\sqrt{s_{NN}}$$ = 14.6, 19.6, 27, and 54.4 GeV Using the STAR Detector

Sharma, Rishabh; ,

doi:10.1007/978-981-97-0289-3_32

Springer Proceedings in Physics

2024

DOI: 10.1007/978-981-97-0289-3_32

|View full text |Cite

Elliptic Flow of Light Nuclei in Au+Au Collisions at $$\sqrt{s_{NN}}$$ = 14.6, 19.6, 27, and 54.4 GeV Using the STAR Detector

Rishabh Sharma

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...

Citation Types

Supporting

Mentioning

Contrasting

Publication Types

Select...

Relationship

Self Cite0

Independent0

Authors

Journals

Cited by 0 publications

References 23 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

No citations

Set email alert for when this publication receives citations?

scite is a Brooklyn-based organization that helps researchers better discover and understand research articles through Smart Citations–citations that display the context of the citation and describe whether the article provides supporting or contrasting evidence. scite is used by students and researchers from around the world and is funded in part by the National Science Foundation and the National Institute on Drug Abuse of the National Institutes of Health.

Contact Info

customersupport@researchsolutions.com

10624 S. Eastern Ave., Ste. A-614

Henderson, NV 89052, USA

This site is protected by reCAPTCHA and the Google Privacy Policy and Terms of Service apply.

Blog Terms and Conditions API Terms Privacy Policy Contact Cookie Preferences Do Not Sell or Share My Personal Information

Made with 💙 for researchers

Part of the Research Solutions Family.

Elliptic Flow of Light Nuclei in Au+Au Collisions at $$\sqrt{s_{NN}}$$ = 14.6, 19.6, 27, and 54.4 GeV Using the STAR Detector

Cited by 0 publications

References 23 publications

No citations

Contact Info

Product

Resources

About